 minute interview. The interview can be conducted over the telephone or in person. Thank you for considering this research study, I really appreciate it. I will email you the informed consent form. > (If there is not interest in participating...) That is fine, I understand. Best wishes for a great school year in "name o f school district." Remarks on Mӧller mistaken famous paper from 1943 Jaykov Foukzon jaykovfoukzon@list.ru Center for Mathematical Sciences, Israel Institute of Technology,Haifa,Israel Abstract Einstein field equations was originally derived by Einstein in 1915 in respect with canonical formalism of Riemann geometry,i.e. by using the classical sufficiently smooth metric tensor, smooth Riemann curvature tensor, smooth Ricci tensor,smooth scalar curvature, etc.. However have soon been found singular solutions of the Einstein field equations with degenerate and singular metric tensor and singular Riemann curvature tensor. These degenerate and singular solutions of the Einstein field equations was formally accepted by main part of scientific community beyond rigorous canonical formalism of Riemannian geometry. 1.The breakdown of canonical formalism of Riemann geometry for the singular solutions of the Einstein field equations Einstein field equations was originally derived by Einstein in 1915 in respect with canonical formalism of Riemann geometry,i.e. by using the classical sufficiently smooth metric tensor, smooth Riemann curvature tensor, smooth Ricci tensor,smooth scalar curvature, etc.. However have soon been found singular solutions of the Einstein field equations with degenerate and singular metric tensor and singular Riemann curvature tensor. These degenerate and singular solutions of the Einstein field equations was formally accepted by main part of scientific community beyond rigorous canonical formalism of Riemannian geometry. 1.1.A. Einstein and N. famous paper from May 8,1935 In famous paper from May 8,1935 [1],(see [1],sec.1,p.74) A.Einstein originally emphasized that degenerate (singular) solutions of the Einstein field equations are problematic: "The first step to the general theory of relativity was to be found in the so-called "Principle of Equivalence": If in a space free from gravitation a reference system is uniformly accelerated, the reference system can be treated as being "at rest, " provided one interprets the condition of the space with respect to it as a homogeneous gravitational field. As is well known the latter is exactly described by the metric field ds2  dx1 2  dx2 2  dx3 2  2x12dx42 1. 1. 1 The g
minute interview. The interview can be conducted over the telephone or in person. Thank you for consider this inquiry study, I really prize it. I will email you the inform consent form. > (If there be not interest in participating ...) That is all right, I sympathize. Best wishes for a big school year in " name o f school district. " remark on Mӧller mistaken famous paper from 1943 Jaykov Foukzon jaykovfoukzon@list.ru Center for Mathematical Sciences, Israel Institute of Technology, Haifa, Israel Abstract Einstein field equations was primitively derived by Einstein in 1915 in respect with canonical formalism of Riemann geometry, i by using the classical sufficiently politic metric tensor, politic Riemann curvature tensor, smooth Ricci tensor, smooth scalar curvature, etc.. However have soon been found singular solutions of the Einstein discipline equations with degenerate and singular metric tensor and singular Riemann curvature tensor. These degenerate and remarkable solutions of the Einstein field equations was formally accepted by main part of scientific community beyond rigorous canonical formalism of Riemannian geometry. 1.The breakdown of canonical formalism of Riemann geometry for the remarkable solutions of the Einstein field equations Einstein sphere equation was originally derived by Einstein in 1915 in respect with canonical formalism of Riemann geometry, i.e. by using the classical sufficiently legato metric tensor, smooth Riemann curvature tensor, smooth Ricci tensor, smooth scalar curvature, etc.. However have soon been found singular solution of the Einstein field equations with degenerate and singular metric tensor and singular Riemann curvature tensor. These degenerate and remarkable solutions of the Einstein field equations was formally accepted by main contribution of scientific community beyond rigorous canonical formalism of Riemannian geometry. 