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Methodologic strategies in the modern cosmology and their foundations
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Jakov V. Tararoyev, Albert T. Kotvitzky, Igor P. Biletsky
Kharkiv National University named after V.N. Karazin
Pl. Svobody, 4, Kharkov, Ukraine, 61 077
The article is dedicated to ontological foundations (or their elements) in cosmology. A detailed analysis of one of the modern cosmology main problems, the problem of dark energy is represented. It'-s demonstrated that in spite of a sufficient quantity of the empirical facts which may be interpreted as an accelerated expanding of the Universe and also the dark energy as a cause of this expanding the nature of the latter may be understood differently. It'-s impossible to choose a mode of understanding empirically but necessary to consider according methodology tied with ontological principles.
Key words: cosmology, dark energy, methodological approach, ontology.
The problem of ontological foundations of scientific knowledge appeared in the philosophy of science not so long ago. If we start counting the time of appearing the philosophy of science from the emergence of positivism, represented by A. Comte, J.S. Mill, H. Spencer, then in the frame of the latter the problem was not only formulated but also solved in its first and unequivocal variant. According to it, & quot-metaphysic"- elements of scientific knowledge must be eliminated from science, for they make vague an essence of things discovered empirically (e.g. [1]). Knowledge itself must be based on a unity of an authentic empirical experience and strict logical approaches. Corresponding methodological settings negating any significance of ontological foundations of scientific knowledge and affirming productivity in the sense of authenticity of empirical, mathematical and logical methods of a scientific investigation were characteristic to neopositivism as well. However, beginning from 30s of the XXth century, at first in works of K. Popper and from 60s in works of some other authors, inconsistency of this approach was demonstrated. In some conceptions of scientific knowledge suggested by Thomas Kuhn, Imre Lakatos, Paul Feurabend, Michael Polani, Stephen Toulmin and some others, whose ideas had obtained the name of postpositivism, the significance of an ontological knowledge was not negated and even more in some of them as, for example, in the conception of T. Kuhn the necessity of & quot-metaphysic elements& quot- of science as its obligatory structure units was affirmed.
The increasing complexity of the scientific knowledge itself and, beforehand, the physical knowledge that, beginning from the crisis of the XIX-XXth centuries'- boundary, didn'-t fit to the positivistic frame promoted this revision of the positions. Mathematical, logical, empirical methods traditional to the nature disciplines by themselves were unable to explain the investigated reality uniquely and comprehensively. Theoretic approaches and principles as well as empirical data allowed describing the reality by means of different, sometimes excluding each other models. Choice of the most optimal and adequate description required considering a wider specter of questions, in particular the question of existing, its criteria and properties or, as a matter of fact, the question of ontology and its using as one method else together with other ones traditional to nature science. This situation was characteristic not only to physics but also to some other disciplines, beforehand, related to it.
It'-s necessary to note that earlier, already in the first half of the XXth century choice problems of some or other theoretical model from the models variety suggested by theorists occurred as well. Still the relativistic cosmology supposed different models of the Universe which obtained the names of the open, closed and flat Universes. Accordingly, the first was seen infinitely expanding and with an infinite volume, its geometry was non-Euclidean with a negative curvature. In the second the expanding in the process of evolution was necessarily changed with a compression, its volume was finite and space was described by a non-Euclidean geometry with a positive curvature. The flat Universe had also an infinite volume and expanded for infinite time but its geometry was Euclidean. Choice of that or other model was determined by observable data of the middle density of the Universe. If the density is less than a critical value p & lt- pcr, the open model is realized- if it'-s greater p & gt- pcr, the closed one is- in the case of equality p = = pcr, the flat model corresponds to the real Universe. The value of the critical density pcr = 3H2/8tcG (where H is a constant of Hubble and G is a gravitational constant) is determined within the relativistic cosmology theory and compounds 9,31×10−30g/cm3.
The problem of model choice from the variety of variants is determined certainly with no ontological criteria but empirical data that simplifies the situation. Nevertheless these data have a certain ontological implied sense and before initiating observance of some objects making a contribution into the middle density in the Universe it'-s necessary to clear up these objects existence. In the case of the relativistic cosmology the task was solved by no ontology but all the set of physics, astronomy and cosmology theoretical and empirical data. However, in the XXIst century these data are not sufficient. It concerns, beforehand, a discovered in the end of the XXth century phenomenon of the Universe accelerated expanding (e.g. [2- 3- 4]). Conception of this phenomenon exceeds from observing supernova stars SNIa. These stars are & quot-standard candles& quot- for determining cosmologic (i.e. very great) distances. The term of & quot-standard candle& quot- means we know an absolute brightness of these stars. Comparing a visible brightness of the star with its absolute brightness we can conclude of the distance to it by formula m — M = = 5lg dL + 25, where m is the visible brightness, M the absolute one and dL the normalized photometric distance. On the other hand, the same photometric distance is a func-
tion of red shift z and the from of the function includes also relative densities taken in a certain moment of time Qm0, Qr0, QA0, Qk0. They are, accordingly, the densities of
substance, radiance, the density bound with repulsion & quot-powers"- (the so-called J-term) (1) and that bound with the curvature of space. Comparing the photometric distances obtained by these two modes showed they coincide in Euclidean (or quasi-Euclidean) cos-mologic models with Qk0 «0 (2) only in the case if QA0 is much more zero. Accordingly, if QA0 = 0 then the supernova SNIa look dimmer that they must be. The latter
shows that one factor else influences the evolution of the Universe and unlike the substance it doesn'-t brake but accelerates its metric evolution.
Discovering of the accelerated expanding of the Universe in astronomical observations actualized the problem of ontological foundations of scientific (in particular cosmological) knowledge. It became an actual not directly, through observance (how it was in the relativistic cosmology where the theory advanced empirical data). Now it'-s actualized directly, through introducing the question of criteria, principles, properties, attributes of the existing because all the latter in implicit or explicit form enters the structure of the theory that lags behind the empirical data in question of the Universe accelerated expanding. In comparison with the relativistic cosmology of the first half of the XXth century the task of a model choice got complicated essentially for now it isn'-t a choice of a model of one single theory. In the case of the Universe accelerated expanding we meet several theories from which a unique choice must be done. Let'-s consider the main of the latter.
