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Graviton Mass, Quintessence and Oscillatory Character of the Universe Evolution

It is shown that using the relativistic field theory of gravity (RTG) and measured value of $\Omega_{\mbox{{\small tot}}}$ one can obtain the upper limit on the graviton mass with 95\%~C.L.: $m\leq 1.6\cdot 10^{-66}$ [g]; within the $(1\sigma)$ range its probable value is $m_{g}= 1.3\cdot 10^{-66}$...

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Detalles Bibliográficos
Autores principales: Gershtein, S S, Logunov, A A, Mestvirishvili, M A, Tkachenko, N P
Lenguaje:eng
rus
Publicado: 2003
Materias:
XX
Acceso en línea:http://cds.cern.ch/record/678970
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author Gershtein, S S
Logunov, A A
Mestvirishvili, M A
Tkachenko, N P
author_facet Gershtein, S S
Logunov, A A
Mestvirishvili, M A
Tkachenko, N P
author_sort Gershtein, S S
collection CERN
description It is shown that using the relativistic field theory of gravity (RTG) and measured value of $\Omega_{\mbox{{\small tot}}}$ one can obtain the upper limit on the graviton mass with 95\%~C.L.: $m\leq 1.6\cdot 10^{-66}$ [g]; within the $(1\sigma)$ range its probable value is $m_{g}= 1.3\cdot 10^{-66}$ [g]. It is pointed out that according to RTG the presence of the quintessence is necessary to explain the Universe accelerated expansion. Experimental data on the Universe age and dark matter density allow one to determine the range of possible values of the $\nu$ parameter in the equation of quintessence state and indicate characteristic time, which corresponds to the beginning and cessation of the accelerated expansion epoch, as well as the time period of the maximal expansion, which corresponds to the half-period of the oscillatory evolution of the Universe.
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institution Organización Europea para la Investigación Nuclear
language eng
rus
publishDate 2003
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spelling cern-6789702019-09-30T06:29:59Zhttp://cds.cern.ch/record/678970engrusGershtein, S SLogunov, A AMestvirishvili, M ATkachenko, N PGraviton Mass, Quintessence and Oscillatory Character of the Universe EvolutionXXIt is shown that using the relativistic field theory of gravity (RTG) and measured value of $\Omega_{\mbox{{\small tot}}}$ one can obtain the upper limit on the graviton mass with 95\%~C.L.: $m\leq 1.6\cdot 10^{-66}$ [g]; within the $(1\sigma)$ range its probable value is $m_{g}= 1.3\cdot 10^{-66}$ [g]. It is pointed out that according to RTG the presence of the quintessence is necessary to explain the Universe accelerated expansion. Experimental data on the Universe age and dark matter density allow one to determine the range of possible values of the $\nu$ parameter in the equation of quintessence state and indicate characteristic time, which corresponds to the beginning and cessation of the accelerated expansion epoch, as well as the time period of the maximal expansion, which corresponds to the half-period of the oscillatory evolution of the Universe.IHEP-2003-13oai:cds.cern.ch:6789702003
spellingShingle XX
Gershtein, S S
Logunov, A A
Mestvirishvili, M A
Tkachenko, N P
Graviton Mass, Quintessence and Oscillatory Character of the Universe Evolution
title Graviton Mass, Quintessence and Oscillatory Character of the Universe Evolution
title_full Graviton Mass, Quintessence and Oscillatory Character of the Universe Evolution
title_fullStr Graviton Mass, Quintessence and Oscillatory Character of the Universe Evolution
title_full_unstemmed Graviton Mass, Quintessence and Oscillatory Character of the Universe Evolution
title_short Graviton Mass, Quintessence and Oscillatory Character of the Universe Evolution
title_sort graviton mass, quintessence and oscillatory character of the universe evolution
topic XX
url http://cds.cern.ch/record/678970
work_keys_str_mv AT gershteinss gravitonmassquintessenceandoscillatorycharacteroftheuniverseevolution
AT logunovaa gravitonmassquintessenceandoscillatorycharacteroftheuniverseevolution
AT mestvirishvilima gravitonmassquintessenceandoscillatorycharacteroftheuniverseevolution
AT tkachenkonp gravitonmassquintessenceandoscillatorycharacteroftheuniverseevolution