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0704.3901
Stefan Kr\"omer
Stefan Kr\"omer
Existence and symmetry of minimizers for nonconvex radially symmetric variational problems
22 pages, submitted to Calculus of Variations and Partial Differential Equations
null
null
null
math.CA
null
Nonconvex functionals with spherical symmetry are studied. Existence of one and radial symmetry of all global minimizers is shown with an approach based on convex relaxation.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 09:12:59 GMT" } ]
2007-05-23T00:00:00
[ [ "Krömer", "Stefan", "" ] ]
0704.3902
Yuri Yakubovich
Alexander Gnedin, Yuri Yakubovich
On the number of collisions in $\Lambda$-coalescents
18 pages
null
null
null
math.PR
null
We examine the total number of collisions $C_n$ in the $\Lambda$-coalescent process which starts with $n$ particles. A linear growth and a stable limit law for $C_n$ are shown under the assumption of a power-like behaviour of the measure $\Lambda$ near 0 with exponent $0<\alpha<1$.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 09:16:35 GMT" } ]
2007-05-23T00:00:00
[ [ "Gnedin", "Alexander", "" ], [ "Yakubovich", "Yuri", "" ] ]
0704.3903
Koji Chinen
Koji Chinen
An abundance of invariant polynomials satisfying the Riemann hypothesis
19 pages
null
null
null
math.NT
null
In 1999, Iwan Duursma defined the zeta function for a linear code as a generating function of its Hamming weight enumerator. It can also be defined for other homogeneous polynomials not corresponding to existing codes. If the homogeneous polynomial is invariant under the MacWilliams transform, then its zeta function satisfies a functional equation and we can formulate an analogue of the Riemann hypothesis. As far as existing codes are concerned, the Riemann hypothesis is believed to be closely related to the extremal property. In this article, we show there are abundant polynomials invariant by the MacWilliams transform which satisfy the Riemann hypothesis. The proof is carried out by explicit construction of such polynomials. To prove the Riemann hypothesis for a certain class of invariant polynomials, we establish an analogue of the Enestr"om-Kakeya theorem.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 09:17:42 GMT" } ]
2007-05-23T00:00:00
[ [ "Chinen", "Koji", "" ] ]
0704.3904
Fabien Mathieu
Anh-Tuan Gai (INRIA Rocquencourt), Dmitry Lebedev (FT R&D), Fabien Mathieu (FT R&D), Fabien De Montgolfier (LIAFA), Julien Reynier (LIENS), Laurent Viennot (INRIA Rocquencourt)
Acyclic Preference Systems in P2P Networks
null
null
null
null
cs.DS cs.GT
null
In this work we study preference systems natural for the Peer-to-Peer paradigm. Most of them fall in three categories: global, symmetric and complementary. All these systems share an acyclicity property. As a consequence, they admit a stable (or Pareto efficient) configuration, where no participant can collaborate with better partners than their current ones. We analyze the representation of the such preference systems and show that any acyclic system can be represented with a symmetric mark matrix. This gives a method to merge acyclic preference systems and retain the acyclicity. We also consider such properties of the corresponding collaboration graph, as clustering coefficient and diameter. In particular, studying the example of preferences based on real latency measurements, we observe that its stable configuration is a small-world graph.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 09:26:39 GMT" }, { "version": "v2", "created": "Wed, 2 May 2007 13:07:31 GMT" } ]
2007-05-23T00:00:00
[ [ "Gai", "Anh-Tuan", "", "INRIA Rocquencourt" ], [ "Lebedev", "Dmitry", "", "FT R&D" ], [ "Mathieu", "Fabien", "", "FT R&D" ], [ "De Montgolfier", "Fabien", "", "LIAFA" ], [ "Reynier", "Julien", "", "LIENS" ], [ "Viennot", "Laurent", "", "INRIA Rocquencourt" ] ]
0704.3905
Marc Schoenauer
Christian Gagn\'e (INFORMATIQUE WGZ INC.), Mich\`ele Sebag (INRIA Futurs), Marc Schoenauer (INRIA Futurs), Marco Tomassini (ISI)
Ensemble Learning for Free with Evolutionary Algorithms ?
null
Dans GECCO (2007)
null
null
cs.AI
null
Evolutionary Learning proceeds by evolving a population of classifiers, from which it generally returns (with some notable exceptions) the single best-of-run classifier as final result. In the meanwhile, Ensemble Learning, one of the most efficient approaches in supervised Machine Learning for the last decade, proceeds by building a population of diverse classifiers. Ensemble Learning with Evolutionary Computation thus receives increasing attention. The Evolutionary Ensemble Learning (EEL) approach presented in this paper features two contributions. First, a new fitness function, inspired by co-evolution and enforcing the classifier diversity, is presented. Further, a new selection criterion based on the classification margin is proposed. This criterion is used to extract the classifier ensemble from the final population only (Off-line) or incrementally along evolution (On-line). Experiments on a set of benchmark problems show that Off-line outperforms single-hypothesis evolutionary learning and state-of-art Boosting and generates smaller classifier ensembles.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 09:29:22 GMT" } ]
2007-05-23T00:00:00
[ [ "Gagné", "Christian", "", "INFORMATIQUE WGZ INC." ], [ "Sebag", "Michèle", "", "INRIA\n Futurs" ], [ "Schoenauer", "Marc", "", "INRIA Futurs" ], [ "Tomassini", "Marco", "", "ISI" ] ]
0704.3906
Michael M. Wolf
M.M. Wolf, F. Verstraete, M.B. Hastings, J.I. Cirac
Area laws in quantum systems: mutual information and correlations
5 pages, 2 figures, published version with appendix
Phys. Rev. Lett. 100, 070502 (2008)
10.1103/PhysRevLett.100.070502
null
quant-ph cond-mat.stat-mech
null
The holographic principle states that on a fundamental level the information content of a region should depend on its surface area rather than on its volume. This counterintuitive idea which has its roots in the nonextensive nature of black-hole entropy serves as a guiding principle in the search for the fundamental laws of Planck-scale physics. In this paper we show that a similar phenomenon emerges from the established laws of classical and quantum physics: the information contained in part of a system in thermal equilibrium obeys an area law. While the maximal information per unit area depends classically only on the number of microscopic degrees of freedom, it may diverge as the inverse temperature in quantum systems. A rigorous relation between area laws and correlations is established and their explicit behavior is revealed for a large class of quantum many-body states beyond equilibrium systems.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 09:36:44 GMT" }, { "version": "v2", "created": "Mon, 10 Mar 2008 18:24:31 GMT" } ]
2009-11-13T00:00:00
[ [ "Wolf", "M. M.", "" ], [ "Verstraete", "F.", "" ], [ "Hastings", "M. B.", "" ], [ "Cirac", "J. I.", "" ] ]
0704.3907
Lucas Lamata
Lucas Lamata
Developments in entanglement theory and applications to relevant physical systems
Ph.D. Thesis, April 2007, Universidad Autonoma de Madrid
null
null
null
quant-ph
null
This Thesis is devoted to the analysis of entanglement in relevant physical systems. Entanglement is the conducting theme of this research, though I do not dedicate to a single topic, but consider a wide scope of physical situations. I have followed mainly three lines of research for this Thesis, with a series of different works each, which are, Entanglement and Relativistic Quantum Theory, Continuous-variable entanglement, and Multipartite entanglement.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 09:37:41 GMT" } ]
2007-05-23T00:00:00
[ [ "Lamata", "Lucas", "" ] ]
0704.3908
Margarita Sharina
M.E. Sharina (SAO RAS), Th.H. Puzia (Herzberg Institute of Astrophysics), A.S. Krylatyh (Kazan State University)
A globular cluster in the dwarf galaxy Sextans B
13 pages, 4 figures, 3 tables, Astrophysical Bulletin, accepted
null
10.1134/S1990341307030029
null
astro-ph
null
We present spectroscopic observations of a massive globular cluster in the dwarf irregular galaxy Sextans B, discovered by us on Hubble Space Telescope Wide Field and Planetary Camera 2 (HST WFPC2) images. Long-slit spectra were obtained with the SCORPIO spectrograph on the the 6-m telescope at the Special Astrophysical observatory of the Russian Academy of Sciences. We determine age, metallicity and alpha-element abundance ratio for the globular cluster to be $ 2 \pm 1$ Gyr, $-1.35 \pm 0.25$ dex, and $ 0.1 \pm 0.1$ dex, respectively. Main photometric and structural parameters of it were determined using our surface photometry on the HST images. The mass ($\sim 10^5 M \sun$), luminosity and structural parameters appear to be typical for the globular clusters in our own Galaxy. Our findings shed a new light on the evolutionary history of Sextans B.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 10:05:55 GMT" } ]
2009-11-13T00:00:00
[ [ "Sharina", "M. E.", "", "SAO RAS" ], [ "Puzia", "Th. H.", "", "Herzberg Institute of\n Astrophysics" ], [ "Krylatyh", "A. S.", "", "Kazan State University" ] ]
0704.3909
Natalia Panikashvili
D0 Collaboration: V. Abazov, et al
Measurement of the Lambda_b lifetime in the exclusive decay Lambda_b to J/psi Lambda
This version has been accepted for publication in Physical Review Letters
Phys.Rev.Lett.99:142001,2007
10.1103/PhysRevLett.99.142001
FERMILAB-PUB-07/094-E
hep-ex
null
We have measured the Lambda_b lifetime using the exclusive decay Lambda_b to J/psi Lambda, based on 1.2 fb-1 of data collected with the D0 detector during 2002-2006. From 171 reconstructed Lambda_b decays, where the J/psi and Lambda are identified via the decays J/psi to mu+ mu- and Lambda to p pi, we measured the Lambda_b lifetime to be tau(Lambda_b) = 1.218(+0.130,-0.115)(stat) +/- 0.042(syst)ps. We also measured the B0 lifetime in the decay B0 to J/psi(mu+ mu-)K0_S(pi+ pi-) to be tau(B0) = 1.501(+0.078,-0.074)(stat) +/ -0.050(syst)ps, yielding a lifetime ratio of tau(Lambda_b)/tau(B0) = 0.811(+0.096,-0.087)(stat) +/ -0.034(syst). These measurements are consistent with the current world averages and support the shorter lifetime of the Lambda_b with respect to B mesons, in contrast to another recent measurement of significant precision.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 09:44:44 GMT" }, { "version": "v2", "created": "Thu, 30 Aug 2007 08:39:17 GMT" } ]
2008-11-26T00:00:00
[ [ "D0 Collaboration", "", "" ], [ "Abazov", "V.", "" ] ]
0704.3910
Guillaume Dubus
P. d'Avezac, G. Dubus, B. Giebels
Cascading on extragalactic background light
5 pages, to be published as a research note in A&A
Astron.Astrophys.469:857-860,2007
10.1051/0004-6361:20066712
null
astro-ph
null
High-energy gamma-rays propagating in the intergalactic medium can interact with background infrared photons to produce e+e- pairs, resulting in the absorption of the intrinsic gamma-ray spectrum. TeV observations of the distant blazar 1ES 1101-232 were thus recently used to put an upper limit on the infrared extragalactic background light density. The created pairs can upscatter background photons to high energies, which in turn may pair produce, thereby initiating a cascade. The pairs diffuse on the extragalactic magnetic field (EMF) and cascade emission has been suggested as a means for measuring its intensity. Limits on the IR background and EMF are reconsidered taking into account cascade emissions. The cascade equations are solved numerically. Assuming a power-law intrinsic spectrum, the observed 100 MeV - 100 TeV spectrum is found as a function of the intrinsic spectral index and the intensity of the EMF. Cascades emit mainly at or below 100 GeV. The observed TeV spectrum appears softer than for pure absorption when cascade emission is taken into account. The upper limit on the IR photon background is found to be robust. Inversely, the intrinsic spectra needed to fit the TeV data are uncomfortably hard when cascade emission makes a significant contribution to the observed spectrum. An EMF intensity around 1e-8 nG leads to a characteristic spectral hump in the GLAST band. Higher EMF intensities divert the pairs away from the line-of-sight and the cascade contribution to the spectrum becomes negligible.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 09:55:01 GMT" } ]
2009-06-23T00:00:00
[ [ "d'Avezac", "P.", "" ], [ "Dubus", "G.", "" ], [ "Giebels", "B.", "" ] ]
0704.3911
Robinson Edward Raja Chandiraraj
C. R. E. Raja
Distal actions and ergodic actions on compact groups
null
null
null
null
math.DS
null
Let $K$ be a compact metrizable group and $\Ga$ be a group of automorphisms of $K$. We first show that each $\ap \in \Ga$ is distal on $K$ implies $\Ga$ itself is distal on $K$, a local to global correspondence provided $\Ga$ is a generalized $\ov{FC}$-group or $K$ is a connected finite-dimensional group. We show that $\Ga$ contains an ergodic automorphism when $\Ga$ is nilpotent and ergodic on a connected finite-dimensional compact abelian group $K$.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 09:55:50 GMT" } ]
2007-05-23T00:00:00
[ [ "Raja", "C. R. E.", "" ] ]
0704.3912
Cinzia Casagrande
C. Casagrande
Quasi elementary contractions of Fano manifolds
Final version, minor changes, to appear in Compositio Mathematica
null
null
null
math.AG
null
Let X be a smooth complex Fano variety. We define and study 'quasi elementary' contractions of fiber type f: X -> Y. These have the property that rho(X) is at most rho(Y)+rho(F), where rho is the Picard number and F is a general fiber of f. In particular any elementary extremal contraction of fiber type is quasi elementary. We show that if Y has dimension at most 3 and Picard number at least 4, then Y is smooth and Fano; if moreover rho(Y) is at least 6, then X is a product. This yields sharp bounds on rho(X) when dim(X)=4 and X has a quasi elementary contraction, and other applications in higher dimensions.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 10:09:24 GMT" }, { "version": "v2", "created": "Fri, 18 Apr 2008 11:10:39 GMT" } ]
2008-04-18T00:00:00
[ [ "Casagrande", "C.", "" ] ]
0704.3913
Wei-shui Xu
Yi-hong Gao, Jonathan P. Shock, Wei-shui Xu and Ding-fang Zeng
A Note on Chiral Symmetry Breaking from Intersecting Branes
16 pp, minor changes, to appear PRD
Phys.Rev.D76:046003,2007
10.1103/PhysRevD.76.046003
null
hep-th
null
In this paper, we will consider the chiral symmetry breaking in the holographic model constructed from the intersecting brane configuration, and investigate the Nambu-Goldstone bosons associated with this symmetry breaking.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 10:43:35 GMT" }, { "version": "v2", "created": "Tue, 12 Jun 2007 16:55:17 GMT" }, { "version": "v3", "created": "Wed, 1 Aug 2007 12:23:48 GMT" } ]
2008-11-26T00:00:00
[ [ "Gao", "Yi-hong", "" ], [ "Shock", "Jonathan P.", "" ], [ "Xu", "Wei-shui", "" ], [ "Zeng", "Ding-fang", "" ] ]
