A statistical representation of the cosmological constant from finite size effects at the apparent horizon

Abstract In this paper we present a statistical description of the cosmological constant in terms of massless bosons (gravitons). To this purpose, we use our recent results implying a non vanishing temperature %${T_{\Lambda }}%$ for the cosmological constant. In particular, we found that a non vanis...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Viaggiu, Stefano [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2016

Schlagwörter:	Cosmological constant Gravitons Apparent horizon Bose–Einstein condensation

Übergeordnetes Werk:	Enthalten in: General relativity and gravitation - New York, NY [u.a.] : Springer Science + Business Media B.V., 1970, 48(2016), 7 vom: 21. Juni
Übergeordnetes Werk:	volume:48 ; year:2016 ; number:7 ; day:21 ; month:06

Links:	Volltext

DOI / URN:	10.1007/s10714-016-2095-5

Katalog-ID:	SPR012693561

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520			\|a Abstract In this paper we present a statistical description of the cosmological constant in terms of massless bosons (gravitons). To this purpose, we use our recent results implying a non vanishing temperature %${T_{\Lambda }}%$ for the cosmological constant. In particular, we found that a non vanishing %$T_{\Lambda }%$ allows us to depict the cosmological constant %$\Lambda %$ as composed of elementary oscillations of massless bosons of energy %$\hbar \omega %$ by means of the Bose–Einstein distribution. In this context, as happens for photons in a medium, the effective phase velocity %$v_g%$ of these massless excitations is not given by the speed of light c but it is suppressed by a factor depending on the number of quanta present in the universe at the apparent horizon. We found interesting formulas relating the cosmological constant, the number of quanta N and the mean value %$\overline{\lambda }%$ of the wavelength of the gravitons. In this context, we study the possibility to look to the gravitons system so obtained as being very near to be a Bose–Einstein condensate. Finally, an attempt is done to write down the Friedmann flat equations in terms of N and %$\overline{\lambda }%$.
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912			\|a GBV_ILN_62
912			\|a GBV_ILN_63
912			\|a GBV_ILN_69
912			\|a GBV_ILN_70
912			\|a GBV_ILN_73
912			\|a GBV_ILN_74
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912			\|a GBV_ILN_95
912			\|a GBV_ILN_100
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912			\|a GBV_ILN_105
912			\|a GBV_ILN_110
912			\|a GBV_ILN_120
912			\|a GBV_ILN_138
912			\|a GBV_ILN_150
912			\|a GBV_ILN_151
912			\|a GBV_ILN_152
912			\|a GBV_ILN_161
912			\|a GBV_ILN_170
912			\|a GBV_ILN_171
912			\|a GBV_ILN_187
912			\|a GBV_ILN_213
912			\|a GBV_ILN_224
912			\|a GBV_ILN_230
912			\|a GBV_ILN_250
912			\|a GBV_ILN_281
912			\|a GBV_ILN_285
912			\|a GBV_ILN_293
912			\|a GBV_ILN_370
912			\|a GBV_ILN_602
912			\|a GBV_ILN_636
912			\|a GBV_ILN_702
912			\|a GBV_ILN_2001
912			\|a GBV_ILN_2003
912			\|a GBV_ILN_2004
912			\|a GBV_ILN_2005
912			\|a GBV_ILN_2006
912			\|a GBV_ILN_2007
912			\|a GBV_ILN_2008
912			\|a GBV_ILN_2009
912			\|a GBV_ILN_2010
912			\|a GBV_ILN_2011
912			\|a GBV_ILN_2014
912			\|a GBV_ILN_2015
912			\|a GBV_ILN_2020
912			\|a GBV_ILN_2021
912			\|a GBV_ILN_2025
912			\|a GBV_ILN_2026
912			\|a GBV_ILN_2027
912			\|a GBV_ILN_2031
912			\|a GBV_ILN_2034
912			\|a GBV_ILN_2037
912			\|a GBV_ILN_2038
912			\|a GBV_ILN_2039
912			\|a GBV_ILN_2044
912			\|a GBV_ILN_2048
912			\|a GBV_ILN_2049
912			\|a GBV_ILN_2050
912			\|a GBV_ILN_2055
912			\|a GBV_ILN_2057
912			\|a GBV_ILN_2059
912			\|a GBV_ILN_2061
912			\|a GBV_ILN_2064
912			\|a GBV_ILN_2065
912			\|a GBV_ILN_2068
912			\|a GBV_ILN_2070
912			\|a GBV_ILN_2086
912			\|a GBV_ILN_2088
912			\|a GBV_ILN_2093
912			\|a GBV_ILN_2106
912			\|a GBV_ILN_2107
912			\|a GBV_ILN_2108
912			\|a GBV_ILN_2110
912			\|a GBV_ILN_2111
912			\|a GBV_ILN_2112
912			\|a GBV_ILN_2113
912			\|a GBV_ILN_2116
