 postulate of the covariance of all systems of equations relative to transformations with the substitution determinant 1. (Eq. 8) (Eq. 9) Nobody who really grasped it can escape from its charm, because it signifies a real triumph of the general differential calculus as founded by Gauss, Riemann, Christoffel, Ricci, and Levi-Civita" [19]. Einstein with the assistance of his friend the philosopher Schlick elaborated "the point argument coincidence" overcoming his hole argument that he built against the general covariance, i.e when he need the limited covariance presented the hole argument" and when he need the general covariance presented "the point argument coincidence" against "the hole argument", therefore the arguments serve to brilliant minds for create or destroy conceptual anything, according to their circumstances and interests. In addition, in a flash, Einstein acting as the best magician of all time due to its consequences in the physical theory, disappeared materiality of the gravitational field the other great obstacle, since Einstein accepting general covariance had that abandon the law conservation of energy of material process and gravitational field taken together. Thus, he had elect between general covariance and gravitational field having stress-energy definitely to favor of the first. In 1913, in the Entwurf theory, Einstein and Grossmann emphasized, that the gravitational field should have an energymomentum tensor as any physical field and they had adverted that make it "there would S μν≡0 H= 1 4 Σ αβτ  gαβ ∂ g τ ∂ xα ∂ g τ ∂ xβ be untenable consequences" [6]. To Einstein, from that moment it was not more importance. Three years before, as mathematician and geometrician, Grossman "distinguished two types of tensors: (a) Those whose components transformed as tensor under arbitrary coordinate transformations; (b) Those whose components transformed as tensor under some limited set of coordinate transformations. "To be generally covariant, the theory would have had to have a gravitation tensor of first type, but Einstein and Grossman offered a tensor of the second type. It followed that the field equations of the theory held only in a restricted set coordinate systems" [17]. Of course, as physicist, Einstein had chosen a tensor of second type to preserve the conservation law of the energy-momentum of the material process and the gravitational field taken together. "In addition to his causality argument, Einstein offered a second reason for abandoning general covariance. He had shown that as a consequence
postulate of the covariance of all systems of equations relative to transformations with the substitution deciding 1. (Eq. 8) (Eq. 9) Nobody who in truth grasped it can escape from its appeal, because it signify a real triumph of the cosmopolitan differential calculus as founded by Gauss, Riemann, Christoffel, Ricci, and Levi - Civita " [ 19 ]. Einstein with the assistance of his ally the philosopher Schlick elaborated " the point argumentation coincidence " overcoming his trap controversy that he built against the general covariance, i.e when he need the limited covariance presented the fix argument " and when he need the general covariance present " the point argument coincidence " against " the hole controversy ", therefore the arguments serve to brilliant minds for create or demolish conceptual anything, according to their circumstances and interests. In addition, in a flash, Einstein acting as the good magician of all time due to its consequences in the physical theory, disappeared materiality of the gravitational field the other bang-up obstacle, since Einstein accepting general covariance have that vacate the law conservation of energy of material process and gravitational field taken together. Thus, he get elect between general covariance and gravitational field having tension - energy definitely to favor of the first. In 1913, in the Entwurf theory, Einstein and Grossmann emphasized, that the gravitational field should get an energymomentum tensor as any forcible field and they had adverted that make it " there would S μν≡0 H= 1 4 Σ αβτ  gαβ ∂ g τ ∂ xα ∂ g τ ∂ xβ be untenable consequences " [ 6 ]. To Einstein, from that moment it was not more importance. Three years before, as mathematician and geometrician, Grossman " distinguish two types of tensors: (a) Those whose components transformed as tensor under arbitrary coordinate transformation; (b) Those whose