0704.3914
Nigel Glover
S. D. Badger (Saclay, SPhT), E. W. N. Glover (IPPP, Durham U.), Kasper Risager (Bohr Inst.)
One-loop phi-MHV amplitudes using the unitarity bootstrap
40 pages, 11 eps figures, JHEP3 class, references added
JHEP 0707:066,2007
10.1088/1126-6708/2007/07/066
IPPP/07/12, SACLAY-SPHT-T07/044
hep-ph
null
We consider a Higgs boson coupled to gluons via the five-dimensional effective operator H Tr G_{munu}G^{munu} produced by considering the heavy top quark limit of the one-loop coupling of Higgs and gluons in the standard model. We treat H as the real part of a complex field phi that couples to the selfdual gluon field strengths and compute the one-loop corrections to amplitudes involving phi, two colour adjacent negative helicity gluons and an arbitrary number of positive helicity gluons - the so-called phi-MHV amplitudes. We use four-dimensional unitarity to construct the cut-containing contributions and the recently developed recursion relations to obtain the rational contribution for an arbitrary number of external gluons. We solve the recursion relations and give explicit results for up to four external gluons. These amplitudes are relevant for Higgs plus jet production via gluon fusion in the limit where the top quark mass is large compared to all other scales in the problem.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 10:49:31 GMT" }, { "version": "v2", "created": "Mon, 11 Jun 2007 08:26:56 GMT" }, { "version": "v3", "created": "Mon, 2 Jul 2007 21:36:42 GMT" } ]
2009-04-21T00:00:00
[ [ "Badger", "S. D.", "", "Saclay, SPhT" ], [ "Glover", "E. W. N.", "", "IPPP, Durham U." ], [ "Risager", "Kasper", "", "Bohr Inst." ] ]
0704.3915
Andrea Borch
Andrea Borch, Rainer Spurzem, Jarrod Hurley
NBODY meets stellar population - The HYDE-PARC Project
21 pages. submitted to A&A
null
null
null
astro-ph
null
N-body simulations give us a rough idea of how the shape of a simulated object appears in three-dimensional space. From an observational point of view this may give us a misleading picture. The faint stars may be the most common stars in the system but the morphological information obtained by observations of an object may be dominated by the color properties of the bright stars. Due to dynamical effects, such as energy equipartition, different masses of stars may populate different regions in the object. Since stars are evolving in mass the stellar evolution may also influence the dynamics of the system. Hence, if one is interested in simulating what the morphology will look like through a telescope, one needs to simulate in addition evolving stars and weight them by their luminosity. Therefore we need to combine simulations of the dynamical evolution and a stellar population synthesis at the same time. For the dynamical evolution part we use a parallel version of a direct N-body code, NBODY6++. This code also includes stellar evolution. We link the parameters from this stellar evolution routine to the BaSeL 2.0 stellar library. For isolated clusters we found results assimilable to standard stellar population synthesis codes such as the PEGASE code. For clusters in a tidal field we found that the integrated colors become relatively bluer due to energy equipartition effects. In the time shortly before dissolution of the cluster the stellar M/L ratio becomes lower compared to isolated clusters. We compared the results of our simulations to integrated spectra of galactic globular clusters. For the cluster NGC 1851 we found good agreement between simulation and observation. For extragalactic clusters in M81 and M31 we looked at medium band spectral energy distributions and found for some clusters also a good agreement.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 10:48:37 GMT" } ]
2007-05-23T00:00:00
[ [ "Borch", "Andrea", "" ], [ "Spurzem", "Rainer", "" ], [ "Hurley", "Jarrod", "" ] ]
0704.3916
Outi Elina Maasalo
Outi Elina Maasalo
The Gehring Lemma in Metric Spaces
16 pages; typos corrected
null
null
null
math.CA math.AP
null
We present a proof for the Gehring lemma in a metric measure space endowed with a doubling measure. As an application we show the self improving property of Muckenhoupt weights.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 10:57:09 GMT" }, { "version": "v2", "created": "Fri, 24 Aug 2007 07:58:51 GMT" }, { "version": "v3", "created": "Tue, 15 Jan 2008 12:39:15 GMT" } ]
2008-01-15T00:00:00
[ [ "Maasalo", "Outi Elina", "" ] ]
0704.3917
Maria Vittoria Garzelli
M.V. Garzelli
A fully microscopical simulation of nuclear collisions by a new QMD model
5 pages, 7 figures. Talk presented at ND2007, International Conference on Nuclear Data for Science and Technology, Nice, France, April 22 - 27 2007
Proceedings of ND2007, International Conference of Nuclear Data for Science and Technology, editors O. Bersillon, F. Gunsing, E. Bauge, R. Jacqmin and S. Leray, EDP Sciences (2008), 1129 - 1132
10.1051/ndata:07673
null
nucl-th
null
Nucleon-ion and ion-ion collisions at non relativistic bombarding energies can be described by means of Monte Carlo approaches, such as those based on the Quantum Molecular Dynamics (QMD) model. We have developed a QMD code, to simulate the fast stage of heavy-ion reactions, and we have coupled it to the de-excitation module available in the FLUKA Monte Carlo transport and interaction code. The results presented in this work span the projectile bombarding energy range within 200 - 600 MeV/A, allowing to investigate the capabilities and limits of our non-relativistic QMD approach.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 11:55:10 GMT" } ]
2008-09-14T00:00:00
[ [ "Garzelli", "M. V.", "" ] ]
0704.3918
Antoine Van Proeyen
Kostas Skenderis, Paul K. Townsend and Antoine Van Proeyen
Domain-wall/Cosmology correspondence in adS/dS supergravity
21 pages;v2: rewritten to clarify the link with fake supergravity -- main results unchanged; v3: typos corrected, two refs added, JHEP version
JHEP0708:036,2007
10.1088/1126-6708/2007/08/036
DAMTP-2007-40, ITFA-2007-16, KUL-TF-07/09
hep-th
null
We realize the domain-wall/cosmology correspondence for (pseudo)supersymmetric domain walls (cosmologies) in the context of four-dimensional supergravity. The OSp(2|4)-invariant anti-de Sitter (adS) vacuum of a particular N=2 Maxwell-Einstein supergravity theory is shown to correspond to the OSp(2^*|2,2)-invariant de Sitter (dS) vacuum of a particular pseudo-supergravity model, with `twisted' reality conditions on spinors. More generally, supersymmetric domain walls of the former model correspond to pseudo-supersymmetric cosmologies of the latter model, with time-dependent pseudo-Killing spinors that we give explicitly.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 19:58:39 GMT" }, { "version": "v2", "created": "Tue, 26 Jun 2007 10:05:16 GMT" }, { "version": "v3", "created": "Tue, 14 Aug 2007 19:25:01 GMT" } ]
2010-02-17T00:00:00
[ [ "Skenderis", "Kostas", "" ], [ "Townsend", "Paul K.", "" ], [ "Van Proeyen", "Antoine", "" ] ]
0704.3919
Andria Rogava
Andria Rogava, Grigol Gogoberidze and Stefaan Poedts
On over-reflection and generation of Gravito-Alfven waves in solar-type stars
20 pages (preprint format), 4 figures; to appear in The Astrophysical Journal (August 1, 2007, v664, N2 issue)
Astrophys.J.664:1221-1227,2007
10.1086/518824
null
astro-ph
null
The dynamics of linear perturbations is studied in magnetized plasma shear flows with a constant shearing rate and with gravity-induced stratification. The general set of linearized equations is derived and the two-dimensional case is considered in detail. The Boussinesq approximation is used in order to examine relatively small-scale perturbations of low-frequency modes: Gravito-Alfven waves (GAW) and Entropy Mode (EM) perturbations. It is shown that for flows with arbitrary shearing rate there exists a finite time interval of non-adiabatic evolution of the perturbations. The non-adiabatic behavior manifests itself in a twofold way, viz. by the over-reflection of the GAWs and by the generation of GAWs from EM perturbations. It is shown that these phenomena act as efficient transformers of the equilibrium flow energy into the energy of the perturbations for moderate and high shearing rate solar plasma flows. Efficient generation of GAW by EM takes place for shearing rates about an order of magnitude smaller than necessary for development of a shear instability. The latter fact could have important consequences for the problem of angular momentum redistribution within the Sun and solar-type stars.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 11:38:22 GMT" } ]
2009-06-23T00:00:00
[ [ "Rogava", "Andria", "" ], [ "Gogoberidze", "Grigol", "" ], [ "Poedts", "Stefaan", "" ] ]
0704.3920
Seong Chan Park
Seong Chan Park (Seoul National University)
Orbifold GUT inflation
12 pages, 6 figures, JCAP accepted version
JCAP0711:001,2007
10.1088/1475-7516/2007/11/001
null
hep-th astro-ph gr-qc hep-ph
null
We consider a scenario of cosmological inflation coming from a grand unified theory in higher dimensional orbifold. Flatness of the potential is automatically guaranteed in this orbifold setup thanks to the nonlocality of the Wilson line on higher dimensions and the local quantum gravitational corrections are exponentially suppressed. The spectral index of scalar perturbation (n_s =0.92 - 0.97) and a significant production of gravitational waves are predicted (r= T/S= 0.01 - 0.12) in the perturbative regime of gauge interaction, (1/g_4 = (5-20) X 2 pi R Mpl) where the size of compactification is constrained (R Mpl = 20- 45) by the measurement of scalar power spectrum (Delta_R = 5 X 10^-5).
[ { "version": "v1", "created": "Mon, 30 Apr 2007 12:17:25 GMT" }, { "version": "v2", "created": "Wed, 17 Oct 2007 16:53:47 GMT" } ]
2008-11-26T00:00:00
[ [ "Park", "Seong Chan", "", "Seoul National University" ] ]
0704.3921
Li Ma
Li Ma, Lin Zhao
Sharp thresholds of blow-up and global existence for the coupled nonlinear Schrodinger system
21 pages
null
10.1063/1.2939238
null
math.AP math.DG
null
In this paper, we establish two new types of invariant sets for the coupled nonlinear Schrodinger system on $\mathbb{R}^n$, and derive two sharp thresholds of blow-up and global existence for its solution. Some analogous results for the nonlinear Schrodinger system posed on the hyperbolic space $\mathbb{H}^n$ and on the standard 2-sphere $\mathbb{S}^2$ are also presented. Our arguments and constructions are improvements of some previous works on this direction. At the end, we give some heuristic analysis about the strong instability of the solitary waves.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 12:03:03 GMT" } ]
2009-11-13T00:00:00
[ [ "Ma", "Li", "" ], [ "Zhao", "Lin", "" ] ]
0704.3922
Nicolas Fournier
Nicolas Fournier
Smoothness of the law of some one-dimensional jumping S.D.E.s with non-constant rate of jump
null
null
null
null
math.PR
null
We consider a one-dimensional jumping Markov process $\{X^x_t\}_{t \geq 0}$, solving a Poisson-driven stochastic differential equation. We prove that the law of $X^x_t$ admits a smooth density for $t>0$, under some regularity and non-degeneracy assumptions on the coefficients of the S.D.E. To our knowledge, our result is the first one including the important case of a non-constant rate of jump. The main difficulty is that in such a case, the map $x \mapsto X^x_t$ is not smooth. This seems to make impossible the use of Malliavin calculus techniques. To overcome this problem, we introduce a new method, in which the propagation of the smoothness of the density is obtained by analytic arguments.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 12:05:21 GMT" } ]
2007-05-23T00:00:00
[ [ "Fournier", "Nicolas", "" ] ]
0704.3923
Prabuddha Sanyal
Prabuddha Sanyal, Subhra Sen Gupta, Nandan Pakhira, H. R. Krishnamurthy, D. D. Sarma and T. V. Ramakrishnan
Unusual doping and temperature dependence of photoemission spectra from manganites
5 pages, 3 figures
null
10.1209/0295-5075/82/47010
null
cond-mat.str-el cond-mat.mtrl-sci
null
A recent, major, puzzle in the core-level photoemission spectra of doped manganites is the observation of a 1-2 eV wide shoulder with intensity varying with temperature T as the square of the magnetization over a T scale of order 200K, an order of magnitude less than electronic energies. This is addressed and resolved here, by extending a recently proposed two electron fluid l-b model for these systems to include core-hole effects. The shoulder arises from a rapid redistribution of e_g electron density, as a function of T, between the highly localized (l) and band-like (b) states. Furthermore, our theory leads to a correspondence between spectral changes due to increasing doping and decreasing T, as experimentally observed.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 13:05:20 GMT" } ]
2009-11-13T00:00:00
[ [ "Sanyal", "Prabuddha", "" ], [ "Gupta", "Subhra Sen", "" ], [ "Pakhira", "Nandan", "" ], [ "Krishnamurthy", "H. R.", "" ], [ "Sarma", "D. D.", "" ], [ "Ramakrishnan", "T. V.", "" ] ]
0704.3924
Lukasz Andrzej Glinka
B.M. Barbashov, L.A. Glinka, V.N. Pervushin, A.F. Zakharov
Higgs effect in Conformal Cosmology & Supernova Data
8 pages, talk on Tenth European Meeting From the Planck Scale to the Electroweak Scale Warsaw, Poland, June 9 - 13, 2007 PLANCK'07
null
null
null
hep-ph
null
The formulation of the Higgs effect is studied in the Glashow--Weinberg--Salam Standard Model, where the constant part of the Higgs potential is identified with the zeroth mode of the Higgs field. In this model, the Coleman--Weinberg effective potential obtained from the vacuum--vacuum transition amplitude is equal to unity at the extremum. This extremum immediately removes tremendous vacuum cosmological density and predicts mass of Higgs field. In this model, the kinetic energy density of the Higgs field and any scalar field can be treated as the rigid state origin that explains Supernova data in the conformal cosmology without the $\Lambda$ term.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 12:47:49 GMT" } ]
2007-05-23T00:00:00
[ [ "Barbashov", "B. M.", "" ], [ "Glinka", "L. A.", "" ], [ "Pervushin", "V. N.", "" ], [ "Zakharov", "A. F.", "" ] ]
0704.3925
Peter Kalberla MW
P.M.W. Kalberla, L. Dedes, J. Kerp, U. Haud
Dark matter in the Milky Way, II. the HI gas distribution as a tracer of the gravitational potential
19 pages, 21 figures, accepted for publication by A&A
null
10.1051/0004-6361:20066362
null
astro-ph
null
Context. Gas within a galaxy is forced to establish pressure balance against gravitational forces. The shape of an unperturbed gaseous disk can be used to constrain dark matter models. Aims. We derive the 3-D HI volume density distribution for the Milky Way out to a galactocentric radius of 40 kpc and a height of 20 kpc to constrain the Galactic mass distribution. Methods. We used the Leiden/Argentine/Bonn all sky 21-cm line survey. The transformation from brightness temperatures to densities depends on the rotation curve. We explored several models, reflecting different dark matter distributions. Each of these models was set up to solve the combined Poisson-Boltzmann equation in a self-consistent way and optimized to reproduce the observed flaring. Results. Besides a massive extended halo of M ~ 1.8 10^{12} Msun, we find a self-gravitating dark matter disk with M=2 to 3 10^{11} Msun, including a dark matter ring at 13 < R < 18.5 kpc with M = 2.2 to 2.8 10^{10} Msun. The existence of the ring was previously postulated from EGRET data and coincides with a giant stellar structure that surrounds the Galaxy. The resulting Milky Way rotation curve is flat up to R~27 kpc and slowly decreases outwards. The \hi gas layer is strongly flaring. The HWHM scale height is 60 pc at R = 4 kpc and increases to ~2700$ pc at R=40 kpc. Spiral arms cause a noticeable imprint on the gravitational field, at least out to R = 30 kpc. Conclusions. Our mass model supports previous proposals that the giant stellar ring structure is due to a merging dwarf galaxy. The fact that the majority of the dark matter in the Milky Way for $R \la 40$ kpc can be successfully modeled by a self-gravitating isothermal disk raises the question of whether this massive disk may have been caused by similar merger events in the past.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 12:18:53 GMT" } ]
2009-11-13T00:00:00
[ [ "Kalberla", "P. M. W.", "" ], [ "Dedes", "L.", "" ], [ "Kerp", "J.", "" ], [ "Haud", "U.", "" ] ]
0704.3926
Wenhua Hai
Wenhua Hai, Guishu Chong, Jianwen Song
Stabilities of one-dimensional stationary states of Bose-Einstein condensates
12 pages
Phys. Lett. A372, 2558 (2008)
10.1016/j.physleta.2007.12.029
null
quant-ph
null
We explore the dynamical stabilities of a quasi-one dimensional (1D) Bose-Einstein condensate (BEC) consisting of fixed $N$ atoms with time-independent external potential. For the stationary states with zero flow density the general solution of the perturbed time evolution equation is constructed, and the stability criterions concerning the initial conditions and system parameters are established. Taking the lattice potential case as an example, the stability and instability regions on the parameter space are found. The results suggest a method for selecting experimental parameters and adjusting initial conditions to suppress the instabilities.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 12:23:24 GMT" }, { "version": "v2", "created": "Wed, 16 Apr 2008 08:18:37 GMT" } ]
2009-11-13T00:00:00
[ [ "Hai", "Wenhua", "" ], [ "Chong", "Guishu", "" ], [ "Song", "Jianwen", "" ] ]
0704.3927
D. N. Basu
P. Roy Chowdhury, D.N. Basu, C. Samanta
Alpha decay chains from element 113
3 pages
Phys.Rev.C75:047306,2007
10.1103/PhysRevC.75.047306
null
nucl-th nucl-ex
null
Theoretical estimates of $\alpha$-decay half lives of several nuclei in the decay from element 113 are presented. Calculations in a WKB framework using DDM3Y interaction and experimental Q-values are in good agreement with the experimental data. Half life calculations are found to be quite sensitive to the Q-values and angular momenta transfers. Calculated decay lifetime decreases, owing to more penetrability as well as thinner barrier, as Q-value increases. Deviations to this predominant behaviour observed in some recent experimental data may be attributed to non zero spin-parities in some cases.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 14:47:01 GMT" } ]
2008-11-26T00:00:00
[ [ "Chowdhury", "P. Roy", "" ], [ "Basu", "D. N.", "" ], [ "Samanta", "C.", "" ] ]
0704.3928
Ian Appelbaum
Biqin Huang (1), Douwe J. Monsma (2), and Ian Appelbaum (1) ((1) University of Delaware, (2) Cambridge NanoTech Inc.)