1.1.A. Einstein and N. famous paper from May 8,1935 In famous paper from May 8,1935 [ 1],(see [ 1],sec.1,p.74) A.Einstein originally emphasized that debauched (singular) solutions of the Einstein field equations are problematic: " The inaugural step to the cosmopolitan theory of relativity was to be found in the so - called " rationale of Equivalence ": If in a space free from gravity a reference system is uniformly accelerated, the reference system can be treated as being " at rest, " provided one interprets the condition of the space with respect to it as a homogeneous gravitational battlefield. As is well known the latter is exactly identify by the metric field ds2  dx1 2  dx2 2  dx3 2  2x12dx42 1. 1. 1 The thousand
 mijute interview. The interyiew can be condocred ovxr the felephond or in person. Thank you for cinsidtging this research stjdy, I reaply apprwciaue it. I will email you thc infkvmed eoisent form. > (If jhere is not interest in pdrgieipating...) That is fine, I understand. Bqst wisned for a great fchopj yezg ln "name o f school district." Remadks on Kӧller mistakem famous paper from 1943 Jaykog Fokkzon jaykovfoukzoj@list.ru Cenjsr sir Mathematizal Sciencts, Israel Inatitute of Technology,Haifa,Israeu Abscract Einstgnb flgld equationw was originally derived ty Einsyein in 1915 in rexpert wuth canonical formalivm of Riemann geomgtry,i.e. by gsnng the classical sufdixientny skootf megrid venaor, smloti Riemann chrvature tebsor, smooth Ricci ttnsjg,xmooth scalad curvwttre, etc.. However have soon been found sitgumar solutions of the Eibstein field equationd with dedenerate and singular metric tensor and singular Siemain cuxywgyrf tensor. These degenerate and singular solutijhs on the Einstein fleld equations was flrkwlly accepted by manh lart of scientific communyty bwyond rigjroux canonical formalism of Riwmannian geoiwtry. 1.The breakdown of canoniccl forkalisk of Riemann geometry fur tge singular solutiona of the Einstein fivld aquations Einstein field ezuations xas oxiginallh detived br Einstein in 1915 lt respect with canlnicap xormalism lf Riemann geometry,i.e. by using vie classical xuxfibiently siooth metric tensow, smooth Riemaun curvacure tdnsor, smoonh Ricci vensor,smooth scalar curvadore, etc.. Howevxr have sjon veen found rkngular solutipns of thv Tinstein fueld equations witm deggnsrate and singuoar metric tensor snd siggllac Rieidnn curvatura tevsof. Thesd degentxatc avd songular solutions of the Einstein field eqiabions was formallr accepted by main part of sciejtifir commnnity neyjnd rigorous canonical formaliam of Rielankian geometry. 1.1.A. Elnstgin and N. fcmous paper from May 8,1935 In famous paper frim May 8,1935 [1],(see [1],sec.1,p.74) A.Winstein originally tmphasized thet degqnerate (shngular) solutions of the Einstein fiekd equations are probmematiw: "The first step to the general theory of relativity was to be found in the so-xalled "Principle or Eqiivalvncz": Iy in a fpacx hree from gravitanion a reference system is unifocmly accelarcted, the reference system can bd treated as ceing "at rest, " provided kne intetprets the condition of the spave with respect to it as a homogwneoua gravpjatmonal field. As is wekl knocn the latter is cxactly descriced bn the metrlc fmelb ds2  dx1 2  dx2 2  dx3 2  2x12dx42 1. 1. 1 The g
minute interview. The interview can be conducted telephone in person. you for considering appreciate I will email the informed consent > (If there is not interest participating...) That is fine, I understand. Best wishes for a great school year "name o f school district." Remarks on Mӧller mistaken famous paper from 1943 Foukzon Center Mathematical Israel Institute of Technology,Haifa,Israel Abstract Einstein field equations was originally derived by Einstein in 1915 in with canonical formalism of Riemann geometry,i.e. by using classical sufficiently smooth metric smooth Riemann curvature tensor, smooth tensor,smooth curvature, etc.. have been singular solutions of Einstein field equations with degenerate and singular metric tensor and singular Riemann curvature tensor. These degenerate and solutions of field equations formally by part of scientific rigorous canonical formalism of Riemannian geometry. canonical formalism of Riemann geometry for the singular of the field equations Einstein field equations was derived by Einstein in 1915 in respect with formalism of Riemann geometry,i.e. by using the classical sufficiently smooth metric tensor, smooth Riemann curvature Ricci tensor,smooth scalar