components transform as tensor under some limited set of coordinate transformation. " To be generally covariant, the hypothesis would have had to have a gravitation tensor of first character, but Einstein and Grossman offered a tensor of the second type. It followed that the playing field equations of the hypothesis held only in a restricted set coordinate system " [ 17 ]. Of course, as physicist, Einstein had chosen a tensor of second type to keep the conservation jurisprudence of the energy - momentum of the material summons and the gravitational field taken in concert. " In addition to his causality argument, Einstein offered a second reason for abandoning general covariance. He had shown that as a consequence
 podtulate of the covarianct of all systems of equavions rslative go transformations with the duvstitytion determinant 1. (Eq. 8) (Eq. 9) Nobofy who rwallb grasped it can escape nxom ifd chcrn, because it slgnifies a seal triumph ox ghz general differential calculus as fjunded ny Gauss, Riemann, Chrpseoffsl, Ricci, and Levi-Civita" [19]. Einstein sith tht assistance of hix friend the philosopher Sfhlifk elaborated "the ooint argumght siincidence" oxercoming his hole argoment that he built against the eenercl covarianxe, i.e fhen he neev the jimited covavpance psesentec the hole argmment" ane when he need the geieral covariance prefented "tha 'oint argument coincieebce" acainvt "tfw hule acgujent", tjerxfore the adguments seeve to brilliant mimdf for create od destwor conceptual anything, according to theig cidcumstances and interesrs. In addition, in a fpash, Einseein acting as the best magician of all time due do ita couwequevxed in the physical theory, disappeared materialyfy on the gravitatiokal field the othet hrrwt obstacle, sknce Enhsfein accepting genfral codariabce had trat sbandon the law conservatiob of energy jd material process and gravitctionak fiekd taken together. Thus, ke had elect betwfen generzu covariance and grsvhtational field having strqss-energy defnnitely go fsvor os the firsh. In 1913, in the Entwurf thelry, Ennstehn and Grodsmann emphasized, that the gravmvational fielc vholld have cn enevgymomentum tenfor as any phyxical fneld avd they has adverved that makq it "there wogpd S μν≡0 H= 1 4 Σ αβτ  gαβ ∂ g τ ∂ vα ∂ g τ ∂ xβ be untdvable consequemces" [6]. To Viustein, frim that moment it xas vkt more importauee. Three years begord, af lavhemaehcian and gemmetficksn, Grussman "distlngjishrd two types of tensmrs: (z) Those whose comppncnts tranwformed ws tensor undrr arbitrary coordlnate trensforkatyons; (b) Those whose components fransformfd ws tensor unqer wome limited set of coordinate transformations. "To bx generally covariant, jhe theory would have mad to have e gravytation tansor of first type, vut Einstein and Nrossman offered a tenaor of the decond type. It followed that the field equations of the theory held only un a rxsericted set cootdinane fvstems" [17]. Of ronrse, as physicist, Einstein had chosen a tensor oh second tfpz to preserve the conservatiom uaw of the engrgy-momentum of the materizl procexs and the gravitational field yaken together. "In additipn to hiw cauaality argnment, Einstein offerrd a szcond eeason dor wbandoning geversl covarianfe. Ht hab shown that as a consequence
postulate of the covariance of all systems relative transformations with substitution determinant 1. who grasped it can from its charm, it signifies a real triumph of general differential calculus as founded by Gauss, Riemann, Christoffel, Ricci, and Levi-Civita" [19]. with the assistance of his friend the philosopher Schlick elaborated "the point argument overcoming hole that built against the general covariance, i.e when he need the limited covariance presented the hole argument" when he need the general covariance presented "the argument coincidence" against "the argument", therefore the arguments serve brilliant for create destroy anything, to their circumstances interests. In addition, in a flash, Einstein acting as the best magician of all time due to consequences in theory, disappeared of gravitational the other great Einstein accepting general covariance had that conservation of energy of material process and gravitational taken together. he had elect between general covariance gravitational field having stress-energy definitely to favor of first. In 1913, in the Entwurf theory, Einstein and Grossmann emphasized, that the gravitational field an energymomentum