It'-s evident from a simple physical reasoning that if two (or some other quantity) bodies are flying apart in a space where there is nothing except them, then the speed of their flying apart will be gradually decreasing because of their mutual gravitational attraction. If in the initial moment their kinetic energy is more than their mutual potential energy, then they'-ll fly apart to infinity and there they'-ll possess a nonzero speed. In the case of the kinetic and potential energies strict equality in the initial moment the two bodies also fly apart to infinity but there their speed will be equal to zero. If the kinetic energy is less than the potential one, then the two bodies will go at some distance from each other, where they'-ll stop and start the opposite movement. Namely these three models of the Universe (the above open, closed and flat Universes) were the chief before the discovering of the accelerated expanding. Using this reasoning to the accelerated expanding of the Universe means that the & quot-factor"- of the potential energy responsible for retardation of interacting bodies'- movement is outweighed by the factor accelerating this movement. That means a gravitational repulsion (anti-gravitation) exists and this anti-gravitation has a cause in the form of an object engendering it. This object has a principally other nature than the gravitational field well-known from the time of Newton. It had been known before but its property of repulsion was discovered for the first time namely in the accelerated expanding of the Universe. This approach is one of three main approaches in the description of the phenomenon of the Universe accelerated expansion. Accordingly to it, the cause of the Universe accelerated expansion may be represented with an object whose essence is a fundamental base of the physical being and whose specifics determines the latter phenomenon. This object obtained the name
of the dark energy. The concept of energy was used because of the repellent (kinetic) energy the object possesses and the term & quot-dark"- characterizes the accelerating energy in that attitude that is invisible in any gamut of electromagnetic spectrum.
Now several candidates of different nature apply for the place of the dark energy (e.g. [5]). However, from the formal mathematical point of view all of them have the same origin — the relativistic cosmology. Its theoretical base is a system of equations called the Friedman equations. There are one algebraic and two differential equations and, accordingly, three parameters: a gauge factor a and its derivatives by time, the density of energy s and pressure p in this system. Two the latter are bound with each other by the same algebraic equation called the equation of the state p = ws. The proportionality coefficient w does determine the difference between the applicants for the dark energy. Variety of different variants of the dark energy may be represented in the table:
Value w w & lt- -1 w= -1 -1 & lt- w & lt- -1/3 w = -2/3
Name of the dark energy Phantom energy Physical vacuum Quintessence Domain walls
Value of the coefficient w is defined from observance. The simplest candidate to the dark energy is the physic vacuum. However, attempts of evaluating the density of the vacuum energy give either too great value or infinite one in general. As zero oscillations of any quantum field have energy h® /2, the density of the energy is defined with an integration dispersing at infinity and therefore it'-s obtruncated with an effective maximal impulse kmax (the parameter of obtruncating). In order to demonstrate the value
problem one may take out only one quantum field and consider that the energy density obtained in this way cannot be more some critical density for the Universe and the obtruncating parameter must be less than 0. 01 eV, that is much less than any scale of energy in the physics of elementary particles. If we take the scale of the Plank energy: ~ 1019 GeV as a parameter of obtruncating, supposing thereby that quantum theory of field stop working in the classical space-time, then the density of the zero oscillations energy will be 120 orders of magnitude more than the critical density in the Universe. This great discrepancy got name of the cosmologic constant problem. A possible exact supersymmetry between bosons and fermions could compensate the odds. The problem, however, consists that in no superparticle has been discovered in experiments. That means the supersymmetry (if it exists) is broken and superpartners have different masses. Experiment gives possibility of existence of particles with masses of the order of magnitude about 1 TeV, that means the difference is compensated instead of 120 we have now 60 orders. The value is too great all the same.
Another approach to problem of the cosmological constant is based on supposition that numerical characteristic of the vacuum energy is a casual value and can accept different meanings in different untied fields of the space. Then in the fields where the value of the cosmological constant occurred being too great no emergence of galaxies, star systems and as a result of a life similar to that of humans is possible and we are namely in that part of the multiversum where auspicious values of the world constants occurred. These theoretical problems as well as the fact that the observable values give w ^ -1 make us to look for other candidates to the dark energy.
The vacuum energy remains unchanged in both space and time, that determines simplicity of the above approach. However, it'-s possible to introduce an additional freedom degree (as a matter of fact an additional parameter characterizing the dark energy) the scalar field 9 for understanding the nature of the dark energy in general and explaining possibilities of existence of other, more complicated applicants to the name of the
dark energy. As the Lagrangian of the scalar field is L = 1 ^99 — V (9), so the density
of energy and pressure are defined with s = 9 + V (9), p = 9 — V (9). Evolution of
the field 9 is defined with an equation 9 + 3H 9 = -V '-(9). The coefficient of proportionality between the pressure and density of energy actually determines a dynamics
.. f-V& lt-9)
of the Universe development. In case of the scalar field it'-s defined as w = -4
f + V (p)
and may change in dependence on speed of changing (evolution) of the scalar field. Thus, if the field changes slowly then cp ^ 0 and therefore w = -1. This corresponds to the cosmological constant. If the field changes quickly, then cp & gt->- V (p) and w = +1. This corresponds to the maximum hard equation of the state. So w is situated in interval from -1 to +1.
The scalar field is introduced as a free parameter, however, its introduction isn'-t absolutely an arbitrary process. We must take into consideration the observed reality conditions called the & quot-problem of coincidence& quot- in the standard cosmological model. Entity of the problem consists in the question why namely at modern stage of the Universe evolution the vacuum'-s and dark substance'-s inputs are commensurable, whereas the substance'-s one prevailed in past and that of vacuum will do in future and what has formed the conditions led to it.
At least two approaches to solving this problem exist. The first is represented with the so-called freezing models where the scalar field is introduced in the way providing, on the one hand, an accelerating expanding of the Universe and, on the other hand, an approximate dynamic coincidence of the dark and other energies'- density. Another approach is suggested with thawing models where the coincidence of these two values is really a casual event defined with the value of the scalar field mass.