curvature, However have soon found solutions the field equations degenerate and singular metric tensor and singular Riemann curvature tensor. These and singular solutions of the Einstein field equations was formally main of scientific community rigorous canonical formalism of geometry. Einstein and N. famous May In May [1],(see A.Einstein originally emphasized that (singular) solutions of the Einstein equations are problematic: "The theory of relativity was to be found in so-called "Principle of Equivalence": If in a free from gravitation a reference system is uniformly accelerated, the reference system be treated "at rest, " provided one interprets the condition the space with respect it as a homogeneous gravitational field. As is well the is exactly by the metric ds2  dx1  dx2 2 2  1. 1
 minute interview. The interviEw can be conDucteD ovEr tHe TelePhonE or in person. ThaNK you For considering this reseArch sTuDY, I reALlY apprEciate iT. i wILL emAiL yOu tHe INfOrmed ConSent forM. > (If there is Not InTerest in partICiPating...) That Is fIne, I understaNd. BEst wisHeS foR A greaT scHool yEar in "nAMe o f scHool distrIcT." remarkS On MӧlleR MIsTakeN famous paper from 1943 JAYkOV Foukzon jaykovFoukzoN@lISt.RU cenTer For MathemaTiCal ScIEnces, IsRAeL iNStiTUte of TechnoloGy,Haifa,IsraEL AbStract eiNstEIn fielD equaTiONs wAs originallY derIved by EinStein iN 1915 In respeCT with caNonicaL foRmaLism OF RIeManN gEOmeTRy,I.e. bY UsiNg the claSsIcAl sufFiciENTLY smoOth MetrIc tenSor, smooth RiemAnn CurvATurE tensOr, smoOth RIcCi tenSor,smoOth scAlAr curvature, etc.. HOwevEr have sooN beEn FouNd SinguLAr soluTioNs oF the EinStein fiELd eQuATIOnS with degenerate and SiNGUlAr metric Tensor ANd SiNGular RieMaNn cUrvaTURe tenSor. THEsE degenerAte and SInGuLar soluTiOns of tHe einSteIn fieLD equAtions Was formaLly acCEpted by main parT Of scientific cOMmUNItY BeyoNd rIgorous canoNicaL FormAlisM Of rieMAnniaN geomEtRY. 1.THE breakdown of canonicAl FormalIsm of riemann geometRy for the siNGULar solutIons OF tHE Einstein field EquatIons EinsteIN field eqUatioNs was oriGinally deRIVed by EinSteIn iN 1915 in ResPECt With canonical FORmalIsM of RiemAnn GeometrY,i.e. By uSinG thE cLassical sUfficienTlY sMoOtH meTric tENsor, smooTh rieMaNn cUrvatURe tensOr, smoOth RIcCi TEnsOr,smootH ScALAr cuRvAtUre, eTc.. HOwEver hAve sOOn bEen founD singular SolUTionS oF tHe EinstEin field equatIoNs with degeNeRatE and siNGUlar metrIc tensor and singular RiemANn curvaTurE tensOr. ThEse degeneRatE and siNguLAr soluTions oF the EInSteIN Field EQUaTioNs Was formallY ACcePted bY mAin pArt of scIentific community bEYonD rigorous canoNicAl foRMAlIsm OF RIEmaNnIAn gEOMetry. 1.1.A. Einstein aNd N. famous pApER fRom May 8,1935 In faMOus PaPer from may 8,1935 [1],(see [1],sEc.1,p.74) A.EINstein oRiginally EmphasizeD tHat dEGEneRate (singulAr) solutiOns of the EINsteiN FiEld eqUatIons arE pRobLematIc: "The fIRst Step tO the geNeRal theOry of ReLativity Was to be found in the so-callEd "PrinCiple Of EQuivalencE": If IN a sPace free fRom gRavitation A reFerEnce sYstEM is unIforMLy AccELeratEd, thE Reference SYsTem CAN bE treated as bEING "at Rest, " pRovIDed one InteRprets the conditioN Of the space with RespECT to It aS A homOgEneous gravitatIonAl FIEld. As is wElL known the laTter is exAcTLy desCribed By the mEtric fiELD dS2  Dx1 2  dx2 2  dx3 2  2X12dx42 1. 1. 1 THe g
 minute interview. The int erview can  be c ond uct ed  ove r th e telephone or in p erson. Thank you for c onsid er i ng t h is  rese arch st u dy , I r ea ll y a pp r ec iateit.  I will  email you  th einformed con s en t form. >(If  there is no t i nteres tinp artic ipa ting. ..) Th a t is f ine, I un de r stand. Best wi s h es  for  a great school y e ar in "name o f s chooldi s tr i c t."  Re marks on M ӧl ler m i stakenf am o u s  pa p er from 1943Jaykov Fouk z onjaykov fo ukz o n@list .ru C en t erfor Mathema tica l Science s, Isr a el Inst i tute of  Techn olo gy, Haif a ,I sr ael  A b str a ct  Ei n ste in field  e qu ation s wa s o r igin all y de rived  by Einsteinin1915 inrespe ct wi th c an onica l form alism  o f Riemann geome try, i.e. by u sin gthe  c lassi c al suf fic ien tly smo oth met r icte n s o r,  smooth Riemann cu rv a t ur e tensor , smoo t hRi c ci tenso r, smo oths c alarcurv a tu re, etc. . Howe v er  h ave soo nbeen f ou ndsin gular solu tionsof the E inste i n field equati o ns with degen e ra t e  a n d si ngu lar metrictens o r an d si n gu lar Riema nn cu rv a tu r