tensor as physical field and had that it would S H= 1 4 Σ αβτ  gαβ ∂ g τ ∂ ∂ g τ ∂ xβ be untenable consequences" [6]. To that it was not importance. Three years before, mathematician geometrician, Grossman "distinguished two tensors: Those as under coordinate transformations; (b) Those components transformed as tensor under limited set of coordinate the theory would have had to have a tensor of first type, but Einstein and offered a tensor of the second type. It followed that the field of the only in a restricted set coordinate systems" [17]. course, as physicist, Einstein chosen a tensor of second type to preserve the law the energy-momentum the material process the gravitational field together. "In addition causality argument, offered second general covariance. He had shown that a
 postulate of the covariance oF all systemS of eqUatIonS rElatIve tO transformatioNS witH the substitution determInant 1. (eq. 8) (eQ. 9) NobODy Who reAlly graSPeD IT caN eScApe FrOM iTs chaRm, bEcause iT signifies A reAl Triumph of the GEnEral differEntIal calculus aS foUnded bY GAusS, riemaNn, CHristOffel, RICci, and levi-CivitA" [19]. EINstein WIth the aSSIsTancE of his friend the phILoSOpher Schlick elAboratEd "THe POInt ArgUment coincIdEnce" oVErcominG HiS HOLe aRGument that he bUilt against THe gEneral CoVarIAnce, i.e When hE nEEd tHe limited coVariAnce preseNted thE Hole argUMent" and When he NeeD thE genERaL cOvaRiANce PReSenTEd "tHe point aRgUmEnt coInciDENCE" agaInsT "the Hole aRgument", therefOre The aRGumEnts sErve tO briLlIant mInds foR creaTe Or destroy concepTual Anything, aCcoRdIng To Their CIrcumsTanCes And inteRests. In ADdiTiON, IN a Flash, Einstein actinG aS THe Best magiCian of ALl TiME due to itS cOnsEqueNCEs in tHe phYSiCal theorY, disapPEaReD materiAlIty of tHe GraVitAtionAL fieLd the oTher greaT obstACle, since EinsteIN accepting genERaL COvARianCe hAd that abandOn thE Law cOnseRVaTioN Of eneRgy of MaTErIAl process and gravitaTiOnal fiEld taKen together. ThUs, he had eleCT BEtween geNeraL CoVAriance and gravItatiOnal field hAVing streSs-eneRgy definItely to faVOR of the fiRst. in 1913, iN thE EnTWUrF theory, EinsteIN And GRoSsmann eMphAsized, tHat The GraVitAtIonal fielD should hAvE aN eNeRgyMomenTUm tensor As Any PhYsiCal fiELd and tHey haD advErTeD ThaT make it "THeRE WoulD S Μν≡0 h= 1 4 Σ αβΤ  gαΒ ∂ g Τ ∂ xα ∂ g τ ∂ Xβ be UNteNable coNsequenceS" [6]. To eInstEiN, fRom that Moment it was noT mOre importaNcE. ThRee yeaRS Before, as Mathematician and geometrICian, GroSsmAn "disTingUished two TypEs of teNsoRS: (a) ThosE whose CompoNeNts TRAnsfoRMEd As tEnSor under arBITraRy cooRdInatE transfOrmations; (b) Those whoSE coMponents transForMed aS TEnSor UNdER soMe LImiTED set of coordinatE transformAtIOnS. "To be generALly CoVariant, The theoRy wouLD have haD to have a gRavitatioN tEnsoR OF fiRst type, but einstein And GrossmAN offeREd A tensOr oF the seCoNd tYpe. It FollowED thAt the Field eQuAtions Of the ThEory held Only in a restricted set cooRdinatE systEms" [17]. of course, aS phYSicIst, EinsteIn haD chosen a teNsoR of SeconD tyPE to prEserVE tHe cONservAtioN Law of the eNErGy-mOMEnTum of the matERIAl pRocesS anD The graVitaTional field taken tOGether. "In additiOn to HIS caUsaLIty aRgUment, Einstein oFfeReD A Second reAsOn for abandoNing geneRaL CovarIance. HE had shOwn that AS A cONsequeNce
 postulate of the covarian ce of allsyste msofeq uati onsrelative to tr a nsfo rmations with the subs titut io n  det e rm inant  1. (Eq .  8 ) (Eq .9)  No bo d ywho r eal ly gras ped it can  es ca pe from itsc ha rm, becaus e i t signifiesa r eal tr iu mph of th e g enera l diff e rentia l calculu sa s foun d ed by G a u ss , Ri emann, Christoffe l ,R icci, and Levi -Civit a" [1 9 ] . E ins tein withth e ass i stanceo fh i s  fr i end the philo sopher Schl i ckelabor at ed" the po int a rg u men t coinciden ce"overcomin g hish ole arg u ment th at hebui ltagai n st  t hege n era l  c ova r ian ce, i.ewh en  he n eedt h e limi ted  cov arian ce presentedthe  hol e  ar gumen t" an d wh en  he n eed th e gen er al covariance p rese nted "the  po in t a rg ument coinci den ce"  agains t "theh ole  a r g u me nt", therefore the  a r g um ents ser ve tob ri ll i ant mind sfor  cre a t e ordest r oy  concept ual an y th in g, acco rd ing to  t hei r c ircum s tanc es and  interes ts. I n  addition, ina  flash, Einst e in a ct i ng a s t he best mag icia n  ofallt im e d u e toits c on s eq u ences in the physic al  theor y, di sappeared mat eriality o f t he gravi tati o na l  field the oth er gr eat obstac l e, since  Eins tein acc epting ge n e ral cova ria nce  ha d t h a tabandon the l a w  con se rvation  of  energy  of  ma ter ial  p rocess an d gravit at io na lfie ld ta k en toget he r.Th us,  he h a d elec t bet ween  g en e ral  covari a nc e andgr av itat ion al  fiel d ha v ing  stress -energy d efi n itel yto  favorof the first.  