In the case of -1 & lt- w & lt- -1/3 (that means the dark energy is realized in quintessence) its (quintessence'-s) dynamic behavior is defined with choice of the potential to the scalar field. Also consideration of a modified canonical form of the kinetic energy for the field p is possible theoretically. In particular change of the sign in the kinetic item makes these models unstable [6], however, ability of effective obtaining the value w & lt- -1 corresponding to the phantom energy appears. In still more complicated models the kinetic item depends on the scalar field itself [7].
Thus, the scalar field models put new questions and opened new abilities: — e.g., are the cosmologic acceleration and inflation bound? In both cases an accelerated expanding inexplicable with the scalar field dynamics emerge-
— is the dark energy bound with the dark substance and the mass of neutrino?
— the scalar field dark energy unlike the vacuum dark energy can be inhomoge-neous and as a result lead to some observable peculiarities.
The object which is the cause of the Universe accelerated expanding may be either physical vacuum or scalar field. The choice of the according approach is determined eventually by observing the value w. An object else that can explain the Universe accelerated expanding is a substance with exotic equations of its state (e.g. [8]). As an example the Chaplygin gas may be put. However, both scalar field and exotic equations of the state may be conditionally grouped into one of three methodological approaches whose ontological foundation is included into affirmation of existence of a new object responsible for the Universe accelerated expanding. This strategy may be conditionally called the strategy of a new object. The choice within it is made with basing on empirical data, however, this choice as well as that of some other rival strategy is beforehand the ontological choice of investigator. Let'-s consider two other strategies.
The next is the strategy of modified (alternative) gravitation (e.g. [9- 10- 11]). It has some methodological advantages before the strategy of a new object. They are:
1. It provides a natural gravitational alternative to the dark energy and no necessity to introduce a new object of reality emerges. In this sense the strategy of modified gravitation accords more to the principle of the Occam'-s razor than the strategy of a new object.
2. It unites naturally the earlier inflationary stage in development of the Universe and the modern accelerated expanding that solves automatically questions emerging the modified theories of the scalar field.
3. It can be a foundation to a united explanation of the dark energy and dark substance (curves of the galaxies revolving).
4. It can explain transition of the Universe from usual expanding to possible phantom expanding without introducing the dark energy.
5. It describes a virtual transition from the delayed to accelerated expanding of the Universe.
6. It'-s useful in descriptions of the high-energies physics.
7. Some expanded models compete with the general relativity theory and give coincident results in weak gravitational fields (of the Sun and Earth).
The idea of alternatives theories of gravitation consists in modification of fundamental principles of the classical gravitation theory. They may be divided into the follow classes:
— Metrical theories (the Logunov'-s relativistic theory of gravitation, the gravitation theory of highest degrees of curvature etc.) —
— Unmetrical theories (as the Einstein-Cartan theory) —
— Vector theories-
— Scalar tensor theories (for example, the Jordan-Brans-Dicke theory) —
— Theories alternative to the classical Newton'-s theory (as the Le Sage theory and modified Newtonian dynamics) —
— Theories of quantum gravitation (e.g., those of canonical quantum gravitation, loopback quantum gravitation etc.) —
— Theories of different physic interactions unification (such as the string theory, the theory of supergravitation, the theory of brane and others).
Aims of alternative theories of gravitation unlike those of the standard cosmologi-cal model elaborated on the base of the general relativity theory are more general and include solutions of some other tasks such as elaboration of a unified field theory, theory of everything (TOE) etc.
Last time the theory of the highest curvature degrees belonging to the metrical alternative theories plays an important role in theoretic cosmology. Gravitation of the highest curvature degrees demonstrates an equivalent accordance with the standard cos-mological model. However, unlike the latter the gravitation theory of the highest curvature degrees doesn'-t require new entities (objects) and is based only on a supposition about more general than in the classical general relativity theory principle of least action. Using of the modified gravitation and in particular the gravitation theory of the highest curvature degrees in cosmology may give results corresponding to the standard classical model. And because of that the idea of this and other models doesn'-t limit choice of the Lagrange density concrete form, it'-s evident cosmological solutions completely corresponding to models of the dark energy can be obtained. The alternative gravitation giving results equivalent to the dark energy model has an advantage in natural mode of modifying cosmological equations without necessity of introducing new exotic forms of the material.
The third methodological approach with its own ontological foundation may be called a strategy of other possibilities. It supposes explanations unbound with introducing special objects and using gravitation. All these explanations are very diversiform and we put only several of them as examples.
Perturbation of metrics. In this case it'-s sufficient, using a standard inflationary model, to introduce gravitational ripple at initial stages of the Universe evolution in order to explain the observed expanding without introducing the dark energy or modifying the theory of gravitation. & quot-We introduce no new entities into the Universe and suggest an explanation in the frame of one of possible variants of the Big Bang standard theory, namely in the frame of the inflationary model suggested as early as in 1981, underlined one of the authors of the article, Antonio Riotto from the Italian Institute of the Nuclear Physics, We understood that'-s sufficient to introduce this key element the gravitational ripple at earlier stages into the Einstein'-s general relativity theory in order to explain the observable acceleration of the expanding Universe. And there is no necessity to invent mysterious phantoms like a dark energy& quot- (e.g. [12]).
Preferential state. Let'-s suppose the tempo of expanding becomes slower everywhere as far as the material brakes it in the space-time. Let'-s suppose further that we live in a gigantic cosmic void which is, of cause, not complete void but its middle substance density two-threefold less than somewhere else. The emptier an area is, the lesser quantity of substance it contains and, accordingly, the tempo of expanding is greater in limits of the void than anywhere else. The quickest tempo of expanding is observed in the center of the void, it becomes slower towards the limits whre the greater density is. In any moment different parts of the space expand with different speed as well as an inflated balloon. This idea was suggested for the first time by George Ellis, Charles
Hellaby and Nazeem Mustapha from the Cape Town university in South Africa (e.g. [13]) and developed later by the Paris observatory.
Cosmic soot. Andrew Steele and his colleague Marc Fries from Institution for Science in Washington DC discovered a whiskering graphite (consisting of high-modulus coal fibrils joined by strongest crystals of alongated form of only several micrometers length) ingrained in the rock formed under ancient high temperature of new-born suns and exploding stars. According to them, wide clouds of this graphite can surround practically all stars, decreasing thereby luminosity of both usual and supernova stars. This discovery will scarcely allow completely to refuse from the dark energy but the hazing effect must be taken into consideration and studied [14].