Spin lifetime in silicon in the presence of parasitic electronic effects
null
J. Appl. Phys. 102, 013901 (2007)
10.1063/1.2750411
null
cond-mat.mtrl-sci cond-mat.other
null
A hybrid ferromagnet/semiconductor device is used to determine a lower bound on the spin lifetime for conduction electrons in silicon. We use spin precession to self-consistently measure the drift velocity vs. drift field of spin-polarized electrons and use this electronic control to change the transit time between electron injection and detection. A measurement of normalized magnetocurrent as a function of drift velocity is used with a simple exponential-decay model to argue that the lifetime obtained (~2 ns) is artificially lowered by electronic effects and is likely orders of magnitude higher.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 13:21:02 GMT" } ]
2009-11-13T00:00:00
[ [ "Huang", "Biqin", "" ], [ "Monsma", "Douwe J.", "" ], [ "Appelbaum", "Ian", "" ] ]
0704.3929
Hideki Maekawa
Hideki Maekawa, Kohsuke Tsubakihara, Hiroshi Matsumiya, Akira Ohnishi
Cascade hypernuclear production spectra at J-PARC
6 pages, 7 figures
null
null
null
nucl-th
null
We predict cascade hypernuclear production spectra expected in the forthcoming J-PARC experiment. In the Green's function method of the distorted wave impulse wave approximation with the local optimal Fermi averaging t-matrix, we can describe the Xi production spectra in the continuum and bound state region reasonably well. Predictions to the high resonlution spectra at J-PARC suggest hat we should observe Xi bound state peak structure in (K-,K+) spectra in light nuclear targets such as 12C and 27Al.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 12:35:00 GMT" } ]
2007-05-23T00:00:00
[ [ "Maekawa", "Hideki", "" ], [ "Tsubakihara", "Kohsuke", "" ], [ "Matsumiya", "Hiroshi", "" ], [ "Ohnishi", "Akira", "" ] ]
0704.3930
Ferenc Gl\"uck
J. Bonn, K. Eitel, F. Gl\"uck, D. Sevilla-Sanchez and N. Titov
The KATRIN sensitivity to the neutrino mass and to right-handed currents in beta decay
4 pages, 2 figures, 12 references
Phys.Lett.B703:310-312,2011
10.1016/j.physletb.2011.08.005
null
hep-ph
null
The aim of the KArlsruhe TRItium Neutrino experiment KATRIN is the determination of the absolute neutrino mass scale down to 0.2 eV, with essentially smaller model dependence than from cosmology and neutrinoless double beta decay. For this purpose, the integral electron energy spectrum is measured close to the endpoint of molecular tritium beta decay. The endpoint, together with the neutrino mass, should be fitted from the KATRIN data as a free parameter. The right-handed couplings change the electron energy spectrum close to the endpoint, therefore they have some effect also to the precise neutrino mass determination. The statistical calculations show that, using the endpoint as a free parameter, the unaccounted right-handed couplings constrained by many beta decay experiments can change the fitted neutrino mass value, relative to the true neutrino mass, by not larger than about 5-10 %. Using, incorrectly, the endpoint as a fixed input parameter, the above change of the neutrino mass can be much larger, order of 100 %, and for some cases it can happen that for large true neutrino mass value the fitted neutrino mass squared is negative. Publications using fixed endpoint and presenting large right-handed coupling effects to the neutrino mass determination are not relevant for the KATRIN experiment.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 12:53:21 GMT" } ]
2011-09-07T00:00:00
[ [ "Bonn", "J.", "" ], [ "Eitel", "K.", "" ], [ "Glück", "F.", "" ], [ "Sevilla-Sanchez", "D.", "" ], [ "Titov", "N.", "" ] ]
0704.3931
Martin Lange
Roland Axelsson, Martin Lange, and Rafal Somla
The Complexity of Model Checking Higher-Order Fixpoint Logic
33 pages, 2 figures, to be published in Logical Methods in Computer Science
Logical Methods in Computer Science, Volume 3, Issue 2 (June 29, 2007) lmcs:754
10.2168/LMCS-3(2:7)2007
null
cs.LO
null
Higher-Order Fixpoint Logic (HFL) is a hybrid of the simply typed \lambda-calculus and the modal \lambda-calculus. This makes it a highly expressive temporal logic that is capable of expressing various interesting correctness properties of programs that are not expressible in the modal \lambda-calculus. This paper provides complexity results for its model checking problem. In particular we consider those fragments of HFL built by using only types of bounded order k and arity m. We establish k-fold exponential time completeness for model checking each such fragment. For the upper bound we use fixpoint elimination to obtain reachability games that are singly-exponential in the size of the formula and k-fold exponential in the size of the underlying transition system. These games can be solved in deterministic linear time. As a simple consequence, we obtain an exponential time upper bound on the expression complexity of each such fragment. The lower bound is established by a reduction from the word problem for alternating (k-1)-fold exponential space bounded Turing Machines. Since there are fixed machines of that type whose word problems are already hard with respect to k-fold exponential time, we obtain, as a corollary, k-fold exponential time completeness for the data complexity of our fragments of HFL, provided m exceeds 3. This also yields a hierarchy result in expressive power.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 13:09:20 GMT" }, { "version": "v2", "created": "Fri, 29 Jun 2007 12:15:42 GMT" } ]
2015-07-01T00:00:00
[ [ "Axelsson", "Roland", "" ], [ "Lange", "Martin", "" ], [ "Somla", "Rafal", "" ] ]
0704.3932
Oscar Esquivel
O. Esquivel and B. Fuchs
Dynamical friction force exerted on spherical bodies
5 pages, 2 figures, accepted in MNRAS
Mon.Not.Roy.Astron.Soc.378:1191-1195,2007
10.1111/j.1365-2966.2007.11870.x
null
astro-ph
null
We present a rigorous calculation of the dynamical friction force exerted on a spherical massive perturber moving through an infinite homogenous system of field stars. By calculating the shape and mass of the polarization cloud induced by the perturber in the background system, which decelerates the motion of the perturber, we recover Chandrasekhar's drag force law with a modified Coulomb logarithm. As concrete examples we calculate the drag force exerted on a Plummer sphere or a sphere with the density distribution of a Hernquist profile. It is shown that the shape of the perturber affects only the exact form of the Coulomb logarithm. The latter converges on small scales, because encounters of the test and field stars with impact parameters less than the size of the massive perturber become inefficient. We confirm this way earlier results based on the impulse approximation of small angle scatterings.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 13:08:45 GMT" } ]
2009-06-23T00:00:00
[ [ "Esquivel", "O.", "" ], [ "Fuchs", "B.", "" ] ]
0704.3933
Stijn Bruers Mr
Stijn Bruers
Testing entropy production hypotheses in non-linear steady states
null
null
null
null
physics.chem-ph
null
In the last few decades, some hypotheses for entropy production (EP) principles have been forwarded as possible candidates for organizational principles in non-linear non- equilibrium systems. Two important hypotheses will be studied: the maximum entropy production (MaxEP) principle that claims that the selected steady state has the highest EP, and the gradient response principle that claims that the EP of the selected steady state (maximally) increases when the external thermodynamic driving force increases. We will formulate these hypotheses more rigorously and present a simple chemical reaction model to test these hypotheses. With the help of this model, we will clearly demonstrate that there are different MaxEP hypotheses being discussed in the literature and we will look at some parts in the literature where these differences are not always clarified. Furthermore, our chemical model will be a general counter example to all of these MaxEP and gradient response hypotheses.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 13:15:09 GMT" } ]
2007-05-23T00:00:00
[ [ "Bruers", "Stijn", "" ] ]
0704.3934
Sascha Bornhauser
Sascha Bornhauser and Manuel Drees
Signals of Very High Energy Neutralinos in Future Cosmic Ray Detectors
14 pages, 2 figures
Phys.Lett.B650:407-415,2007
10.1016/j.physletb.2007.05.048
null
hep-ph
null
``Top--down'' models explain the observation of ultra high energy cosmic rays (UHECR; $E \gsim 5 \cdot 10^{19}$ eV) through the decay of very massive, long--lived ``$X$ particles''. If superparticles with masses near a TeV exist, $X$ decays also lead to a significant flux of very energetic neutralinos, assumed to be the (stable or long--lived) lightest superparticles. There is a range of energies where neutrinos get absorbed in the Earth, but neutralinos can still traverse it. These neutralinos could in principle be detected. We calculate the detection rate in planned experiments such as OWL and EUSO. For bino--like neutralinos, which have been considered previously, we find detection rates below 1 event per Teraton of target and year in all cases; often the rates are much smaller. In contrast, if the neutralino is higgsino--like, more than ten events per year per Teraton might be observed, if the mass of the $X$ particle is near its lower bound of $\sim 10^{12}$ GeV.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 13:20:04 GMT" } ]
2008-11-26T00:00:00
[ [ "Bornhauser", "Sascha", "" ], [ "Drees", "Manuel", "" ] ]
0704.3935
Martin R. Bridson
Martin R Bridson, James Howie, Charles F Miller III, Hamish Short
Subgroups of direct products of limit groups
20 pages, no figures. Final version. Accepted by the Annals of Mathematics
null
null
null
math.GR math.GT
null
If $G_1,...,G_n$ are limit groups and $S\subset G_1\times...\times G_n$ is of type $\FP_n(\mathbb Q)$ then $S$ contains a subgroup of finite index that is itself a direct product of at most $n$ limit groups. This settles a question of Sela.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 13:29:38 GMT" }, { "version": "v2", "created": "Tue, 6 Nov 2007 22:51:24 GMT" } ]
2007-11-07T00:00:00
[ [ "Bridson", "Martin R", "" ], [ "Howie", "James", "" ], [ "Miller", "Charles F", "III" ], [ "Short", "Hamish", "" ] ]
0704.3936
Leonardo Fernandez-Jambrina
L. Fernandez-Jambrina
Hidden past of dark energy cosmological models
6 pages, 1 figure, RevTeX4, new references and comments added
Phys.Lett.B656:9-14,2007
10.1016/j.physletb.2007.08.091
null
gr-qc astro-ph hep-th
null
In this paper we analyse the possibility of having homogeneous isotropic cosmological models with observers reaching $t=\infty$ in finite proper time. It is shown that just observationally-suggested dark energy models with $w\in(-5/3,-1)$ show this feature and that they are endowed with an exotic curvature singularity. Furthermore, it is shown that non-accelerated observers in these models may experience a duration of the universe as short as desired by increasing their linear momentum. A subdivision of phantom models in two families according to this behavior is suggested.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 13:30:04 GMT" }, { "version": "v2", "created": "Thu, 3 May 2007 10:08:42 GMT" }, { "version": "v3", "created": "Thu, 27 Sep 2007 17:05:12 GMT" } ]
2008-11-26T00:00:00
[ [ "Fernandez-Jambrina", "L.", "" ] ]
0704.3937
Athanasios Batakis
Athanasios Batakis, Benoit Testud
Multifractal Analysis of inhomogeneous Bernoulli products
17 pages
null
null
null
math.MG math.DS
null
We are interested to the multifractal analysis of inhomogeneous Bernoulli products which are also known as coin tossing measures. We give conditions ensuring the validity of the multifractal formalism for such measures. On another hand, we show that these measures can have a dense set of phase transitions.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 13:30:27 GMT" } ]
2007-05-23T00:00:00
[ [ "Batakis", "Athanasios", "" ], [ "Testud", "Benoit", "" ] ]
0704.3938
Kevin J. Resch
K.J. Resch, P. Puvanathasan, J.S. Lundeen, M.W. Mitchell, and K. Bizheva
Classical dispersion-cancellation interferometry
4 pages, 3 figures
Optics Express 15, 8797 (2007).