912			\|a GBV_ILN_2118
912			\|a GBV_ILN_2119
912			\|a GBV_ILN_2122
912			\|a GBV_ILN_2129
912			\|a GBV_ILN_2143
912			\|a GBV_ILN_2144
912			\|a GBV_ILN_2147
912			\|a GBV_ILN_2148
912			\|a GBV_ILN_2152
912			\|a GBV_ILN_2153
912			\|a GBV_ILN_2188
912			\|a GBV_ILN_2190
912			\|a GBV_ILN_2232
912			\|a GBV_ILN_2336
912			\|a GBV_ILN_2446
912			\|a GBV_ILN_2470
912			\|a GBV_ILN_2472
912			\|a GBV_ILN_2507
912			\|a GBV_ILN_2522
912			\|a GBV_ILN_2548
912			\|a GBV_ILN_4035
912			\|a GBV_ILN_4037
912			\|a GBV_ILN_4046
912			\|a GBV_ILN_4112
912			\|a GBV_ILN_4125
912			\|a GBV_ILN_4242
912			\|a GBV_ILN_4246
912			\|a GBV_ILN_4249
912			\|a GBV_ILN_4251
912			\|a GBV_ILN_4305
912			\|a GBV_ILN_4306
912			\|a GBV_ILN_4307
912			\|a GBV_ILN_4313
912			\|a GBV_ILN_4322
912			\|a GBV_ILN_4323
912			\|a GBV_ILN_4324
912			\|a GBV_ILN_4325
912			\|a GBV_ILN_4326
912			\|a GBV_ILN_4333
912			\|a GBV_ILN_4334
912			\|a GBV_ILN_4335
912			\|a GBV_ILN_4336
912			\|a GBV_ILN_4338
912			\|a GBV_ILN_4393
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author_variant	s v sv
matchkey_str	article:15729532:2016----::saitclersnainfhcsooiacntnfofntszef
hierarchy_sort_str	2016
bklnumber	33.00
publishDate	2016
allfields	10.1007/s10714-016-2095-5 doi (DE-627)SPR012693561 (SPR)s10714-016-2095-5-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Viaggiu, Stefano verfasserin aut A statistical representation of the cosmological constant from finite size effects at the apparent horizon 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract In this paper we present a statistical description of the cosmological constant in terms of massless bosons (gravitons). To this purpose, we use our recent results implying a non vanishing temperature %${T_{\Lambda }}%$ for the cosmological constant. In particular, we found that a non vanishing %$T_{\Lambda }%$ allows us to depict the cosmological constant %$\Lambda %$ as composed of elementary oscillations of massless bosons of energy %$\hbar \omega %$ by means of the Bose–Einstein distribution. In this context, as happens for photons in a medium, the effective phase velocity %$v_g%$ of these massless excitations is not given by the speed of light c but it is suppressed by a factor depending on the number of quanta present in the universe at the apparent horizon. We found interesting formulas relating the cosmological constant, the number of quanta N and the mean value %$\overline{\lambda }%$ of the wavelength of the gravitons. In this context, we study the possibility to look to the gravitons system so obtained as being very near to be a Bose–Einstein condensate. Finally, an attempt is done to write down the Friedmann flat equations in terms of N and %$\overline{\lambda }%$. Cosmological constant (dpeaa)DE-He213 Gravitons (dpeaa)DE-He213 Apparent horizon (dpeaa)DE-He213 Bose–Einstein condensation (dpeaa)DE-He213 Enthalten in General relativity and gravitation New York, NY [u.a.] : Springer Science + Business Media B.V., 1970 48(2016), 7 vom: 21. Juni (DE-627)320528928 (DE-600)2015524-4 1572-9532 nnns volume:48 year:2016 number:7 day:21 month:06 https://dx.doi.org/10.1007/s10714-016-2095-5 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 48 2016 7 21 06
spelling	10.1007/s10714-016-2095-5 doi (DE-627)SPR012693561 (SPR)s10714-016-2095-5-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Viaggiu, Stefano verfasserin aut A statistical representation of the cosmological constant from finite size effects at the apparent horizon 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract In this paper we present a statistical description of the cosmological constant in terms of massless bosons (gravitons). To this purpose, we use our recent results implying a non vanishing temperature %${T_{\Lambda }}%$ for the cosmological constant. In particular, we found that a non vanishing %$T_{\Lambda }%$ allows us to depict the cosmological constant %$\Lambda %$ as composed of elementary oscillations of massless bosons of energy %$\hbar \omega %$ by means of the Bose–Einstein