Cosmological averaging. This approach is based on historic parallel between ether (the XIX-XX boundary) and dark energy (the XX-XXI boundary). It summarized the week and strong principles of equivalence (the first asserts that in every point of the space-time in an arbitrary gravitational field it'-s possible to establish a coordinate system in which the laws of movement will be the same as in a not accelerated Cartesian axils, the second generalized the first to all the nature laws besides the laws of movement) to the cosmological principle of equivalence. Essence of this generalization consists in that always and everywhere it is possible to point out certain vicinity of the spacetime, a cosmological inertial system where middle (time- and light-alike) movements can be described geodesic in the Minkowski geometry with exactitude to a conform transformation. However, it'-s impossible to introduce a system describing all the Universe. I.e. the Universe is subdivided into domains described with a FRW metrics but no general metrics of this kind can be. Thus, laws of nature are fulfilled by an averaged space-time of the Universe. Averaging must be led by local domains with using special mathematic methods of averaging and different local domains are homogenous and isotropic but differing each other.
For the Universe develops against a curved background, the weak field limit isn'-t admissible and, therefore, a relatively small deceleration of the local domain'-s middle background can lead to great changes in the clocks normalization that can lead in its own turn to different observable (apparent) effects, for example, to an accelerated expanding of the Universe (e.g. [15- 16- 17]).
Thus, we may summarize certain results. The Universe accelerated expanding discovered in 1998 engendered a new situation in the modern cosmology. Scientific society suggested three strategies for seeking and describing the causes of this acceleration. The first may be called the strategy of the dark energy. A new physical object that obtained this name is considered responsible for the Universe accelerated expanding. The second strategy may be called the strategy of the modified (alternative) gravitation. Gravitation is considered the cause for the Universe accelerated expanding in its frame and the acceleration itself is a new, unknown before property of the gravitation. The third strategy is that of other possibilities, its essence consists in explaining the Universe accelerated expanding without introducing special new objects or addressing to gravitation. This strategy is remarkable with that the objects explaining the accelerated expanding or rather its observable effects are very various by their nature.
These three strategies with different ontological fundamentals (dark energy, gravitation, other objects) fit completely to the modern tendencies of the scientific knowledge development. In short these tendencies may be describes as follows. A transformation in objects of physical knowledge occurred from the beginning of the XXth century. The objects of physical investigation lost their visual character already in the Maxwell electrodynamics, thermodynamics, statistical physics and especially in special and general relativity theories, quantum mechanics, physics of elementary particles. Unlike the objects of reality in the old physics which were physical bodies interacting by means of forces (phenomenology of Newton) the objects of the new physics are particles, fields, quanta, space-time. These objects unlike bodies given to our direct perception should be considered rather logical constructs consisting of according properties. We deal with sensual data in the empirical material and with logical properties in mathematical and theoretical models. These properties are primary data for us, the objects are constructed of them. All this is just for the problem of the accelerated expanding in full measure. Empirical properties of this phenomenon are given us in empirical data and we fill them with some or other theoretical properties, depending on our methodological strategy. And in accordance with an accepted strategy we obtain some or other object as a cause of the Universe accelerated expanding. The problem and specifics of cosmology consists in that empirical properties given us in observation may be endorsed in any of the represented strategies. The choice of some or other strategy isn'-t determined by empirical factors. The choice is beforehand a theoretical choice where not empirical but theoretical factors prevail. In this context the Godel theorem or rather, strictly speaking, its corollary according to which it'-s impossible to set a verity or falsity of a formal system in the frame of the same system. Outer foundations are necessary for it. Different extra-scientific including ontological foundations may play the role of these outer foundations. Setting of some or other properties, attributes or criteria of existence will promote choice of the object responsible for the Universe accelerated expanding and methods of its cognizing in the choice of methodological strategy.
The situation that has developed in the modern cosmology may be estimated as critical, at least from the point of norms, methods, rules and principles used in nature science during several last centuries. However, if we consider science in a wider historic perspective, we shall see that similar situations occurred. As an example the concurrence of two ontological methodological strategies that emerged still in the antique physics. We mean strategy of atomists, according to whom anything is atoms, and that of Aristotle, who said anything is body. The results of the competition were influenced with both scientific (impossibility of direct empirical data concerning atoms) and extra-scientific (& quot-canonization"- of the Aristotle'-s works and anathema to atomism from the side of the Christian church) factors. The Aristotelianism victory, its creative reformulation in the New Time and creation of the classical mechanics as a physics of bodies eliminated atomism. Its return as an ontological methodological strategy in the second half of the XIXth century occurred when the strategy of bodies couldn'-t explain some empirical data (the principle of the mechanical work-heat identity proved experimentally by Joule). Let'-s hope the choice between three ontological methodological strategies in explaining the phenomenon of the Universe accelerated expanding won'-t last for mil-
lenniums. Probably the precipitant progress of science and technologies will be able to give all necessary proofs in favor of one of the above hypotheses but until it'-ll occur they will develop parallelly in accordance with own scientific and extra-scientific foundations including the ontological ones.
(1) The-term was introduced for the first time into the cosmological equation of gravitational field by Einstein himself in order to obtain a model of a stationary Universe. In this model the member bound with the-term described some repulsion phenomenon and was to compensate activity of the member bound with presence of the attracting substance. Later Einstein called using the-term a & quot-greatest mistake of his life& quot-. Cosmologic models with the-term appeared in cosmology in the end of the 60s of the XXth century.
(2) Zero curvature of the Universe was deduced with other independent modes.
[1] Kuhn, T.S. The Structure of Scientific Revolutions. — Chicago, 1962.
[2] Aldering G. Supernova Acceleration Probe: A Satellite Experiment to Study the Nature of the Dark Energy / G. Aldering, W. Althouse, R. Amanullah, J. Annis, P. Astier and other // arXiv: astro-ph/405 232 v1. — Access Mode magazine: http: //xxx. lanl. gov
[3] Perlmutter S. Measurements of Omega and Lambda from 42 High-Redshift Supernovae / S. Perlmutter, G. Aldering, G. Goldhaber and others //The Astrophysical Journal. — Volume 517. — Issue 2. — 1999.