I n 1913, in  t heEntwur f theory,Einstein and Grossmanne mphasiz ed,  that  the  gravitat ion al fie lds houldhave a n ene rg ymo m e ntumt e ns oras  any physi c a l f ieldan d th ey hadadverted that make it"there wouldS μ ν≡0H =  1  4Σ  α β τ   g α β ∂ g  τ ∂ xα ∂ g τ  ∂ xβ be u nt e na ble conseq u enc es " [6].To Eins tein, from th at moment  it was n ot  mor e imp ortance. T hree yea rs before ,  as m a th emati cia n andge ome trici an, Gr o ssm an "d isting ui shed t wo ty pe s of ten sors: (a) Those whose c ompone nts t ran sformed a s t e nso r under a rbit rary coord ina tetrans for m ation s; ( b )Tho s e who se c o mponentst ra nsf o r me d as tensor u n der  some  li m ited s et o f coordinate tran s formations. "T o be g ene ral l y co va riant, the the ory  w o u ld haveha d to have a  gravita ti o n ten sor of  first  type,b u tE instei n an d G rossman o ffe re d  a tens or  o f  the s econ dtype.It fol l owed t hat the field eq uatio n s  of t h e t heory  h eld onl y  ina restrict ed set coor dinate  sys tems"  [17].Of  cours e,as  physicist ,  Einstein  hadchosenatens orof sec ondt y pe to  pre se rve  the cons e r va t io nl awof t he en er gy-m omentum o f  the mat eri a l proce ss  an d the gr a vi t a tional fie ldtaken t ogether. " I n ad d it i on to  his c ausali ty argu m ent ,Einstei n o f f ered a se cond reas o n f or  aba ndoningge nera lcov ar iance. He had s hown tha t as a c o n sequen ce
 postulate_of the_covariance of all systems_of equations_relative_to transformations_with_the substitution determinant_1. (Eq. 8)_(Eq. 9) Nobody who_really grasped it_can_escape from its charm, because it signifies a real triumph of the general differential_calculus_as founded_by_Gauss,_Riemann, Christoffel, Ricci, and Levi-Civita"_[19]. Einstein with the assistance_of his_friend the philosopher Schlick elaborated "the point argument_coincidence"_overcoming his hole_argument that he built against the general covariance, i.e_when he need the limited covariance_presented the hole_argument"_and_when he need the_general covariance presented "the point argument_coincidence" against "the hole argument", therefore_the arguments serve to brilliant minds for_create or destroy conceptual anything, according_to their circumstances and interests._In addition,_in a flash, Einstein acting_as the best_magician of_all time due_to its consequences in the physical_theory, disappeared materiality_of the gravitational field the other_great_obstacle, since Einstein_accepting_general_covariance had_that abandon the_law_conservation of_energy_of material process and gravitational field_taken_together. Thus, he had elect between general_covariance and gravitational field_having_stress-energy definitely to favor_of the first. In 1913,_in the Entwurf theory, Einstein and_Grossmann emphasized,_that the_gravitational field should have an energymomentum tensor as any physical field_and they had adverted that make_it "there would S_μν≡0 H=_1_4 Σ αβτ__gαβ ∂_g τ ∂ xα ∂ g τ_∂ xβ_be untenable consequences" [6]. To Einstein,_from that moment it_was_not more importance. Three years before,_as mathematician and geometrician, Grossman "distinguished_two types of tensors: (a)_Those_whose_components transformed as tensor under_arbitrary coordinate transformations; (b) Those whose_components transformed as_tensor under some limited set of coordinate_transformations._"To be generally covariant, the theory_would_have had to have a gravitation_tensor_of_first type, but Einstein and_Grossman offered a tensor of the_second type. It followed that the field equations of_the theory held_only in a restricted set_coordinate_systems"_[17]. Of course, as physicist, Einstein had chosen a tensor_of second_type to preserve_the conservation law of the energy-momentum of the material process_and the gravitational field taken together. "In_addition to his causality argument, Einstein offered a second reason for_abandoning general covariance. He had shown that as_a consequence