10.1364/OE.15.008797
null
quant-ph physics.optics
null
Even-order dispersion cancellation, an effect previously identified with frequency-entangled photons, is demonstrated experimentally for the first time with a linear, classical interferometer. A combination of a broad bandwidth laser and a high resolution spectrometer was used to measure the intensity correlations between anti-correlated optical frequencies. Only 14% broadening of the correlation signal is observed when significant material dispersion, enough to broaden the regular interferogram by 4250%, is introduced into one arm of the interferometer.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 13:32:37 GMT" } ]
2009-11-13T00:00:00
[ [ "Resch", "K. J.", "" ], [ "Puvanathasan", "P.", "" ], [ "Lundeen", "J. S.", "" ], [ "Mitchell", "M. W.", "" ], [ "Bizheva", "K.", "" ] ]
0704.3939
H. W. Braden
H.W. Braden and V.Z. Enolski
Monopoles, Curves and Ramanujan
Rewritten version of math-ph/0601040
null
null
null
math-ph math.MP
null
We develop the Ercolani-Sinha construction of SU(2) monopoles and make this effective for (a five parameter family of centred) charge 3 monopoles. In particular we show how to solve the transcendental constraints arising on the spectral curve. For a class of symmetric curves the transcendental constraints become a number theoretic problem and a recently proven identity of Ramanujan provides a solution.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 13:33:37 GMT" } ]
2007-05-23T00:00:00
[ [ "Braden", "H. W.", "" ], [ "Enolski", "V. Z.", "" ] ]
0704.3940
Ryan Budney
Ryan Budney, Alexandra Mozgova
An obstruction to a knot being deform-spun via Alexander polynomials
6 Pages, 1 Figure. to appear in Proceedings of the AMS
Proc. Amer. Math. Soc. 137 (2009), 3547-3552.
null
null
math.GT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We show that if a co-dimension two knot is deform-spun from a lower-dimensional co-dimension 2 knot, there are constraints on the Alexander polynomials. In particular this shows, for all n, that not all co-dimension 2 knots in S^n are deform-spun from knots in S^{n-1}.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 13:34:57 GMT" }, { "version": "v2", "created": "Mon, 16 Feb 2009 18:52:46 GMT" } ]
2009-08-11T00:00:00
[ [ "Budney", "Ryan", "" ], [ "Mozgova", "Alexandra", "" ] ]
0704.3941
Nicola Menci
A. Cavaliere (1), N. Menci (2) ((1) Dip. Fisica Universita' di Roma ''Tor Vergata'', (2) INAF - Osservatorio Astronomico di Roma)
Bimodal AGNs in Bimodal Galaxies
7 pages, accepted for publication in the Astrophysical Journal
Astrophys.J.664:47-52,2007
10.1086/518879
Report-no: OAR/07/110
astro-ph
null
By their star content, the galaxies split out into a red and a blue population; their color index peaked around u-r=2.5 or u-r=1, respectively, quantifies the ratio of the blue stars newly formed from cold galactic gas, to the redder ones left over by past generations. On the other hand, upon accreting substantial gas amounts the central massive black holes energize active galactic nuclei (AGNs); here we investigate whether these show a similar, and possibly related, bimodal partition as for current accretion activity relative to the past. To this aim we use an updated semianalytic model; based on Monte Carlo simulations, this follows with a large statistics the galaxy assemblage, the star generations and the black hole accretions in the cosmological framework over the redshift span from z=10 to z=0. We test our simulations for yielding in close detail the observed split of galaxies into a red, early and a blue, late population. We find that the black hole accretion activities likewise give rise to two source populations: early, bright quasars and later, dimmer AGNs. We predict for their Eddington parameter $\lambda_E$ -- the ratio of the current to the past black hole accretions -- a bimodal distribution; the two branches sit now under $\lambda_E \approx 0.01$ (mainly contributed by low-luminosity AGNs) and around $\lambda_E \approx 0.3-1$. These not only mark out the two populations of AGNs, but also will turn out to correlate strongly with the red or blue color of their host galaxies.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 13:45:31 GMT" } ]
2009-06-23T00:00:00
[ [ "Cavaliere", "A.", "" ], [ "Menci", "N.", "" ] ]
0704.3942
Pramod Joag
Ali Saif M. Hassan and Pramod S. Joag
Separability Criterion for multipartite quantum states based on the Bloch representation of density matrices
23 pages no figures comments are welcome
Quantum Information and Computation, vol. 8, No. 8&9 (2008) 0773-0790
null
null
quant-ph
null
We give a new separability criterion, a necessary condition for separability of $N$-partite quantum states. The criterion is based on the Bloch representation of a $N$-partite quantum state and makes use of multilinear algebra, in particular, the matrization of tensors. Our criterion applies to {\it arbitrary} $N$-partite quantum states in $\mathcal{H}=\mathcal{H}^{d_1}\otimes \mathcal{H}^{d_2} \otimes ... \otimes \mathcal{H}^{d_N}.$ The criterion can test whether a $N$-partite state is entangled and can be applied to different partitions of the $N$-partite system. We provide examples that show the ability of this criterion to detect entanglement. We show that this criterion can detect bound entangled states. We prove a sufficiency condition for separability of a 3-partite state, straightforwardly generalizable to the case $N > 3,$ under certain condition. We also give a necessary and sufficient condition for separability of a class of $N$-qubit states which includes $N$-qubit PPT states.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 13:59:29 GMT" }, { "version": "v2", "created": "Mon, 7 May 2007 15:44:02 GMT" }, { "version": "v3", "created": "Wed, 27 Jun 2007 10:14:22 GMT" }, { "version": "v4", "created": "Mon, 16 Jul 2007 10:44:50 GMT" }, { "version": "v5", "created": "Sun, 13 Apr 2008 13:17:23 GMT" } ]
2008-07-17T00:00:00
[ [ "Hassan", "Ali Saif M.", "" ], [ "Joag", "Pramod S.", "" ] ]
0704.3943
Jan Olzem
Jan Olzem
Signatures of SUSY Dark Matter at the LHC and in the Spectra of Cosmic Rays
PhD thesis, RWTH Aachen 2007, 117 pages, 67 figures; the full resolution version (9.2M pdf) is available from http://darwin.bth.rwth-aachen.de/opus3/volltexte/2007/1842/pdf/Olzem_Jan.pdf
null
null
null
astro-ph
null
This thesis discusses the search for supersymmetry at the future Large Hadron Collider (LHC) and the ongoing construction of one of the four large LHC experiments, the Compact Muon Solenoid (CMS), and focuses on the detection of signals from the annihilation of supersymmetric dark matter in the spectra of cosmic rays. Measurements of cosmic ray antiparticles, such as positrons, can impose strong constraints on the nature of new physics beyond the Standard Model. However, cosmic ray positron measurements are experimentally very challenging due to the vast proton background. A novel approach of positron identification with the space-borne AMS-01 experiment, namely through the detection of bremsstrahlung conversion in a silicon microstrip detector, is introduced. Bremsstrahlung from protons is suppressed by a factor of more than 3*10^6 with respect to positrons. The results of the positron measurement show that the bremsstrahlung approach extends the sensitivity range of AMS-01 to positron momenta up to 50 GeV/c, which is far beyond the original scope of the experiment. At momenta above 8 GeV/c there is indication for a positron overabundance with respect to model predictions for purely secondary positron production. Therefore, the AMS-01 data lend further weight to the hints of a positron overabundance seen in the data from earlier experiments. The positron fraction measurements from the most recent experiments are combined with the results of this analysis, giving the most precise positron fraction data yet available.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 14:02:34 GMT" } ]
2007-05-23T00:00:00
[ [ "Olzem", "Jan", "" ] ]
0704.3944
Lars Fuhrmann
L. Fuhrmann, J. A. Zensus, T. P. Krichbaum, E. Angelakis, A. C. S. Readhead
Simultaneous Radio to (Sub-) mm-Monitoring of Variability and Spectral Shape Evolution of potential GLAST Blazars
3 pages, to appear in the Proceedings of the First GLAST Symposium, Stanford University, February 2007
AIP Conf.Proc.921:249-251,2007
10.1063/1.2757314
null
astro-ph
null
The Large Area Telescope (LAT) instrument onboard GLAST offers a tremendous opportunity for future blazar studies. In order to fully benefit from its capabilities and to maximize the scientific return from the LAT, it is of great importance to conduct dedicated multi-frequency monitoring campaigns that will result comprehensive observations. Consequently, we initiated an effort to conduct a GLAST-dedicated, quasi-simultaneous, broad-band flux-density (and polarization) monitoring of potential GLAST blazars with the Effelsberg and OVRO radio telescopes (11cm to 7mm wavelength). Here, we present a short overview of these activities which will complement the multi-wavelengths activities of the GLAST/LAT collaboration towards the 'low-energy' radio bands. Further we will give a brief outlook including the extension of this coordinated campaign towards higher frequencies and future scientific aims.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 14:09:36 GMT" } ]
2009-06-23T00:00:00
[ [ "Fuhrmann", "L.", "" ], [ "Zensus", "J. A.", "" ], [ "Krichbaum", "T. P.", "" ], [ "Angelakis", "E.", "" ], [ "Readhead", "A. C. S.", "" ] ]
0704.3945
Jean-Baptiste Masson
Jean-Baptiste Masson (LOB), Guilhem Gallot (LOB)
Extra energy coupling through subwavelength hole arrays via stochastic resonance
12 pages
null
null
null
cond-mat.other physics.optics
null
Interaction between metal surface waves and periodic geometry of subwavelength structures is at the core of the recent but crucial renewal of interest in plasmonics. One of the most intriguing points is the observation of abnormal strong transmission through these periodic structures, which can exceed by orders of magnitude the classical transmission given by the filling factor of the plate. The actual paradigm is that this abnormal transmission arises from the periodicity, and then that such high transmission should disappear in random geometries. Here, we show that extra energy can be coupled through the subwavelength structure by adding a controlled quantity of noise to the position of the apertures. This result can be modelled in the statistical framework of stochastic resonance. The evolution of the coupled energy with respect to noise gives access to the extra energy coupled at the surface of the subwavelength array.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 14:17:51 GMT" } ]
2007-05-23T00:00:00
[ [ "Masson", "Jean-Baptiste", "", "LOB" ], [ "Gallot", "Guilhem", "", "LOB" ] ]
0704.3946
Harald Kittang
Bj{\o}rn Ian Dundas and Harald {\O}yen Kittang
Excision for K-theory of connective ring spectra
11 pages
null
null
null
math.KT
null
We extend Geisser and Hesselholt's result on ``bi-relative K-theory'' from discrete rings to connective ring spectra. That is, if $\mathcal A$ is a homotopy cartesian $n$-cube of ring spectra (satisfying connectivity hypotheses), then the $(n+1)$-cube induced by the cyclotomic trace $$K(\mathcal A)\to TC(\mathcal A)$$ is homotopy cartesian after profinite completion. In other words, the fiber of the profinitely completed cyclotomic trace satisfies excision.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 14:20:56 GMT" } ]
2007-05-23T00:00:00
[ [ "Dundas", "Bjørn Ian", "" ], [ "Kittang", "Harald Øyen", "" ] ]
0704.3947
Ross Springell
R Springell, S W Zochowski, R C C Ward, M R Wells, S D Brown, L Bouchenoire, F Wilhelm, S Langridge, W G Stirling and G H Lander
A study of uranium-based multilayers: I. Fabrication and structural characterisation
18 pages, 7 figures, submitted to J. Phys.: Condens. Matter
null
null
null
cond-mat.mtrl-sci cond-mat.other
null
This paper addresses the structural characterisation of a series of U/Fe, U/Co and U/Gd multilayers. X-ray reflectivity has been employed to investigate the layer thickness and roughness parameters along the growth direction and high-angle diffraction measurements have been used to determine the crystal structure and orientation of the layers. For the case of uranium/transition metal systems, the interfaces are diffuse and the transition metals are present in a polycrystalline form of their common bulk phases with a preferred orientation along the closest packed planes; Fe, bcc (110) and Co, hcp (001), respectively. The uranium is present in a poorly crystalline orthorhombic, alpha-U state. In contrast, the U/Gd multilayers have sharp interfaces with negligible intermixing of atomic species, and have a roughness, which is strongly dependent on the gadolinium layer thickness. Diffraction spectra indicate a high degree of crystallinity in both U and Gd layers with intensities consistent with the growth of a novel hcp U phase, stabilised by the hcp gadolinium layers.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 14:23:22 GMT" } ]
2007-05-23T00:00:00
[ [ "Springell", "R", "" ], [ "Zochowski", "S W", "" ], [ "Ward", "R C C", "" ], [ "Wells", "M R", "" ], [ "Brown", "S D", "" ], [ "Bouchenoire", "L", "" ], [ "Wilhelm", "F", "" ], [ "Langridge", "S", "" ], [ "Stirling", "W G", "" ], [ "Lander", "G H", "" ] ]
0704.3948
Alexey Mazur K
Alexey K. Mazur
The Worm-Like Chain Theory And Bending Of Short DNA
4 pages, 3 figures, to appear in PRL
Phys. Rev. Lett. 98, 218102, 2007.
10.1103/PhysRevLett.98.218102
null
q-bio.BM cond-mat.soft physics.bio-ph
null
The probability distributions for bending angles in double helical DNA obtained in all-atom molecular dynamics simulations are compared with theoretical predictions. The computed distributions remarkably agree with the worm-like chain theory for double helices of one helical turn and longer, and qualitatively differ from predictions of the semi-elastic chain model. The computed data exhibit only small anomalies in the apparent flexibility of short DNA and cannot account for the recently reported AFM data (Wiggins et al, Nature nanotechnology 1, 137 (2006)). It is possible that the current atomistic DNA models miss some essential mechanisms of DNA bending on intermediate length scales. Analysis of bent DNA structures reveals, however, that the bending motion is structurally heterogeneous and directionally anisotropic on the intermediate length scales where the experimental anomalies were detected. These effects are essential for interpretation of the experimental data and they also can be responsible for the apparent discrepancy.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 14:24:59 GMT" } ]
2009-11-13T00:00:00
[ [ "Mazur", "Alexey K.", "" ] ]
0704.3949
Ian Appelbaum
Biqin Huang (1), Lai Zhao (1), Douwe J. Monsma (2), Ian Appelbaum (1) ((1) University of Delaware, (2) Cambridge NanoTech Inc.)