[4] Riess A. Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant / A. Riess, A. Filippenko, P. Challis and others // The Astronomical Journal. -Volume 116. — Issue 3. — 1998.
[5] Padmanabhan T. Cosmological constant — the weight of the vacuum / T. Padmanabhan // Review Article Physics Reports. — Volume 380. — Issues 5−6. — 2003.
[6] Carroll S. Can the dark energy equation-of-state parameter w be less than -1? / Carroll Sean, Hoffman Mark, Trodden Mark // Physical Review D. — Volume 68. — Issue 2. — 2003.
[7] Armendariz-Picon C. Dynamical Solution to the Problem of a Small Cosmological Constant and Late-Time Cosmic Acceleration / C. Armendariz-Picon, V. Mukhanov- Paul J. Steinhardt // Physical Review Letters. — Volume 85. — Issue 21. — 2000.
[8] Carturan D. Cosmological effects of a class of fluid dark energy models/ D. Carturan F. Fi-nelli // Physical Review D. — Volume 68. — Issue 10. — 2003.
[9] Goheer N. Coexistence of matter dominated and accelerating solutions in f (G) gravity / N. Go-heer, R. Goswami, P. Dunsby, K. Ananda // Physical Review D. — Volume 85. — Issue 12. — 2009.
[10] Uddin K. Cosmological scaling solutions in generalised Gauss-Bonnet gravity theories / K. Ud-din, J. Lidsey, R. Tavakol // General Relativity and Gravitation. — Volume 41. — Issue 12. — 2009.
[11] Bohmer Ch. Stability of the Einstein static universe in modified Gauss-Bonnet gravity / Ch. Bohmer, F. Lobo // Physical Review D. — Volume 79. — Issue 6. — 2009.
[12] Basilakos S. Cosmic acceleration without dark energy / S. Basilakos, M. Plionis // Journal of Physics: Conference Series. — Volume 189. — Issue 1. — 2009.
[13] Nazeem M. The distortion of the area distance-redshift relation in inhomogeneous isotropic universes / M. Nazeem- B. Hellaby, Ch. Ellis // Classical and Quantum Gravity. — Volume 15. — Issue 8. — 1998.
[14] Fries M. Comet 81P/Wild-2 Carbon — An Extraordinarily Diverse Suite of Materials / M. Fries, A. Steele // 41st Lunar and Planetary Science Conference, held March 1−5, 2010 in The Woodlands, Texas. LPI Contribution. — № 1533. — 2010.
[15] Wiltshire D. From Time to Timescape — Einstein'-s Unfinished Revolution / David L. Wiltshire // International Journal of Modern Physics D. — Volume 18. — Issue 14. — 2009.
[16] Wiltshire D. Average observational quantities in the timescape cosmology / David L. Wiltshire // Physical Review D. — Volume 80. — Issue 12. — 2009.
[17] Wiltshire D. Gravitational energy as dark energy: Average observational quantities / David L. Wiltshire // INVISIBLE UNIVERSE: Proceedings of the Conference. AIP Conference Proceedings. — Volume 1241. — 2010.
Харьковский национальный университет имени
Статья посвящена онтологическим основаниям (или элементам) в современной космологии. В ней представлен детальный анализ одной из основных проблем современной космологии — проблемы темной энергии. Показано, что несмотря на достаточное количество эмпирических фактов, которые можно интерпретировать как ускоренное расширение Вселенной и соответственно как наличие причины этого ускорения — темной энергии, природа этой темной энергии может пониматься различным образом. Выбор среди всех этих пониманий однозначно не может быть осуществлен эмпирически, и для его реализации необходимо обращаться к методологии, связанной с онтологическими принципами и правилами.
Ключевые слова: космология, темная энергия, методологический подход, онтология.


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Nam June Paik, 19322006
In Memoriam
Nam June Paik, 19322006
Nam June Paik, the color-addicted, chaos-loving, more-is-more cosmographer of the cathode tube, who in the early 1960s began piling boodles of television sets into stacks and setting them into grids while altering video feeds, causing images to wobble, go fuzzy, turn abstract, and get psychedelic, died last week at the age of 74. This Korean born puckish progenitor of what is now known as "video art" and coiner of the two terms "electronic superhighway" and "the future is now," was clearly a mannerist poet of overkill and discordant drown-out. His revelry will echo on.
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Loss of Erection
Till couple of months ago everything was fine but off late I am not getting erection. even if I manage that it subsides during foreplay and not able to penetrate. Im a diabetic but well in control with HbA1c of 6.7. please suggest.
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Dr. Suresh Radhakrishnan
3 yrs. of exp | Chennai | Urologist
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Pet Sitter in Antigonish
My name is Samantha Wilson, I am a musician and lover of animals and offering PetCare services. I have had several dogs and cats growing up and have been the primary care giver as well as assisted in training them. I am a compassionate, responsible, and dedicated person. If you need someone to walk your dog, or come pet sit over night I can help you out!
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Newton Mayor Setti Warren's campaign for U.S. Senate is more than $22,000 in the hole, according to just released Federal Election Commission reports.
Newton Mayor Setti Warren's two-month old campaign for U.S. Senate is more than $22,000 in the hole, according to just released Federal Election Commission reports (PDF)
As of June 30, Warren's campaign reported having $54,736 cash-on-hand, but $77,513 in debts.
The report says Warren owes $7,500 to his campaign manager Deborah Shah's consulting company Management Partners. Warren already owed Shah $12,000 dating back to 2009, according to his last mayoral finance report filed with the state Office of Campaign and Political Finance in January 2011.
Warren's campaign spokesman Chuck Gilboy told the Newton TAB that the candidate's outstanding debt is largely from investments made at the beginning of the campaign.
Overall, Warren's campaign reported spending $69,374 during the reporting period.