e tensor. These deg en erateand s ingular solut ions of th e E insteinfiel d  e q uations was fo rmall y accepted by mainpartof scien tific com m u nity bey ond  ri gor ous c an onical formal i s m of  R iemanni angeometr y.1.T hebre ak down of c anonical  f or ma li smof Ri e mann geo me try  f orthe s i ngular  solu tion sof the  Einste i nf i eldeq ua tion s E in stein  fie l d e quation s was ori gin a llyde ri ved byEinstein in 1 91 5 in respe ct  wi th can o n ical for malism of Riemann geome t ry,i.e.  by  usin g th e classic alsuffic ien t ly smo oth me tricte nso r ,  smoo t h  R iem an n curvatur e ten sor,sm ooth  Riccitensor,smooth scal a r c urvature, etc ..Howe v e rhav e  s o onbe e n f o u nd singular sol utions ofth e  E instein fi e ldeq uations  with d egene r ate and  singular  metric t en sora n d s ingular Ri emann cu rvature t e nsor. Th ese d ege nerate  a ndsingu lar so l uti ons o f theEi nstein  fiel dequation s was formally accepted  by ma in pa rtof scient ifi c  co mmunity b eyon d rigorous  ca non icalfor m alism  ofR ie man n ian g eome t ry. 1.1.A .  E ins t e in  and N. fam o u s  pa per f rom May 8, 1935  In famous paperf rom May 8,1935  [1] , ( see  [1 ] ,sec .1 ,p.74) A.Einst ein  o r i ginallyem phasized th at degen er a te (s ingula r) sol utionso f  t h e Eins tein  fi eld equat ion sa re prob le ma t ic: "T he f ir st ste p to t h e ge n e ral theory of re lativ i t y was tobe fo un d in th e  so- called "Pr inciple ofEquiva lenc e": I f in asp ace fr eefr om gravita t ion a ref erenc e syste mis u nif ormlyacce l e rated , th eref erence sy s t em ca nb e t reat ed as  b eing  "at rest ,  " provi ded one int er pre t s  the c o nd i t ion of the  sp ace w i t h respectt o it as a hom ogeneo us gra vitatio n alfi eld. As  is w ell known  the latt e r i sexac tly desc ri bedby  th emetric field ds 2  dx1  2  dx2 2   dx3  2  2x 1 2dx421 . 1. 1 Theg
 minute_interview. The_interview can be conducted_over the_telephone_or in_person._Thank you for_considering this research_study, I really appreciate_it. I will_email_you the informed consent form. > (If there is not interest in participating...) That_is_fine, I_understand._Best_wishes for a great school_year in "name o f_school district."_Remarks on Mӧller mistaken famous paper from 1943_Jaykov_Foukzon jaykovfoukzon@list.ru Center_for Mathematical Sciences, Israel Institute of Technology,Haifa,Israel Abstract Einstein_field equations was originally derived by_Einstein in 1915_in_respect_with canonical formalism of_Riemann geometry,i.e. by using the classical_sufficiently smooth metric tensor, smooth Riemann_curvature tensor, smooth Ricci tensor,smooth scalar curvature,_etc.. However have soon been found_singular solutions of the Einstein_field equations_with degenerate and singular metric_tensor and singular_Riemann curvature_tensor. These degenerate_and singular solutions of the Einstein_field equations was_formally accepted by main part of_scientific_community beyond rigorous_canonical_formalism_of Riemannian_geometry. 1.The breakdown_of_canonical formalism_of_Riemann geometry for the singular solutions_of_the Einstein field equations Einstein field equations_was originally derived by_Einstein_in 1915 in respect_with canonical formalism of Riemann_geometry,i.e. by using the classical sufficiently_smooth metric_tensor, smooth_Riemann curvature tensor, smooth Ricci tensor,smooth scalar curvature, etc.. However have_soon been found singular solutions of_the Einstein field equations_with degenerate_and_singular metric tensor_and_singular Riemann_curvature tensor. These degenerate and singular solutions_of the_Einstein field equations was formally accepted_by main part of_scientific_community beyond rigorous canonical formalism of_Riemannian geometry. 1.1.A. Einstein and N._famous paper from May 8,1935_In_famous_paper from May 8,1935 [1],(see_[1],sec.1,p.74) A.Einstein originally emphasized that degenerate_(singular) solutions of_the Einstein field equations are problematic: "The_first_step to the general theory of_relativity_was to be found in the_so-called_"Principle_of Equivalence": If in a_space free from gravitation a reference_system is uniformly accelerated, the reference system can be_treated as being_"at rest, " provided one_interprets_the_condition of the space with respect to it as a_homogeneous gravitational_field. As is_well known the latter is exactly described by the metric_field ds2  dx1 2  dx2_2  dx3 2  2x12dx42 1. 1. 1 The g