35% magnetocurrent with spin transport through Si
null
Appl. Phys. Lett. 91, 052501 (2007)
10.1063/1.2767198
null
cond-mat.mtrl-sci cond-mat.other
null
Efficient injection of spin-polarized electrons into the conduction band of silicon is limited by the formation of a silicide at the ferromagnetic metal (FM)/silicon interface. In the present work, this "magnetically-dead" silicide (where strong spin-scattering significantly reduces injected spin polarization) is eliminated by moving the FM in the spin injector from the tunnel junction base anode to the emitter cathode and away from the silicon surface. This results in over an order-of-magnitude increase in spin injection efficiency, from a previously-reported magnetocurrent ratio of ~2% to ~35% and an estimated spin polarization in Si from ~1% to at least ~15%. The injector tunnel-junction bias dependence of this spin transport signal is also measured, demonstrating the importance of low bias voltage to preserve high injected spin polarization.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 14:31:01 GMT" } ]
2009-11-13T00:00:00
[ [ "Huang", "Biqin", "", "University of Delaware" ], [ "Zhao", "Lai", "", "University of Delaware" ], [ "Monsma", "Douwe J.", "", "Cambridge NanoTech Inc" ], [ "Appelbaum", "Ian", "", "University of Delaware" ] ]
0704.3950
Mu-Lin Yan
Wei Huang, Wang Xu, Mu-Lin Yan
Backward Compton Scattering and QED with Noncommutative Plane in the Strong Uniform Magnetic Field
13 pages, 5 figures
Chinese Physics C 2008 32 (05): 342-347
10.1088/1674-1137/32/5/003
USTC-ICTS-07-08
hep-ph cond-mat.mes-hall
null
In the strong uniform magnetic field, the noncommutative plane (NCP) caused by the lowest Landau level (LLL) effect, and QED with NCP (QED-NCP) are studied. Being similar to the condensed matter theory of quantum Hall effect, an effective filling factor $f(B)$ is introduced to character the possibility that the electrons stay on the LLL. The analytic and numerical results of the differential cross section for the process of backward Compton scattering in the accelerator with unpolarized or polarized initial photons are calculated. The existing data of BL38B2 in Spring-8 have been analyzed roughly and compared with the numerical predictions primitively. We propose a precise measurement of the differential cross sections of backward Compton scattering in a strong perpendicular magnetic field, which may lead to reveal the effects of QED-NCP.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 14:34:09 GMT" }, { "version": "v2", "created": "Wed, 14 May 2008 15:41:44 GMT" } ]
2012-05-22T00:00:00
[ [ "Huang", "Wei", "" ], [ "Xu", "Wang", "" ], [ "Yan", "Mu-Lin", "" ] ]
0704.3951
G. Griffith Elder
Nigel P. Byott and G. Griffith Elder
On the necessity of new ramification breaks
null
null
null
null
math.NT
null
Ramification invariants are necessary, but not in general sufficient, to determine the Galois module structure of ideals in local number field extensions. This insufficiency is associated with elementary abelian extensions, where one can define a refined ramification filtration -- one with more ramification breaks [JNTB 17 (2005)]. The first refined break number comes from the usual ramification filtration and is therefore necessary. Here we study the second refined break number.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 14:36:16 GMT" } ]
2007-05-23T00:00:00
[ [ "Byott", "Nigel P.", "" ], [ "Elder", "G. Griffith", "" ] ]
0704.3952
Peter Grabner
Gregory Derfel, Peter J. Grabner, Fritz Vogl
Complex asymptotics of Poincar\'e functions and properties of Julia sets
Final version accepted for publication in Math. Proc. Camb. Philos. Soc
Mathematical Proceedings of the Cambridge Philosophical Society 2008
10.1017/S0305004108001564
null
math.CV math.DS
null
The asymptotic behaviour of the solutions of Poincar\'e's functional equation $f(\lambda z)=p(f(z))$ ($\lambda>1$) for $p$ a real polynomial of degree $\geq2$ is studied in angular regions of the complex plain. The constancy of an occurring periodic function is characterised in terms of geometric properties of the Julia set of $p$. For real Julia sets we give inequalities for multipliers of Pommerenke-Levin-Yoccoz type. The distribution of zeros of $f$ is related to the harmonic measure on the Julia set of $p$.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 14:41:57 GMT" }, { "version": "v2", "created": "Fri, 23 Nov 2007 10:09:08 GMT" } ]
2020-07-27T00:00:00
[ [ "Derfel", "Gregory", "" ], [ "Grabner", "Peter J.", "" ], [ "Vogl", "Fritz", "" ] ]
0704.3953
Pierre-Henri Chavanis
P.H. Chavanis
Kinetic theory of two dimensional point vortices from a BBGKY-like hierarchy
null
Physica A, 387, 1123 (2008)
10.1016/j.physa.2007.10.022
null
cond-mat.stat-mech
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Starting from the Liouville equation, we derive the exact hierarchy of equations satisfied by the reduced distribution functions of the single species point vortex gas in two dimensions. Considering an expansion of the solution in powers of 1/N in a proper thermodynamic limit $N\to +\infty$, and neglecting some collective effects, we derive a kinetic equation satisfied by the smooth vorticity field which is valid at order $O(1/N)$. This equation was obtained previously [P.H. Chavanis, Phys. Rev. E, 64, 026309 (2001)] from a more abstract projection operator formalism. If we consider axisymmetric flows and make a markovian approximation, we obtain a simpler kinetic equation which can be studied in great detail. We discuss the properties of these kinetic equations in regard to the $H$-theorem and the convergence (or not) towards the statistical equilibrium state. We also study the growth of correlations by explicitly calculating the time evolution of the two-body correlation function in the linear regime. In a second part of the paper, we consider the relaxation of a test vortex in a bath of field vortices and obtain the Fokker-Planck equation by directly calculating the second (diffusion) and first (drift) moments of the increment of position of the test vortex. A specificity of our approach is to obtain general equations, with a clear physical meaning, that are valid for flows that are not necessarily axisymmetric and that take into account non-Markovian effects. A limitations of our approach, however, is that it ignores collective effects.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 14:45:03 GMT" }, { "version": "v2", "created": "Thu, 19 Jun 2008 08:53:17 GMT" } ]
2009-11-13T00:00:00
[ [ "Chavanis", "P. H.", "" ] ]
0704.3954
Pamela Morehouse
G. Bonvicini, et al, CLEO Collaboration
Dalitz Plot Analysis of the D+ --> pi- pi+ pi+ Decay
31 pages postscript,also available through http://www.lns.cornell.edu/public/CLNS/2007/
Phys.Rev.D76:012001,2007
10.1103/PhysRevD.76.012001
CLNS 07/1993, CLEO 07-3
hep-ex
null
Using 281 pb^{-1} of data recorded by the CLEO-c detector in e^+e^- collisions at the psi(3770), corresponding to 0.78 million D^+D^- pairs, we investigate the substructure of the decay D^+ to pi^- pi^+ pi^+ using the Dalitz plot technique. We find that our data are consistent with the following intermediate states: rho(770)pi^+, f_2(1270)pi^+, f_0(1370)pi^+, f_0(1500)pi^+, f_0(980) pi^+, and sigma pi^+. We confirm large S wave contributions at low pi pi mass. We set upper limits on contributions of other possible intermediate states. We consider three models of the pi pi S wave and find that all of them adequately describe our data.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 14:57:30 GMT" }, { "version": "v2", "created": "Thu, 5 Jul 2007 13:12:26 GMT" } ]
2010-04-08T00:00:00
[ [ "Bonvicini", "G.", "" ], [ "Collaboration", "CLEO", "" ] ]
0704.3955
Claude Dion
P. Sjolund, S. J. H. Petra, C. M. Dion, H. Hagman, S. Jonsell, and A. Kastberg
Characterisation of a three-dimensional Brownian motor in optical lattices
8 pages, 14 figures
Eur. Phys. J. D 44, 381 (2007)
10.1140/epjd/e2007-00233-3
null
physics.atom-ph
null
We present here a detailed study of the behaviour of a three dimensional Brownian motor based on cold atoms in a double optical lattice [P. Sjolund et al., Phys. Rev. Lett. 96, 190602 (2006)]. This includes both experiments and numerical simulations of a Brownian particle. The potentials used are spatially and temporally symmetric, but combined spatiotemporal symmetry is broken by phase shifts and asymmetric transfer rates between potentials. The diffusion of atoms in the optical lattices is rectified and controlled both in direction and speed along three dimensions. We explore a large range of experimental parameters, where irradiances and detunings of the optical lattice lights are varied within the dissipative regime. Induced drift velocities in the order of one atomic recoil velocity have been achieved.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 14:58:08 GMT" } ]
2007-09-18T00:00:00
[ [ "Sjolund", "P.", "" ], [ "Petra", "S. J. H.", "" ], [ "Dion", "C. M.", "" ], [ "Hagman", "H.", "" ], [ "Jonsell", "S.", "" ], [ "Kastberg", "A.", "" ] ]
0704.3956
Gordon Petrie
G.J.D. Petrie, J.W.S. Blokland and R. Keppens
Magnetohydrostatic solar prominences in near-potential coronal magnetic fields
To appear in ApJ August 2007
Astrophys.J.665:830-845,2007
10.1086/519276
null
astro-ph
null
We present numerical magnetohydrostatic solutions describing the gravitationally stratified, bulk equilibrium of cool, dense prominence plasma embedded in a near-potential coronal field. These solutions are calculated using the FINESSE magnetohydrodynamics equilibrium solver and describe the morphologies of magnetic field distributions in and around prominences and the cool prominence plasma that these fields support. The equilibrium condition for this class of problem is usually different in distinct subdomains, separated by free boundaries, across which solutions are matched by suitable continuity or jump conditions describing force balance. We employ our precise finite element elliptic solver to calculate solutions not accessible by previous analytical techniques with temperature or entropy prescribed as free functions of the magnetic flux function, including a range of values of the polytropic index, temperature variations mainly across magnetic field lines and photospheric field profiles sheared close to the polarity inversion line. Out of the many examples computed here, perhaps the most noteworthy is one which reproduces precisely the three-part structure often encountered in observations: a cool dense prominence within a cavity/flux rope embedded in a hot corona. The stability properties of these new equilibria, which may be relevant to solar eruptions, can be determined in the form of a full resistive MHD spectrum using a companion hyperbolic stability solver.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 15:00:03 GMT" } ]
2019-08-19T00:00:00
[ [ "Petrie", "G. J. D.", "" ], [ "Blokland", "J. W. S.", "" ], [ "Keppens", "R.", "" ] ]
0704.3957
Vasily Ogryzko V
Vasily Ogryzko
Erwin Schroedinger, Francis Crick and epigenetic stability
New and improved version of the essay, now published in the online journal 'Biology Direct'. Contains more expanded discussion on entanglement. 18 pages, 2 figures. The file includes open reviews by E.Koonin, V.Vedral and E.Karsenti
Biol Direct. 2008 Apr 17;3(1):15
null
null
physics.gen-ph q-bio.MN
null
Schroedinger's book 'What is Life?' is widely credited for having played a crucial role in development of molecular and cellular biology. My essay revisits the issues raised by this book from the modern perspective of epigenetics and systems biology. I contrast two classes of potential mechanisms of epigenetic stability: 'epigenetic templating' and 'systems biology' approaches, and consider them from the point of view expressed by Schroedinger. I also discuss how quantum entanglement, a nonclassical feature of quantum mechanics, can help to address the 'problem of small numbers' that lead Schroedinger to promote the idea of molecular code-script for explanation of stability of biological order.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 17:35:02 GMT" }, { "version": "v2", "created": "Wed, 28 May 2008 12:16:59 GMT" } ]
2008-05-30T00:00:00
[ [ "Ogryzko", "Vasily", "" ] ]
0704.3958
Brian Rodriguez
Sergei V. Kalinin, Brian J. Rodriguez, Stephen Jesse, Katyayani Seal, Roger Proksch, Sophia Hohlbauch, Irene Revenko, Gary Lee Thompson, Alexey A. Vertegel
Towards local electromechanical probing of cellular and biomolecular systems in a liquid environment
37 pages (including refs), 8 figures
2007 Nanotechnology 18 424020 (10pp)
10.1088/0957-4484/18/42/424020
null
cond-mat.other cond-mat.soft
null
Electromechanical coupling is ubiquitous in biological systems with examples ranging from simple piezoelectricity in calcified and connective tissues to voltage-gated ion channels, energy storage in mitochondria, and electromechanical activity in cardiac myocytes and outer hair cell stereocilia. Piezoresponse force microscopy (PFM) has originally emerged as a technique to study electromechanical phenomena in ferroelectric materials, and in recent years, has been employed to study a broad range of non-ferroelectric polar materials, including piezoelectric biomaterials. At the same time, the technique has been extended from ambient to liquid imaging on model ferroelectric systems. Here, we present results on local electromechanical probing of several model cellular and biomolecular systems, including insulin and lysozyme amyloid fibrils, breast adenocarcinoma cells, and bacteriorhodopsin in a liquid environment. The specific features of SPM operation in liquid are delineated and bottlenecks on the route towards nanometer-resolution electromechanical imaging of biological systems are identified.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 15:20:18 GMT" } ]
2008-03-13T00:00:00
[ [ "Kalinin", "Sergei V.", "" ], [ "Rodriguez", "Brian J.", "" ], [ "Jesse", "Stephen", "" ], [ "Seal", "Katyayani", "" ], [ "Proksch", "Roger", "" ], [ "Hohlbauch", "Sophia", "" ], [ "Revenko", "Irene", "" ], [ "Thompson", "Gary Lee", "" ], [ "Vertegel", "Alexey A.", "" ] ]
0704.3959
Eric Charron
Naceur Gaaloul (PPM, LSAMA), Amine Jaouadi (PPM, LSAMA), Mourad Telmini (LSAMA), Laurence Pruvost (LAC), Eric Charron (PPM)
Optical Devices for Cold Atoms and Bose-Einstein Condensates
Proceedings of the International Spectroscopy Conference ISC-2007, Sousse, Tunisia
AIP Conference Proceedings 935 (2007) 10
10.1063/1.2795399
null
quant-ph
null
The manipulation of cold atoms with optical fields is a very promising technique for a variety of applications ranging from laser cooling and trapping to coherent atom transport and matter wave interferometry. Optical fields have also been proposed as interesting tools for quantum information processing with cold atoms. In this paper, we present a theoretical study of the dynamics of a cold 87Rb atomic cloud falling in the gravity field in the presence of two crossing dipole guides. The cloud is either deflected or split between the two branches of this guide. We explore the possibilities of optimization of this device and present preliminary results obtained in the case of zero-temperature dilute Bose-Einstein condensates.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 15:16:47 GMT" }, { "version": "v2", "created": "Mon, 11 Jun 2007 15:33:06 GMT" } ]
2007-09-24T00:00:00
[ [ "Gaaloul", "Naceur", "", "PPM, LSAMA" ], [ "Jaouadi", "Amine", "", "PPM, LSAMA" ], [ "Telmini", "Mourad", "", "LSAMA" ], [ "Pruvost", "Laurence", "", "LAC" ], [ "Charron", "Eric", "", "PPM" ] ]
0704.3960
Justyn Maund
J. Craig Wheeler, Justyn R. Maund and Shizuka Akiyama
Supernova Asymmetries
8 pages, 3 figures, to be published in the proceedings of the conference "Supernova 1987A: 20 Years After" Aspen, 2007
AIP Conf.Proc.937:349-356,2007
10.1063/1.2803590
null
astro-ph
null