"We wanted to build a strong infrastructure to bring our message out to voters across the state and really get out there and engage with folks on the ground and we've been doing that," said Gilboy, adding that the investments are paying off with a jump in polling numbers. "We're going to continue to be out there aggressively building relationships across the state and raising the necessary resources to build a strong campaign."
Included in the earlier expenses is $10,340 Warren spent for his campaign launch video. Warren still owes the amount to the Arlington, Va., based Putnam Partners. According to its website, Putnam Partners produced television advertisements for three presidential campaigns including Barrack Obama's. Warren's campaign also owes money to Putnam Partners for travel expenses as well.
The campaign also owes $9,250 to Liberty Concepts, based out of Allston, Mass., for developing Warren's website. Warren's campaign also reported owing money to the Washington, D.C.-based political consulting firm Buzzmaker.
The campaign raised $123,636 from 374 donations - not including a $500 donation from the Carpenters Union Local 275 and two $50 contrbutions Warren gave himself - from May 3 through June 30 – the close of the reporting period.
Warren, who previously worked for the Clinton administration and on Sen. John Kerry's presidential campaign, received numerous donations from Washington, D.C. including from the Heinz family.
Warren spent $100 of his own money on the campaign.
The mayor also received donations from city politicians, including $500 from former Newton Alderman Bill Brandel, who is volunteering as a consultant on the campaign, and current Alderman John Freedman who donated $2,500.
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Bwoglines: Our Strange City
Written by Bwog Staff
October 11, 20097:57 am 0 Comments
Fairway is the best way, reason no. 1362: bodegas charge nearly twice as much for grocery staples. (New York Post)
Open House New York ends today–check out this 53rd Street MTA Powerstation, designed with help from our old friends McKim, Mead and White. (Gothamist)
New York in a box! A man sends his soldier pal "the ultimate Gotham care package." (NYT)
A large, large woman sits on a fellow gym-goer in an attempt to reclaim her spinning bike. Naturally, the sittee is suing. (New York Post)
A brave fisherman saves the driver and two passengers of a car that found its way into Sheepshead Bay. (Gothamist)
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SAL RODRIGUEZ: Americans with Disabilities Act has been abused
Abusing well-intended laws for financial gain has become a pastime in states like California.
When President George H. W. Bush signed the Americans with Disabilities Act into law in 1990, the intent was to enhance the quality of life for persons with disabilities by prohibiting discrimination.
Removing barriers to employment and public accommodations are the cornerstone of the law. State governments primarily are responsible for seeing that the goal of expanded accommodations is realized and provide different legal remedies to violations.
California building codes and business regulations are designed to ensure compliance with the federal law. Businesses can use only certain types of door knobs, parking spaces must be within precise dimensions and signage rules must be obeyed.
At the time the ADA was enacted, California already had its own anti-discrimination law, the Unruh Civil Rights Act, which prohibits discrimination on the basis of categories like age, sex and disability. Plaintiffs filing suit under the Unruh Act are entitled to no less than $4,000 in damages.
The state effectively has paired the ADA with the Unruh Act, so that violations of the ADA are subject to the remedies provided through the pre-existing state law.
In practice, this has incentivized wave after wave of lawsuits filed or threatened against business and property owners across the state. No matter how small the violation, be it improper bathroom dimensions or signage, the $4,000 minimum damages are state law.
Between 2005 and 2014, over 7,000 ADA lawsuits were filed across the state – most by serial filers who sued at least 30 times.
One of the more infamous offenders in the past decade was Theodore Pinnock, a disabled San Diego lawyer who filed at least 1,000 ADA lawsuits.
Pinnock came to national attention after demanding varying sums of money from small business owners in the historic town of Julian, California. If business owners did not send the money, Pinnock threatened costly lawsuits for noncompliance with the ADA. Many businesses complied, while others were taken to court.
Pinnock later would be disbarred for unrelated reasons, but shakedowns of businesses in that style persist throughout California.
State legislators have been slow to protect business owners from lawsuit abuses. In 2012, the state prohibited letters demanding money in exchange for not filing a lawsuit. Litigators simply adjusted by skipping the letters and just filing lawsuits.
In Riverside County, businesses have been forced to shell out thousands of dollars, or even close entirely, due to ADA lawsuits. Kuma Tire & Wheel in the city of Riverside paid $8,000 to settle a lawsuit for not having a marked handicapped parking spot. Pablo and Maria Mercado in Woodcrest were forced to shut down their fruit stand because they could not afford to bring their restroom into compliance after being hit with a lawsuit.
In the past year, dozens of business and property owners in the county reported receiving letters and visits from Rodolfo de Hoyos, including the Greater Riverside Chambers of Commerce.
Mr. de Hoyos presented himself as an advocate for people with disabilities and an owner of ADA Advocates and Consulting. He was arrested April 30 on felony charges, including extortion, grand theft and money laundering.


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A classic, gracious apartment building from the 1920's, featuring:
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Kesprytt III
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Kesprytt III was the inhabited third planet of its star system. This was the homeworld of the Kesprytt. The planet was divided into two large nation-states controlled by the Kes and the Prytt.
During the 24th century, the Kes was the larger of the two nations, comprising three quarters of the planet's population, while Prytt contained the remaining one quarter of the population. The two nation-states had a paranoid dislike of each other, bordering on xenophobia.
In 2370, the Kes applied for an "associate" Federation membership, as an exception to the normal rule requiring a planet be unified socially and politically for membership. The application for the admission of Kes to the Federation was rejected due to the unresolved social, political, and military problems between the two nations. (TNG: "Attached")


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Chicago Heights Dog Rescue
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YP - The Real Yellow PagesSM - helps you find the right local businesses to meet your specific needs. Search results are sorted by a combination of factors to give you a set of choices in response to your search criteria. These factors are similar to those you might use to determine which business to select from a local Yellow Pages directory, including proximity to where you are searching, expertise in the specific services or products you need, and comprehensive business information to help evaluate a business's suitability for you. "Preferred" listings, or those with featured website buttons, indicate YP advertisers who directly provide information about their businesses to help consumers make more informed buying decisions. YP advertisers receive higher placement in the default ordering of search results and may appear in sponsored listings on the top, side, or bottom of the search results page.