All core collapse supernovae are strongly aspherical. The "Bochum event," with velocity components displaced symmetrically about the principal H$\alpha$ line, strongly suggests that SN 1987A was a bi-polar rather than a uni-polar explosion. While there is a general tendency to display a single prominant axis in images and spectropolarimetry, there is also growing evidence for frequent departures from axisymmetry. There are various mechanisms that might contribute to large scale departures from spherical symmetry: jet-induced processes, the spherical shock accretion instability (SASI) and associated phenomena, and non-axisymmetric instabilities (NAXI). The MRI gives inevitable production of large toroidal magnetic fields. In sum: no $\Omega$ without B. The role of magnetic fields, non-axisymmetric instabilities, and of the de-leptonization phase are discussed.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 15:19:17 GMT" } ]
2009-06-23T00:00:00
[ [ "Wheeler", "J. Craig", "" ], [ "Maund", "Justyn R.", "" ], [ "Akiyama", "Shizuka", "" ] ]
0704.3961
Pablo Arrighi
Pablo Arrighi, Renan Fargetton, Zizhu Wang
Intrinsically universal one-dimensional quantum cellular automata in two flavours
27 pages, revtex, 23 figures. V3: The results of V1-V2 are better explained and formalized, and a novel result about intrinsic universality with only finite initial configurations is given
V1-V2: DCM 2007, Poland. V3: Fudam. Informaticae journal
null
null
quant-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We give a one-dimensional quantum cellular automaton (QCA) capable of simulating all others. By this we mean that the initial configuration and the local transition rule of any one-dimensional QCA can be encoded within the initial configuration of the universal QCA. Several steps of the universal QCA will then correspond to one step of the simulated QCA. The simulation preserves the topology in the sense that each cell of the simulated QCA is encoded as a group of adjacent cells in the universal QCA. The encoding is linear and hence does not carry any of the cost of the computation. We do this in two flavours: a weak one which requires an infinite but periodic initial configuration and a strong one which needs only a finite initial configuration. KEYWORDS: Quantum cellular automata, Intrinsic universality, Quantum computation.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 15:22:05 GMT" }, { "version": "v2", "created": "Tue, 1 May 2007 14:50:57 GMT" }, { "version": "v3", "created": "Wed, 10 Dec 2008 15:09:29 GMT" } ]
2008-12-10T00:00:00
[ [ "Arrighi", "Pablo", "" ], [ "Fargetton", "Renan", "" ], [ "Wang", "Zizhu", "" ] ]
0704.3962
Christine Noot-Huyghe
Christine Noot-Huyghe (IRMA)
Un th\'eor\`eme de Beilinson-Bernstein pour les D-modules arithm\'etiques
22 pages; Preprint (29/04/2007)
null
null
null
math.AG
null
One proves a Beilinson-Bernstein theorem in the context of arithmetic D-modules introduced by Berthelot, for flag varieties. This generalizes in the arithmetic context previous results of Brylinski-Kashiwara and Beilinson-Bernstein in the complex case.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 15:29:18 GMT" }, { "version": "v2", "created": "Fri, 25 May 2007 12:04:45 GMT" } ]
2007-06-13T00:00:00
[ [ "Noot-Huyghe", "Christine", "", "IRMA" ] ]
0704.3963
Andreas Mueller
Andreas Mueller and Bernd Aschenbach
Non-monotonic orbital velocity profiles around rapidly rotating Kerr-(anti-)de Sitter black holes
9 pages, 4 figures, accepted for Class. Quant. Grav
Class.Quant.Grav.24:2637-2644,2007
10.1088/0264-9381/24/10/009
null
gr-qc astro-ph
null
It has been recently demonstrated that the orbital velocity profile around Kerr black holes in the equatorial plane as observed in the locally non-rotating frame exhibits a non-monotonic radial behaviour. We show here that this unexpected minimum-maximum feature of the orbital velocity remains if the Kerr vacuum is generalized to the Kerr-de Sitter or Kerr-anti-de Sitter metric. This is a new general relativity effect in Kerr spacetimes with non-vanishing cosmological constant. Assuming that the profile of the orbital velocity is known, this effect constrains the spacetime parameters.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 15:32:14 GMT" } ]
2008-11-26T00:00:00
[ [ "Mueller", "Andreas", "" ], [ "Aschenbach", "Bernd", "" ] ]
0704.3964
Fernando Martinez-Vidal
F. Martinez-Vidal (On behalf of the BaBar Collaboration)
Measurement of the CKM angle gammma with B-+ ->D^(*)[K0s pi- pi+]K^(*)-+ decays in BaBar
Proceedings of the 4th International Workshop on the CKM Unitarity Triangle (CKM'06), 12-16 December, 2006, Nagoya (Japan)
null
null
null
hep-ex
null
We report on the measurement of the Cabibbo-Kobayashi-Maskawa angle gamma through a Dalitz analysis of neutral D decays to K0s pi- pi+ in the processes B-+ -> D^(*) K-+ and B-+ -> D K^*-+, D^* -> D pi0, D gamma, with the Babar detector at the SLAC PEP-II e^+ e^- asymmetric-energy collider.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 15:59:02 GMT" } ]
2007-05-23T00:00:00
[ [ "Martinez-Vidal", "F.", "", "On behalf of the BaBar Collaboration" ] ]
0704.3965
Servio Perez
S.T. Perez-Merchancano, G. E. Marques, and L.E. Bolivar-Marinez
Optical Transitions in New Trends Organic Materials
4 pages, 5 figures, references. Submitted to the Microelectronic Journal
null
null
null
cond-mat.other
null
The PTCDA (3,4,9,10-Perylene-tetracarboxylic dianhydride) and the NTCDA (1,4,5,8-Naphtalenetetracarboxylic dianhydride) are aromatic, stable, planar and highly symmetric with unusual electrical properties. The PTCDA is a semiconductor organic crystalline of particular interest due to its excellent properties and electronic potential that are used in optoelectronic devices and the NTCDA it is monoclinic and its space group is similar to that of the PTCDA. Recently, alternate layers of PTCDA and NTCDA were growth forming multiple structures of quantum wells showing a new class of materials with new optic lineal properties. Some have assured that their big utilities would be centered in the construction of diodes and of possible guides of waves. We have carried out calculations semi-empirical of the electronic structures and of optic properties of the PTCDA and of the NTCDA that show us that they are structures highly orderly polymeric, semiconductors in a negative load state (charge state= -2)
[ { "version": "v1", "created": "Mon, 30 Apr 2007 16:29:41 GMT" } ]
2007-05-23T00:00:00
[ [ "Perez-Merchancano", "S. T.", "" ], [ "Marques", "G. E.", "" ], [ "Bolivar-Marinez", "L. E.", "" ] ]
0704.3966
Gary Goldstein
Gary R. Goldstein
Dick Dalitz: Examples of His Contributions to Particle Physics
14 pages, 9 figures, for Proceedings ISSP Erice 2006
null
10.1142/9789812832467_0017
null
physics.hist-ph hep-ph nucl-th
null
Dick Dalitz produced lasting contributions to particle physics for 50 years. Along with Dalitz pairs, Dalitz plots and CDD poles, he did major work in parity violation, hyperon resonance identification, the quark model, and hypernuclei. These topics will be summarized, with some emphasis on the author's collaboration with Dalitz on quark spin and fragmentation correlations, and, particularly, the work on the identification of the top quark and its mass. Short biographical information is interspersed. This paper is based on a presentation at the International School of Subnuclear Physics, Erice 2006.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 16:02:16 GMT" } ]
2017-08-23T00:00:00
[ [ "Goldstein", "Gary R.", "" ] ]
0704.3967
Michael Potthoff
A. Fleszar, M. Potthoff, W. Hanke
Electronic structure of zinc-blende MnTe within the GW approximation
9 pages, accepted for publication in pssc (special issue on II-VI semiconductors)
null
10.1002/pssc.200775407
null
cond-mat.str-el
null
Using the local spin-density approximation (LSDA) and the (non self-consistent) GW approach, the (quasi-particle) band structure is calculated for MnTe in zinc-blende geometry. Different parameters characterizing the electronic structure are computed for an antiferromagnetic and the ferromagnetic phase and compared with the experiment. The strong Hubbard-type repulsion on the Mn-3d orbitals and the p-d hybridization are seen to be responsible for substantial defects found in the LSDA picture. It is discussed to which extent these can be improved upon by means of the GW approach.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 16:20:27 GMT" } ]
2015-05-13T00:00:00
[ [ "Fleszar", "A.", "" ], [ "Potthoff", "M.", "" ], [ "Hanke", "W.", "" ] ]
0704.3968
Andrzej Czarnecki
A. Czarnecki, W. J. Marciano, and A. Sirlin
Electroweak Radiative Corrections to Muon Capture
6 pages
Phys.Rev.Lett.99:032003,2007
10.1103/PhysRevLett.99.032003
null
hep-ph
null
Electroweak radiative corrections to muon capture on nuclei are computed and found to be sizable. They enhance the capture rates for hydrogen and helium by 2.8% and 3.0% respectively. As a result, the value of the induced pseudoscalar coupling, g_P^exp, extracted from a recent hydrogen 1S singlet capture experiment is increased by about 21% to g_P^exp = 7.3 +/- 1.2 and brought into good agreement with the prediction of chiral perturbation theory, g_P^theory=8.2 +/- 0.2. Implications for helium capture rate predictions are also discussed.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 16:25:46 GMT" } ]
2008-11-26T00:00:00
[ [ "Czarnecki", "A.", "" ], [ "Marciano", "W. J.", "" ], [ "Sirlin", "A.", "" ] ]
0704.3969
Jean-Claude Belfiore
Sheng Yang and Jean-Claude Belfiore
Diversity of MIMO Multihop Relay Channels - Part I: Amplify-and-Forward
37 pages, 15 figures. submitted to IEEE Transactions on Information Theory
null
null
null
cs.IT math.IT
null
In this two-part paper, we consider the multiantenna multihop relay channels in which the source signal arrives at the destination through N independent relaying hops in series. The main concern of this work is to design relaying strategies that utilize efficiently the relays in such a way that the diversity is maximized. In part I, we focus on the amplify-and-forward (AF) strategy with which the relays simply scale the received signal and retransmit it. More specifically, we characterize the diversity-multiplexing tradeoff (DMT) of the AF scheme in a general multihop channel with arbitrary number of antennas and arbitrary number of hops. The DMT is in closed-form expression as a function of the number of antennas at each node. First, we provide some basic results on the DMT of the general Rayleigh product channels. It turns out that these results have very simple and intuitive interpretation. Then, the results are applied to the AF multihop channels which is shown to be equivalent to the Rayleigh product channel, in the DMT sense. Finally, the project-and-forward (PF) scheme, a variant of the AF scheme, is proposed. We show that the PF scheme has the same DMT as the AF scheme, while the PF can have significant power gain over the AF scheme in some cases. In part II, we will derive the upper bound on the diversity of the multihop channels and show that it can be achieved by partitioning the multihop channel into AF subchannels.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 16:28:51 GMT" } ]
2007-07-13T00:00:00
[ [ "Yang", "Sheng", "" ], [ "Belfiore", "Jean-Claude", "" ] ]
0704.3970
Ross Springell
R Springell, S W Zochowski, R C C Ward, M R Wells, S D Brown, L Bouchenoire, F Wilhelm, S Langridge, W G Stirling and G H Lander
A study of uranium-based multilayers: II. Magnetic properties
18 pages, 8 figures, submitted to J. Phys.: Condens. Matter
null
10.1088/0953-8984/20/21/215230
null
cond-mat.mtrl-sci cond-mat.other
null
SQUID magnetometry and polarised neutron reflectivity measurements have been employed to characterise the magnetic properties of U/Fe, U/Co and U/Gd multilayers. The field dependence of the magnetisation was measured at 10K in magnetic fields from -70kOe to 70kOe. A temperature dependent study of the magnetisation evolution was undertaken for a selection of U/Gd samples. PNR was carried out in a field of 4.4kOe for U/Fe and U/Co samples (at room temperature) and for U/Gd samples (at 10K). Magnetic 'dead' layers of about 15 Angstrom were observed for U/Fe and U/Co samples, consistent with a picture of interdiffused interfaces. A large reduction in the magnetic moment, constant over a wide range of Gd layer thicknesses, was found for the U/Gd system (about 4 Bohr magnetons compared with 7.63 for the bulk metal). This could be understood on the basis of a pinning of Gd moments arising from a column-like growth mechanism of the Gd layers. A study of the effective anisotropy suggests that perpendicular magnetic anisotropy could occur in multilayers consisting of thick U and thin Gd layers. A reduction in the Curie temperature was observed as a function of Gd layer thickness, consistent with a finite-size scaling behaviour.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 16:51:44 GMT" } ]
2009-11-13T00:00:00
[ [ "Springell", "R", "" ], [ "Zochowski", "S W", "" ], [ "Ward", "R C C", "" ], [ "Wells", "M R", "" ], [ "Brown", "S D", "" ], [ "Bouchenoire", "L", "" ], [ "Wilhelm", "F", "" ], [ "Langridge", "S", "" ], [ "Stirling", "W G", "" ], [ "Lander", "G H", "" ] ]
0704.3971
Tobias Kipp
Ch. Strelow, C. M. Schultz, H. Rehberg, H. Welsch, Ch. Heyn, D. Heitmann and T. Kipp
Three-Dimensionally Confined Optical Modes in Quantum Well Microtube Ring Resonators
5 pages, 4 figures
null
10.1103/PhysRevB.76.045303
null
cond-mat.other
null
We report on microtube ring resonators with quantum wells embedded as an optically active material. Optical modes are observed over a broad energy range. Their properties strongly depend on the exact geometry of the microtube along its axis. In particular we observe (i) preferential emission of light on the inside edge of the microtube and (ii) confinement of light also in direction of the tube axis by an axially varying geometry which is explained in an expanded waveguide model.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 16:31:31 GMT" } ]
2009-11-13T00:00:00
[ [ "Strelow", "Ch.", "" ], [ "Schultz", "C. M.", "" ], [ "Rehberg", "H.", "" ], [ "Welsch", "H.", "" ], [ "Heyn", "Ch.", "" ], [ "Heitmann", "D.", "" ], [ "Kipp", "T.", "" ] ]
0704.3972
Servio Perez
P.J. Salazar-Valencia, L.E. Bolivar-Marinez, and S.T. Perez-Merchancano
Electronic Emition Properties of Bi Layer Novel Organic Semiconductor Systems
4 pages, 2 figures, 1 table, references. Submitted to the Microelectronic Journal
null
null
null
cond-mat.mes-hall
null
The perylene-3,4,9,10-tetracarboxylic-dianhydride (PTCDA) and 1,4,5,8-naphthalene-tetracaboxylic-dianhydride (NTCDA) are planar pi-stacking organic molecules that have been shown to be excellent model compounds for studying the growth and optoelectronic properties of organic semiconductor thin films, particularly organic diodes. Some observations have shown that this molecules, particularly PTCDA a brick-like shaped molecule easily forms well-ordered films on various substrates due to its unique crystal structure which is characterized by flat lying molecules In this work we will explore some energetic and optical characteristics such as heats of formation, optic GAP energies, electronic transitions and others of novel tow layer systems of alternate layers of PTCDA and NTCDA by means of the semiempirical methods Parametric Model 3 (PM3) and Zerner's Intermediate Neglect of Differential Overlap (ZINDO/S) in Configuration Interaction mode.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 16:35:54 GMT" } ]
2007-05-23T00:00:00
[ [ "Salazar-Valencia", "P. J.", "" ], [ "Bolivar-Marinez", "L. E.", "" ], [ "Perez-Merchancano", "S. T.", "" ] ]
0704.3973
Alexei Yu. Karlovich
Alexei Yu. Karlovich
Semi-Fredholm singular integral operators with piecewise continuous coefficients on weighted variable Lebesgue spaces are Fredholm
16 pages
null
null
null
math.FA
null