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International Law in the U.S. Supreme Court: Continuity and ChangeBy: Michael D. Ramsey (editor), David L. Sloss (editor), William S. Dodge (editor)Paperback
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DescriptionFrom its earliest decisions in the 1790s, the US Supreme Court has used international law to help resolve major legal controversies. This book presents a comprehensive account of the Supreme Court's use of international law from its inception to the present day. Addressing treaties, the direct application of customary international law and the use of international law as an interpretive tool, this book examines all the cases or lines of cases in which international law has played a material role, showing how the Court's treatment of international law both changed and remained consistent over the period. Although there was substantial continuity in the Supreme Court's international law doctrine through the end of the nineteenth century, the past century has been a time of tremendous doctrinal change. Few aspects of the Court's international law doctrine remain the same in the twenty-first century as they were two hundred years ago.
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About AuthorDavid L. Sloss is Professor of Law at Santa Clara University School of Law, where he serves as Director of the Center for Global Law and Policy. He is the editor of The Role of Domestic Courts in Treaty Enforcement: A Comparative Study (2009). He has published numerous articles on the history of US foreign affairs law and the judicial enforcement of treaties in US courts. Michael D. Ramsey is Professor of Law at the University of San Diego School of Law. He is the author of The Constitution's Text in Foreign Affairs (2007) and of numerous articles examining the foreign affairs aspects of the US Constitution in the founding era. William S. Dodge is Professor of Law at the University of California, Hastings College of the Law. He is coauthor (with Detlev Vagts and Harold Koh) of Transnational Business Problems, 4th edition (2008) and has written extensively on the history of international law in American courts and on statutory interpretation in the international context.
ContentsPart I. From the Founding to the Civil War: 1. International law in the Supreme Court, 1789-1860 David L. Sloss, Michael D. Ramsey and William S. Dodge; Part II. From the Civil War to the Turn of the Century: 2. Treaties in the Supreme Court, 1861-1900 Duncan B. Hollis; 3. Customary international law in the Supreme Court, 1861-1900 David J. Bederman; 4. International law as an interpretive tool in the Supreme Court, 1861-1900 Thomas H. Lee and David L. Sloss; 5. A social history of international law: historical commentary, 1861-1900 John Fabian Witt; Part III. From the Turn of the Century to World War II: 6. Treaties in the Supreme Court, 1901-45 Michael P. Van Alstine; 7. Customary international law in the Supreme Court, 1901-45 Michael D. Ramsey; 8. International law as an interpretive tool in the Supreme Court, 1901-45 Roger P. Alford; 9. Varieties and complexities of doctrinal change: historical commentary, 1901-45 Edward A. Purcell, Jr; Part IV. From World War II to the New Millenium: 10. Treaties in the Supreme Court, 1946-2000 Paul B. Stephan; 11. Customary international law in the Supreme Court, 1946-2000 William S. Dodge; 12. International law as an interpretive tool in the Supreme Court, 1946-2000 Melissa A. Waters; 13. Global power in an age of rights: historical commentary, 1946-2000 Martin S. Flaherty; Part V. International Law in the US Supreme Court in the Twenty-First Century: 14. Medellin and Sanchez-Llamas: treaties from John Jay to John Roberts Lori F. Damrosch; 15. Sosa and the derivation of customary international law John O. McGinnis; 16. International law and constitutional interpretation in the twenty-first century: change and continuity Mark Tushnet; 17. Empagran's empire: international law and statutory interpretation in the US Supreme Court of the twenty-first century Ralf Michaels; 18. The Supreme Court, the war on terror, and the American just war constitutional tradition David Golove.
Product Details
- publication date: 13/08/2012
- Format: Paperback
- Number Of Pages: 632
- weight: 1100
Delivery Information
- Saver Delivery: Yes
- 1st Class Delivery: Yes
- Courier Delivery: Yes
- Store Delivery: Yes


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I just booked a client on Budapest-JFK on American for next summer and realized I never wrote about Oneworld's new transatlantic routes (which have a good amount of award availability)
Per their press release
"American, British Airways and Iberia also announced four new routes beginning next Spring as a benefit of the new joint business. They are: New York JFK-Budapest and Chicago-Helsinki (operated by American Airlines), London Heathrow-San Diego (operated by British Airways) and Madrid-Los Angeles (operated by Iberia). American will also add additional frequencies from JFK to Barcelona and Miami to Madrid.
Great news for West Coast flyers (especially San Diegoans) who have limited direct options to Europe. Nothing puts a damper on a trip to Europe than a weather related flight cancellation in JFK or Chicago!
As mentioned, I just booked BUD-JFK tickets for next June and there were multiple days with multiple seats available. Book them while you can!
I see continued emphasis on alliances as a major theme in the future of air travel. Delta/Air France/ KLM are continuing to lead the pack with this and are looking to incorporate SkyTeam partners Alitalia and Korean in the near future. I forsee United/Lufthansa and other Star Alliance carriers doing this as well. Right now elite benefits and upgrade certificates are not seamless between alliances and I imagine that will continue to change (like Delta announcing System Wide Upgrades are now available for use on Air France– a major win for Delta flyers).
What are you thoughts on the future of the alliances?
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38 Strandloper Ave Paternoster Western Cape 7381
St Augustine St Paternoster Western Cape 7381
On The Beach, Langstrand Paternoster Western Cape
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Senate President Bukola Saraki, who led a team of National Assembly leaders to visit President Muhammadu Buhari in London, said at the end of the visit: "there is no cause for alarm"
All Airtel users can now read News 24 Nigeria for free through a Facebook-led Internet.org initiative.
Manchester - Jose Mourinho's mood was a little brighter on
Wednesday after an EFL Cup victory over Manchester City, but there is still
much work to be done in order to get his season back on track.
The Manchester United manager issued a public apology to the
club's supporters after an embarrassing 4-0 defeat at Chelsea last Sunday,
which left his team seventh in the Premier League.
Despite only winning one of their last six league matches,
United are just six points behind leaders City as they go into Saturday's home
match against Burnley.
There is plenty of time to close the gap, and winger Juan
Mata is optimistic that an improvement in form is imminent.
"After a defeat, everyone is going to speak badly about
the team, about the manager. But we, as a group, need to stay strong and
believe we can do great things together," said Mata.