Suppose $\Gamma$ is a Carleson Jordan curve with logarithmic whirl points, $\varrho$ is a Khvedelidze weight, $p:\Gamma\to(1,\infty)$ is a continuous function satisfying $|p(\tau)-p(t)|\le -\mathrm{const}/\log|\tau-t|$ for $|\tau-t|\le 1/2$, and $L^{p(\cdot)}(\Gamma,\varrho)$ is a weighted generalized Lebesgue space with variable exponent. We prove that all semi-Fredholm operators in the algebra of singular integral operators with $N\times N$ matrix piecewise continuous coefficients are Fredholm on $L_N^{p(\cdot)}(\Gamma,\varrho)$.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 16:40:26 GMT" } ]
2007-05-23T00:00:00
[ [ "Karlovich", "Alexei Yu.", "" ] ]
0704.3974
Servio Perez
Julian A. Zu\~niga, O.L. Hernandez-Rosero, and S.T. Perez-Merchancano
Rectangular Potential Barrier Affected by External Fields, Hydrostatic Pressure and Impurities
3 pages, 3 figures. Submitted to the Microelectronic Journal
null
null
null
cond-mat.mes-hall
null
In this work the influence of the electric and magnetic fields over a tunneling particle in a rectangular potential barrier is shown, we have taken into account the presence of an impurity at the barrier center and the effects of a hydrostatic pressure parallel to the barrier height considering the BenDaniel-Duke boundary conditions. Given that the particle is moving inside a GaAs-AlxGa1-xAs-GaAs heterostructures it is evident a change in the transmission coefficient due to the impurity concentration and the presence of the hydrostatic pressure. The potential due to the presence of the impurity is approximate with a second degree polynomial function that resolves the discontinuity generated by heavily modifying the transmission coefficient.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 16:49:24 GMT" } ]
2007-05-23T00:00:00
[ [ "Zuñiga", "Julian A.", "" ], [ "Hernandez-Rosero", "O. L.", "" ], [ "Perez-Merchancano", "S. T.", "" ] ]
0704.3975
Audrey Cottet
Audrey Cottet
Spectroscopy and critical temperature of diffusive superconducting/ferromagnetic hybrid structures with spin-active interfaces
12 pages, 6 figures, to be published in Phys. Rev. B
Phys. Rev. B 76, 224505 (2007)
10.1103/PhysRevB.76.224505
null
cond-mat.supr-con
null
The description of the proximity effect in superconducting/ferromagnetic heterostructures requires to use spin-dependent boundary conditions. Such boundary conditions must take into account the spin dependence of the phase shifts acquired by electrons upon scattering on the boundaries of ferromagnets. The present article shows that this property can strongly affect the critical temperature and the energy dependence of the density of states of diffusive heterostructures. These effects should allow a better caracterisation of diffusive superconductor/ferromagnet interfaces.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 16:50:52 GMT" }, { "version": "v2", "created": "Tue, 17 Jul 2007 10:05:13 GMT" }, { "version": "v3", "created": "Mon, 12 Nov 2007 20:46:17 GMT" } ]
2009-11-13T00:00:00
[ [ "Cottet", "Audrey", "" ] ]
0704.3976
Dirk Hofmann
Maria Manuel Clementino (University of Coimbra) and Dirk Hofmann (University of Aveiro)
Lawvere completeness in Topology
null
null
null
null
math.CT math.GN
null
It is known since 1973 that Lawvere's notion of (Cauchy-)complete enriched category is meaningful for metric spaces: it captures exactly Cauchy-complete metric spaces. In this paper we introduce the corresponding notion of Lawvere completeness for $(\mathbb{T},\mathsf{V})$-categories and show that it has an interesting meaning for topological spaces and quasi-uniform spaces: for the former ones means weak sobriety while for the latter means Cauchy completeness. Further, we show that $\mathsf{V}$ has a canonical $(\mathbb{T},\mathsf{V})$-category structure which plays a key role: it is Lawvere-complete under reasonable conditions on the setting; permits us to define a Yoneda embedding in the realm of $(\mathbb{T},\mathsf{V})$-categories.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 16:52:30 GMT" } ]
2007-05-23T00:00:00
[ [ "Clementino", "Maria Manuel", "", "University of Coimbra" ], [ "Hofmann", "Dirk", "", "University of Aveiro" ] ]
0704.3977
Servio Perez
M.M. Falla Sol\'orzano, L.E. Bolivar-Marinez, and S.T. Perez-Merchancano
Electronic Properties of Eumelanin Monomers and Dimmers
4 pages, 2 figures, 2 tables. Submitted to the Microelectronic Journal
null
null
null
cond-mat.mes-hall
null
The melanin is a group of biological pigments commonly found in living beings, it can be classified in three groups: eumelanin human beings, pheomelanins in animals, and allomelanins in the vegetal kingdom. There is a special interest in the eumelanin because this biopolymer exhibits the typical properties of a semiconductor. Eumelanin is also responsible of the main cellular photoprotection mechanisms in the human beings. The exact structural pattern of eumelanin is not completely known yet, the planar molecules 5, 6-indolquinine and its reduced forms semiquinone and hydroquinone outline the greater part of the biological pigment. In this work the structural, electronic and optical properties of monomers in various charged states (0, -1) and dimmers of eumelanin in vacuum, are found for the neutral state of charge, by means of the Semiempirical methods MNDO, AM1, PM3 and ZINDO/S-CI
[ { "version": "v1", "created": "Mon, 30 Apr 2007 16:53:40 GMT" } ]
2007-05-23T00:00:00
[ [ "Solórzano", "M. M. Falla", "" ], [ "Bolivar-Marinez", "L. E.", "" ], [ "Perez-Merchancano", "S. T.", "" ] ]
0704.3978
Jose W. F. Valle
V. B. Semikoz and J. W. F. Valle
Lepton asymmetries and the growth of cosmological seed magnetic fields
4 pages, no figures, final published version available online at http://www.iop.org/EJ/abstract/1029-8479/2008/03/067
JHEP 0803:067,2008
10.1088/1126-6708/2008/03/067
IFIC/07-19
hep-ph astro-ph
null
Primordial cosmological hypermagnetic fields polarize the early Universe plasma prior to the electroweak phase transition (EWPT). As a result of the long range parity violating gauge interaction present in the Standard Model their magnitude gets amplified, opening a new, perturbative way, of accounting for the observed intergalactic magnetic fields.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 17:45:58 GMT" }, { "version": "v2", "created": "Fri, 28 Mar 2008 12:04:50 GMT" } ]
2009-09-17T00:00:00
[ [ "Semikoz", "V. B.", "" ], [ "Valle", "J. W. F.", "" ] ]
0704.3979
Javier Trujillo Bueno
Luca Belluzzi, Javier Trujillo Bueno and Egidio Landi Degl'Innocenti
The Magnetic Sensitivity of the Ba II D1 and D2 Lines of the Fraunhofer Spectrum
40 pages, 1 table and 19 figures. Accepted for publication in The Astrophysical Journal (ApJ)
Astrophys.J.666:588-608,2007
10.1086/519078
null
astro-ph
null
The physical interpretation of the spectral line polarization produced by the joint action of the Hanle and Zeeman effects offers a unique opportunity to obtain empirical information about hidden aspects of solar and stellar magnetism. To this end, it is important to achieve a complete understanding of the sensitivity of the emergent spectral line polarization to the presence of a magnetic field. Here we present a detailed theoretical investigation on the role of resonance scattering and magnetic fields on the polarization signals of the Ba II D1 and D2 lines of the Fraunhofer spectrum, respectively at 4934 \AA\ and 4554 \AA. We adopt a three-level model of Ba II, and we take into account the hyperfine structure that is shown by the $^{135}$Ba and $^{137}$Ba isotopes. Despite of their relatively small abundance (18%), the contribution coming from these two isotopes is indeed fundamental for the interpretation of the polarization signals observed in these lines. We consider an optically thin slab model, through which we can investigate in a rigorous way the essential physical mechanisms involved (resonance polarization, Zeeman, Paschen-Back and Hanle effects), avoiding complications due to radiative transfer effects. We assume the slab to be illuminated from below by the photospheric solar continuum radiation field, and we investigate the radiation scattered at 90 degrees, both in the absence and in the presence of magnetic fields, deterministic and microturbulent. We show in particular the existence of a differential magnetic sensitivity of the three-peak Q/I profile that is observed in the D2 line in quiet regions close to the solar limb, which is of great interest for magnetic field diagnostics.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 19:09:26 GMT" } ]
2009-06-23T00:00:00
[ [ "Belluzzi", "Luca", "" ], [ "Bueno", "Javier Trujillo", "" ], [ "Degl'Innocenti", "Egidio Landi", "" ] ]
0704.3980
Ivan Penkov
Ivan Penkov, Gregg Zuckerman
A construction of generalized Harish-Chandra modules for locally reductive Lie algebras
null
null
null
null
math.RT
null
We study cohomological induction for a pair $(\frak g,\frak k)$, $\frak g$ being an infinite dimensional locally reductive Lie algebra and $\frak k \subset\frak g$ being of the form $\frak k_0 + C_\gg(\frak k_0)$, where $\frak k_0\subset\frak g$ is a finite dimensional reductive in $\frak g$ subalgebra and $C_{\gg} (\frak k_0)$ is the centralizer of $\frak k_0$ in $\frak g$. We prove a general non-vanishing and $\frak k$-finiteness theorem for the output. This yields in particular simple $(\frak g,\frak k)$-modules of finite type over $\frak k$ which are analogs of the fundamental series of generalized Harish-Chandra modules constructed in \cite{PZ1} and \cite{PZ2}. We study explicit versions of the construction when $\frak g$ is a root-reductive or diagonal locally simple Lie algebra.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 17:13:09 GMT" } ]
2007-05-23T00:00:00
[ [ "Penkov", "Ivan", "" ], [ "Zuckerman", "Gregg", "" ] ]
0704.3981
Stephen West
Ben Gripaios and Stephen M. West
Anomaly Holography
26 pages, references added
Nucl.Phys.B789:362-381,2008
10.1016/j.nuclphysb.2007.08.008
OUTP-0705P
hep-ph hep-th
null
We consider, in the effective field theory context, anomalies of gauge field theories on a slice of a five-dimensional, Anti-de Sitter geometry and their four-dimensional, holographic duals. A consistent effective field theory description can always be found, notwithstanding the presence of the anomalies and without modifying the degrees of freedom of the theory. If anomalies do not vanish, the d=4 theory contains additional pseudoscalar states, which are either present in the low-energy theory as physical, light states, or are eaten by (would-be massless) gauge bosons. We show that the pseudoscalars ensure that global anomalies of the four-dimensional dual satisfy the 't Hooft matching condition and comment on the relevance for warped models of electroweak symmetry breaking.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 17:22:35 GMT" }, { "version": "v2", "created": "Thu, 14 Feb 2008 10:46:30 GMT" } ]
2008-11-26T00:00:00
[ [ "Gripaios", "Ben", "" ], [ "West", "Stephen M.", "" ] ]
0704.3982
Hanfei Yan
Hanfei Yan, Jorg Maser, Albert Macrander, Qun Shen, Stefan Vogt, Brian Stephenson and Hyon Chol Kang
Takagi-Taupin Description of X-ray Dynamical Diffraction from Diffractive Optics with Large Numerical Aperture
18 pages, 12 figures
null
10.1103/PhysRevB.76.115438
null
physics.optics physics.class-ph
null
We present a formalism of x-ray dynamical diffraction from volume diffractive optics with large numerical aperture and high aspect ratio, in an analogy to the Takagi-Taupin equations for strained single crystals. We derive a set of basic equations for dynamical diffraction from volume diffractive optics, which enable us to study the focusing property of these optics with various grating profiles. We study volume diffractive optics that satisfy the Bragg condition to various degrees, namely flat, tilted and wedged geometries, and derive the curved geometries required for ultimate focusing. We show that the curved geometries satisfy the Bragg condition everywhere and phase requirement for point focusing, and effectively focus hard x-rays to a scale close to the wavelength.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 17:25:35 GMT" } ]
2009-11-13T00:00:00
[ [ "Yan", "Hanfei", "" ], [ "Maser", "Jorg", "" ], [ "Macrander", "Albert", "" ], [ "Shen", "Qun", "" ], [ "Vogt", "Stefan", "" ], [ "Stephenson", "Brian", "" ], [ "Kang", "Hyon Chol", "" ] ]
0704.3983
Julien Barre
Julien Barre
Retrieving information from a noisy "knowledge network"
10 pages, 4 figures. Writing of the last section improved; version accepted in JSTAT
null
10.1088/1742-5468/2007/08/P08015
null
cond-mat.stat-mech cond-mat.dis-nn
null
We address the problem of retrieving information from a noisy version of the ``knowledge networks'' introduced by Maslov and Zhang. We map this problem onto a disordered statistical mechanics model, which opens the door to many analytical and numerical approaches. We give the replica symmetric solution, compare with numerical simulations, and finally discuss an application to real datas from the United States Senate.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 17:27:01 GMT" }, { "version": "v2", "created": "Thu, 5 Jul 2007 07:35:06 GMT" } ]
2009-11-13T00:00:00
[ [ "Barre", "Julien", "" ] ]
0704.3984
Boris Krippa
Boris Krippa
Exact renormalisation group flow for ultracold Fermi gases in unitary limit
11 pages, Revtex, misprints corrected, references and comments added
J.Phys.A42:465002,2009
10.1088/1751-8113/42/46/465002
null
cond-mat.supr-con nucl-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study the exact renormalisation group flow for ultracold Fermi-gases in unitary regime. We introduce a pairing field to describe the formation of the Cooper pairs, and take a simple ansatz for the effective action. Set of approximate flow equations for the effective couplings including boson and fermionic fluctuations is derived. At some value of the running scale, the system undergoes a phase transition to a gapped phase. The values of the energy density, chemical potential, pairing gap and the corresponding proportionality constants relating the interacting and non-interacting Fermi gases are calculated. Standard mean field results are recovered if we omit the boson loops.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 17:40:35 GMT" }, { "version": "v2", "created": "Tue, 1 May 2007 16:17:39 GMT" }, { "version": "v3", "created": "Tue, 8 May 2007 15:55:05 GMT" }, { "version": "v4", "created": "Thu, 18 Dec 2008 16:25:38 GMT" } ]
2009-11-05T00:00:00
[ [ "Krippa", "Boris", "" ] ]
0704.3985
Ioannis Bakas
I. Bakas, C. Sourdis
Dirichlet sigma models and mean curvature flow
77 pages, 21 figures
JHEP 0706:057,2007
10.1088/1126-6708/2007/06/057
null
hep-th math-ph math.DG math.MP
null
The mean curvature flow describes the parabolic deformation of embedded branes in Riemannian geometry driven by their extrinsic mean curvature vector, which is typically associated to surface tension forces. It is the gradient flow of the area functional, and, as such, it is naturally identified with the boundary renormalization group equation of Dirichlet sigma models away from conformality, to lowest order in perturbation theory. D-branes appear as fixed points of this flow having conformally invariant boundary conditions. Simple running solutions include the paper-clip and the hair-pin (or grim-reaper) models on the plane, as well as scaling solutions associated to rational (p, q) closed curves and the decay of two intersecting lines. Stability analysis is performed in several cases while searching for transitions among different brane configurations. The combination of Ricci with the mean curvature flow is examined in detail together with several explicit examples of deforming curves on curved backgrounds. Some general aspects of the mean curvature flow in higher dimensional ambient spaces are also discussed and obtain consistent truncations to lower dimensional systems. Selected physical applications are mentioned in the text, including tachyon condensation in open string theory and the resistive diffusion of force-free fields in magneto-hydrodynamics.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 17:48:53 GMT" } ]
2009-11-13T00:00:00
[ [ "Bakas", "I.", "" ], [ "Sourdis", "C.", "" ] ]
0704.3986
Sergiu Vacaru I.