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critics and we showed on Wednesday that if we are focused 100%, we can win
against such a good team."
Also read: Penitent Mourinho humbled by Man Utd support
The concern for Mourinho is that injury problems are
Striker Marcus Rashford limped out of Wednesday's match with
nine minutes left clutching his thigh, and is being assessed by United's
medical team.
That setback came after defender Eric Bailly was ruled out
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Martial, withdrawn from the squad to face City because of a
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It is not the first time that Mourinho has got into trouble
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Jose Mourinho (Getty Images)
Like everyone else, I believe that the most popular definition of democracy is "government of the people, by the people and for the people". Read more...
Like NDDC Unlike MONDA. This notion is an intuition that does not portend political participation, affiliation, intrusion or aggression but a submission with the intention of completion of the previous administration's noble vision. Read more...
The problems of Nigeria is not in its conventional composition, formation, functionality, constitution or treaty, while the solutions are not disintegrations as promulgated by some faiths fanatics and bigotries.
Read more...
It was unbelievable when the social and mainstream media all over the world began airing the breaking news of Donald Trump's victory in the most contentious US Presidential elections in recent years. Read more...
A new novel by a prolific young Nigerian author features gay characters, which could help increase the visibility of the gay community and possibly lead to greater understanding of LGBT Nigerians. Read more...
Your Excellency, Governor Adams Oshiomhole, as a leader that pays attention to details, I understand that the odd title of this piece would definitely arouse your curiosity. Read more...
We have recently returned from a visit to Nigeria's Borno State. Amid the hunger and displacement, we saw that something else was terribly wrong. Read more...
We the student body known as Biafran Students in Diaspora (BSD) wish to take this opportunity to respond formally to the utterances attributed to the Nigerian Foreign Affairs Minister Geoffrey Onyeama, an Igbo. Read more...
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A leader's job is not to dictate, but rather to be respected, admired and be a trustee, of the land we love, with so much potential, a land which should be freer than free. Its still a long way to fufilling our destiny! Read more...
The recession should be seen as an opportunity for the country's promotion as long as we all collectively conduct ourselves in a patriotic manner, writes Isaac Asabor.
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We want to imitate the whites in everything because we are ignorant of our inherent originality and content. We spend all our Naira to acquire his inventions because we so oblivious of our natural endowments that we allow him have it for free. Read more...
ADSU integrity forum has accused the Sunday Joshua Wugira, a lawyer, of adopting unorthodox tactics by abusing his privilege by attacking the integrity of ADSU Vice Chancellor Dr. Moses Zira Zaruwa, writes a News24 reader. Read more...
Poetry by Abdulsalam Jubril. Read more...
Every leader has the opportunity to become great and making himself immortal in the lives and hearts of people for generations to come. Will Mr. President seize this opportunity?, questions Abdulsalam Jubril. Read more...
Members of the black nationhood are very funny people with specialty in compromising everything they touch or learn, writes Olaniyi Odina. Read more...


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Can a vegan person get a good meal at this restaurant?
Can a gluten free person get a good meal at this restaurant?
Is this restaurant good for bar scene?
Is this restaurant appropriate for Kids?
Is this restaurant good for brunch?
Does this restaurant offer free wifi?
Does this restaurant offer takeout or food to go?
Does this restaurant offer delivery?
Does this restaurant accept reservations?
Is this restaurant good for dinner?
Thanks for helping!
Ok food but TERRIBLE everything else! I've tried this location many times, but I always receive very bad service with rude workers and management.
I will start by saying the food was excellent. However, our visit left much to be desired. I called the day prior to set up a reservation because we were going during Charleston Restaurant Week. I was told they did not do reservations, which was fine. When we arrived for dinner, however, we were asked if we had a reservation...
Thank you for taking the time to let me know about your recent visit. I apologize your service and experience was less than satisfactory.
Would you mind giving me a call? I would love to learn more details about your visit (When, time etc) and to see what we can do to correct this.
Director of...
Very Good Food, Full Bar, Amazing Dessert, and Pet Friendly made this place a must to visit! Actually visited 3 times over the course of 3 days. It was chilly, but this Grill had outdoor heaters which made it very nice and inviting!
Wife and I split a pita pizza which was very good. Interesting outdoor eating, good service, and reasonably priced.
Let me start by saying our waiter was very nice, and even apologized for the slow kitchen. He said the kitchen was "really backed up" although both our meals were not quite warm when we got them, so not sure about that. We were there on a Sunday for brunch, so maybe the food was leftover from the day before,...
I was in Charleston with some friends last week and one group member wanted something other than low country for dinner one night so we walked to Tabbuli. We sat outside in a patio area which was very nice. I think the manager assigned our table of 8 women the newest wait person because, though nice enough, she new nothing...
Wonderful food, attentive and kind wait-staff, knowledgeable bartenders, beautiful location, diverse clientele and a beautiful place to enjoy well-prepared food.
I could go on, but I am planning my next visit!
Awesome authentic mediterranean flavor. Great gyros and hummus, Greek Yogurt. Fresh pita and greek salad. Nothing too fancy, but excellent tzatziki sauce and a pleasant atmosphere with variety of menu options for those not so inspired by Greek fare.
The place looks more like a bar than I would prefer but the food was very flavorful and fresh. It's a great location at the end of Market St so it's convenient but not in the middle of everything. We both had the lamb gyros one with fries which were nicely seasoned and one with hummus. Wonderful lunch!
The day...
If you like mediterranean food -- run to this place. We started with the lentil soup which was delicious. We ordered the hummus, babaganoush, and falafel with warm pita bread as our tabouli trio -- then fries going to another table looked so good -- we had to get them too. Everything was delicious. Our waitress was very nice and...
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Kevin Margo
Kevin Margo is a professional in the game industry.
Gameography ( 3 )
Dark Souls II (2014) ()
Lighting and Compositing (Frognation)
Hellgate: London (2007) ()
CG Supervisor (Blur Studio), Modeling (Blur Studio), Lighting and Compositing (Blur Studio)
Halo Wars (2009) ()
Sequence Lead (Blur Studio), Modeling (Blur Studio)
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