Sergiu I. Vacaru
Parametric Nonholonomic Frame Transforms and Exact Solutions in Gravity
a latex 2e [11pt] variant corresponding to proofs for IJMMP, 54 pages
Int.J.Geom.Meth.Mod.Phys.04:1285-1334,2008
10.1142/S0219887807002570
null
gr-qc hep-th math-ph math.DG math.MP
null
A generalized geometric method is developed for constructing exact solutions of gravitational field equations in Einstein theory and generalizations. First, we apply the formalism of nonholonomic frame deformations (formally considered for nonholonomic manifolds and Finsler spaces) when the gravitational field equations transform into systems of nonlinear partial differential equations which can be integrated in general form. The new classes of solutions are defined by generic off-diagonal metrics depending on integration functions on one, two and three (or three and four) variables if we consider four (or five) dimensional spacetimes. Second, we use a general scheme when one (two) parameter families of exact solutions are defined by any source-free solutions of Einstein's equations with one (two) Killing vector field(s). A successive iteration procedure results in new classes of solutions characterized by an infinite number of parameters for a non-Abelian group involving arbitrary functions on one variable. Five classes of exact off-diagonal solutions are constructed in vacuum Einstein and in string gravity describing solitonic pp-wave interactions. We explore possible physical consequences of such solutions derived from primary Schwarzschild or pp-wave metrics.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 17:49:57 GMT" }, { "version": "v2", "created": "Tue, 1 May 2007 21:29:55 GMT" }, { "version": "v3", "created": "Mon, 24 Sep 2007 20:32:45 GMT" }, { "version": "v4", "created": "Mon, 19 Nov 2007 18:07:55 GMT" } ]
2008-11-26T00:00:00
[ [ "Vacaru", "Sergiu I.", "" ] ]
0704.3987
Ana Firan
Ana Firan and Ryszard Stroynowski
Internal conversions in Higgs decays to two photons
one .tex file and two .eps figures
Phys.Rev.D76:057301,2007
10.1103/PhysRevD.76.057301
null
hep-ph
null
We evaluate the partial widths for internal conversions in the Higgs decays to two photons. For the Higgs masses of interest at LHC in the range of 100-150 GeV, the conversions to pairs of fermions represent significant fraction of Higgs decays.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 18:03:27 GMT" }, { "version": "v2", "created": "Wed, 18 Jul 2007 22:26:10 GMT" } ]
2008-11-26T00:00:00
[ [ "Firan", "Ana", "" ], [ "Stroynowski", "Ryszard", "" ] ]
0704.3988
Nathanial P. Brown
Nathanial P. Brown and Andrew S. Toms
Three Applications of the Cuntz Semigroup
10 pages
null
null
null
math.OA
null
Building on work of Elliott and coworkers, we present three applications of the Cuntz semigroup: (i) for many simple C$^*$-algebras, the Thomsen semigroup is recovered functorially from the Elliott invariant, and this yields a new proof of Elliott's classification theorem for simple, unital AI algebras; (ii) for the algebras in (i), classification of their Hilbert modules is similar to the von Neumann algebra context; (iii) for the algebras in (i), approximate unitary equivalence of self-adjoint operators is characterised in terms of the Elliott invariant.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 18:03:28 GMT" } ]
2007-05-23T00:00:00
[ [ "Brown", "Nathanial P.", "" ], [ "Toms", "Andrew S.", "" ] ]
0704.3989
Michael Robinson
Michael Robinson
Instability of an equilibrium of a partial differential equation
12 pages
null
null
null
math.AP math.DS
null
A nonlinear parabolic differential equation with a quadratic nonlinearity is presented which has at least one equilibrium. The linearization about this equilibrium is asymptotically stable, but by using a technique inspired by H. Fujita, we show that the equilibrium is unstable in the nonlinear setting. The perturbations used have the property that they are small in every $L^p$ norm, yet they result in solutions which fail to be global.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 18:21:26 GMT" }, { "version": "v2", "created": "Sun, 9 Sep 2007 23:10:03 GMT" } ]
2007-09-10T00:00:00
[ [ "Robinson", "Michael", "" ] ]
0704.3990
Elie Raphael
Alexei Chepelianskii (LPCT, LPS), Fr\'ed\'eric Chevy (LKB - Lhomond), Elie Raphael (LPCT)
On capillary-gravity waves generated by a slow moving object
null
null
10.1103/PhysRevLett.100.074504
null
physics.class-ph
null
We investigate theoretically and experimentally the capillary-gravity waves created by a small object moving steadily at the water-air interface along a circular trajectory. It is well established that, for straight uniform motion, no steady waves appear at velocities below the minimum phase velocity $c_{min} = 23 \rm{cm \cdot s}^{-1}$. We show theoretically that no such velocity threshold exists for a steady circular motion, for which, even at small velocities, a finite wave drag is experienced by the object. This wave drag originates from the emission of a spiral-like wave pattern. Our results are in good agreement with direct experimental observations of the wave pattern created by a circularly moving needle in contact with water. Our study leads to new insights into the problem of animal locomotion at the water-air interface.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 18:24:09 GMT" }, { "version": "v2", "created": "Tue, 1 Jan 2008 16:30:10 GMT" } ]
2009-11-13T00:00:00
[ [ "Chepelianskii", "Alexei", "", "LPCT, LPS" ], [ "Chevy", "Frédéric", "", "LKB - Lhomond" ], [ "Raphael", "Elie", "", "LPCT" ] ]
0704.3991
Alan Kogut
A. Kogut, J. Dunkley, C. L. Bennett, O. Dor\'e, B. Gold, M. Halpern, G. Hinshaw, N. Jarosik, E. Komatsu, M. R. Nolta, N. Odegard, L. Page, D. N. Spergel, G. S. Tucker, J. L. Weiland, E. Wollack, E. L. Wright
Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Foreground Polarization
9 pages with 8 figures. For higher quality figures, see the version posted at http://lambda.gsfc.nasa.gov/product/map/dr2/map_bibliography.cfm
Astrophys.J.665:355-362,2007
10.1086/519754
null
astro-ph
null
We present a full-sky model of polarized Galactic microwave emission based on three years of observations by the Wilkinson Microwave Anisotropy Probe (WMAP) at frequencies from 23 to 94 GHz. The model compares maps of the Stokes Q and U components from each of the 5 WMAP frequency bands in order to separate synchrotron from dust emission, taking into account the spatial and frequency dependence of the synchrotron and dust components. This simple two-component model of the interstellar medium accounts for at least 97% of the polarized emission in the WMAP maps of the microwave sky. Synchrotron emission dominates the polarized foregrounds at frequencies below 50 GHz, and is comparable to the dust contribution at 65 GHz. The spectral index of the synchrotron component, derived solely from polarization data, is -3.2 averaged over the full sky, with a modestly flatter index on the Galactic plane. The synchrotron emission has mean polarization fraction 2--4% in the Galactic plane and rising to over 20% at high latitude, with prominent features such as the North Galactic Spur more polarized than the diffuse component. Thermal dust emission has polarization fraction 1% near the Galactic center, rising to 6% at the anti-center. Diffuse emission from high-latitude dust is also polarized with mean fractional polarization 0.036 +/- 0.011.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 18:38:26 GMT" } ]
2009-06-23T00:00:00
[ [ "Kogut", "A.", "" ], [ "Dunkley", "J.", "" ], [ "Bennett", "C. L.", "" ], [ "Doré", "O.", "" ], [ "Gold", "B.", "" ], [ "Halpern", "M.", "" ], [ "Hinshaw", "G.", "" ], [ "Jarosik", "N.", "" ], [ "Komatsu", "E.", "" ], [ "Nolta", "M. R.", "" ], [ "Odegard", "N.", "" ], [ "Page", "L.", "" ], [ "Spergel", "D. N.", "" ], [ "Tucker", "G. S.", "" ], [ "Weiland", "J. L.", "" ], [ "Wollack", "E.", "" ], [ "Wright", "E. L.", "" ] ]
0704.3992
Birbrair Lev
Lev Birbrair, Dirk Siersma
Metric Properties of Conflict Sets
8 pages
null
null
null
math.MG math.AG
null
In this paper we show that the tangent cone of a conflict set in $R^n$ is a linear affine cone over a conflict set of smaller dimension and has dimension $n-1$. Moreover we give an example where the conflict sets is not normally embedded and not locally bi-Lipschitz equivalent to the corresponding tangent cone.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 18:41:43 GMT" } ]
2007-05-23T00:00:00
[ [ "Birbrair", "Lev", "" ], [ "Siersma", "Dirk", "" ] ]
0704.3993
Sergey Fedosov
S. N. Fedosov, A. E. Sergeeva, A. F. Butenko
Depolarization Currents in Fresh and Aged Corona Poled P(VDF-TFE) Films
5 pages, 2 figures
null
null
null
cond-mat.mtrl-sci
null
Using short circuit and open circuit modifications of the thermally stimulated depolarization current technique, relaxation currents have been measured in corona poled copolymer of vinylidene fluoride with tetrafluoroethylene in samples stored after poling for either 1 day, or 16 month. Two well structured peaks observed in aged samples were attributed to relaxation of electret and ferroelectric components of the remnant polarization. In fresh samples the two components were mixed forming one broad peak. Relaxation of the space charge caused inversion of the current in the open circuit mode both in fresh and in aged samples. Space charge peaks extracted from the total current by appropriate calculations have shown that the trapped charges were more stable than the polarization. It was suggested that both the electret and the ferroelectric components of the remnant polarization were accompanied by either space, or surface charges.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 19:16:57 GMT" } ]
2007-05-23T00:00:00
[ [ "Fedosov", "S. N.", "" ], [ "Sergeeva", "A. E.", "" ], [ "Butenko", "A. F.", "" ] ]
0704.3994
Dawei Chen
Dawei Chen
Covers of Elliptic Curves and the Lower Bound for Slopes of Effective Divisors on $\bar{\mathcal M}_{g}$
41 pages, 19 figures
null
null
null
math.AG math.CO math.GT
null
Consider genus $g$ curves that admit degree $d$ covers to elliptic curves only branched at one point with a fixed ramification type. The locus of such covers forms a one parameter family $Y$ that naturally maps into the moduli space of stable genus $g$ curves $\bar{\mathcal M}_{g}$. We study the geometry of $Y$, and produce a combinatorial method by which to investigate its slope, irreducible components, genus and orbifold points. As a by-product of our approach, we find some equalities from classical number theory. Moreover, a correspondence between our method and the viewpoint of square-tiled surfaces is established. We also use our results to study the lower bound for slopes of effective divisors on $\bar{\mathcal M}_{g}$.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 18:43:14 GMT" } ]
2007-05-23T00:00:00
[ [ "Chen", "Dawei", "" ] ]
0704.3995
Masahico Saito
Kheira Ameur, Masahico Saito
Polynomial cocycles of Alexander quandles and applications
null
null
null
null
math.GT
null
Cocycles are constructed by polynomial expressions for Alexander quandles. As applications, non-triviality of some quandle homology groups are proved, and quandle cocycle invariants of knots are studied. In particular, for an infinite family of quandles, the non-triviality of quandle homology groups is proved for all odd dimensions.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 18:47:03 GMT" } ]
2007-05-23T00:00:00
[ [ "Ameur", "Kheira", "" ], [ "Saito", "Masahico", "" ] ]
0704.3996
Po-Shan Leang
Peter Arnold and Po-Shan Leang
Lessons from Non-Abelian Plasma Instabilities in Two Spatial Dimensions
15 pages, 10 figures
Phys.Rev.D76:065012,2007
10.1103/PhysRevD.76.065012
null
hep-ph nucl-th
null
Plasma instabilities can play a fundamental role in quark-gluon plasma equilibration in the high energy (weak coupling) limit. Early simulations of the evolution of plasma instabilities in non-abelian gauge theory, performed in one spatial dimension, found behavior qualitatively similar to traditional QED plasmas. Later simulations of the fully three-dimensional theory found different behavior, unlike traditional QED plasmas. To shed light on the origin of this difference, we study the intermediate case of two spatial dimensions. Depending on how the "two-dimensional'' theory is formulated, we can obtain either behavior.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 19:00:21 GMT" } ]
2008-11-26T00:00:00
[ [ "Arnold", "Peter", "" ], [ "Leang", "Po-Shan", "" ] ]
0704.3997
Gennadiy Burlak
G.N. Burlak, A.B. Klimov
The solitons redistribution in Bose-Einstein condensate in quasiperiodic optical lattice
16 pages, 6 figures
null
10.1016/j.physleta.2007.05.012
null
nlin.PS
null
We numerically study the dynamical excitations in Bose-Einstein condensate (BEC) placed in periodic and quasi-periodic 2D optical lattice (OL). In case of the repulsive mean-field interaction the BEC quantum tunnelling leads to a progressive soliton's splitting and generating of secondary solitons, which migrate to closest trapping potential minima. A nontrivial soliton dynamics appears when a series of pi-pulses (phase kicks) are applied to the optical lattice. Such sudden perturbation produces a dynamic redistribution of the secondary solitons, leading to a formation of an artificial solitonic superlattice. Different geometries of OL are analyzed.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 19:03:32 GMT" } ]
2009-11-13T00:00:00
[ [ "Burlak", "G. N.", "" ], [ "Klimov", "A. B.", "" ] ]
0704.3998
Arnold W. Miller
Arnold W. Miller
Long Borel Hierarchies
null
null
null
null
math.LO
null
We show that it is relatively consistent with ZF that the Borel hierarchy on the reals has length $\omega_2$. This implies that $\omega_1$ has countable cofinality, so the axiom of choice fails very badly in our model. A similar argument produces models of ZF in which the Borel hierarchy has length any given limit ordinal less than $\omega_2$, e.g., $\omega$ or $\omega_1+\omega_1$. Latex2e: 24 pages plus 8 page appendix Latest version at: www.math.wisc.edu/~miller
[ { "version": "v1", "created": "Mon, 30 Apr 2007 19:06:50 GMT" } ]
2007-05-23T00:00:00
[ [ "Miller", "Arnold W.", "" ] ]
0704.3999
Julius Kuti
Chuan Liu
Strongly Interacting Higgs Sector Without Technicolor
156 pages, 25 figures, Ph.D. Thesis (1994)
null
null
null
hep-ph
null
Several years ago, we proposed a modification of the Standard Model, in which the Higgs sector was stabilized by the addition of higher derivative operators, similar to Lee-Wick Electrodynamics. We studied this theory extensively, both using continuum Hamiltonian and path integral methods. We also reported detailed lattice studies of the higher derivative Higgs sector. In view of some recent revived interest in our original idea, we are providing here our extensive notes from the time period on this topic. The key results were already published in our papers at that time. The many additional details that we make available here were previously available only in Chuan Liu's UCSD Ph.D. thesis (1994). Very recently, our idea has been revived by other groups. In view of the renewed interest, and to perhaps correct some misconceptions in the literature, we are here making our original extensive notes available to the wider community.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 19:07:26 GMT" } ]
2007-05-23T00:00:00
[ [ "Liu", "Chuan", "" ] ]
0704.4000
Erhan Iltan
E. O. Iltan
Radiative lepton flavor violating decays in the Randall Sundrum background with localized leptons
23 pages, 10 figures, 2 tables
Int.J.Mod.Phys.A23:1055-1073,2008
10.1142/S0217751X08039748
null
hep-ph
null
We study the radiative lepton flavor violating l_i -> l_j\gamma decays in the two Higgs doublet model, respecting the Randall Sundrum scenario and estimate the contributions of the KK modes of left (right) handed charged lepton doublets (singlets) on the branching ratios. We observe that the branching ratios are sensitive to the contributions of the charged lepton KK modes.
[ { "version": "v1", "created": "Mon, 30 Apr 2007 19:32:07 GMT" }, { "version": "v2", "created": "Mon, 25 Feb 2008 12:24:06 GMT" } ]
2008-11-26T00:00:00
[ [ "Iltan", "E. O.", "" ] ]