distribution. In this context, as happens for photons in a medium, the effective phase velocity %$v_g%$ of these massless excitations is not given by the speed of light c but it is suppressed by a factor depending on the number of quanta present in the universe at the apparent horizon. We found interesting formulas relating the cosmological constant, the number of quanta N and the mean value %$\overline{\lambda }%$ of the wavelength of the gravitons. In this context, we study the possibility to look to the gravitons system so obtained as being very near to be a Bose–Einstein condensate. Finally, an attempt is done to write down the Friedmann flat equations in terms of N and %$\overline{\lambda }%$. Cosmological constant (dpeaa)DE-He213 Gravitons (dpeaa)DE-He213 Apparent horizon (dpeaa)DE-He213 Bose–Einstein condensation (dpeaa)DE-He213 Enthalten in General relativity and gravitation New York, NY [u.a.] : Springer Science + Business Media B.V., 1970 48(2016), 7 vom: 21. Juni (DE-627)320528928 (DE-600)2015524-4 1572-9532 nnns volume:48 year:2016 number:7 day:21 month:06 https://dx.doi.org/10.1007/s10714-016-2095-5 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 48 2016 7 21 06
allfields_unstemmed	10.1007/s10714-016-2095-5 doi (DE-627)SPR012693561 (SPR)s10714-016-2095-5-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Viaggiu, Stefano verfasserin aut A statistical representation of the cosmological constant from finite size effects at the apparent horizon 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract In this paper we present a statistical description of the cosmological constant in terms of massless bosons (gravitons). To this purpose, we use our recent results implying a non vanishing temperature %${T_{\Lambda }}%$ for the cosmological constant. In particular, we found that a non vanishing %$T_{\Lambda }%$ allows us to depict the cosmological constant %$\Lambda %$ as composed of elementary oscillations of massless bosons of energy %$\hbar \omega %$ by means of the Bose–Einstein distribution. In this context, as happens for photons in a medium, the effective phase velocity %$v_g%$ of these massless excitations is not given by the speed of light c but it is suppressed by a factor depending on the number of quanta present in the universe at the apparent horizon. We found interesting formulas relating the cosmological constant, the number of quanta N and the mean value %$\overline{\lambda }%$ of the wavelength of the gravitons. In this context, we study the possibility to look to the gravitons system so obtained as being very near to be a Bose–Einstein condensate. Finally, an attempt is done to write down the Friedmann flat equations in terms of N and %$\overline{\lambda }%$. Cosmological constant (dpeaa)DE-He213 Gravitons (dpeaa)DE-He213 Apparent horizon (dpeaa)DE-He213 Bose–Einstein condensation (dpeaa)DE-He213 Enthalten in General relativity and gravitation New York, NY [u.a.] : Springer Science + Business Media B.V., 1970 48(2016), 7 vom: 21. Juni (DE-627)320528928 (DE-600)2015524-4 1572-9532 nnns volume:48 year:2016 number:7 day:21 month:06 https://dx.doi.org/10.1007/s10714-016-2095-5 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 48 2016 7 21 06
allfieldsGer	10.1007/s10714-016-2095-5 doi (DE-627)SPR012693561 (SPR)s10714-016-2095-5-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Viaggiu, Stefano verfasserin aut A statistical representation of the cosmological constant from finite size effects at the apparent horizon 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract In this paper we present a statistical description of the cosmological constant in terms of massless bosons (gravitons). To this purpose, we use our recent results implying a non vanishing temperature %${T_{\Lambda }}%$ for the cosmological constant. In particular, we found that a non vanishing %$T_{\Lambda }%$ allows us to depict the cosmological constant %$\Lambda %$ as composed of elementary oscillations of massless bosons of energy %$\hbar \omega %$ by means of the Bose–Einstein distribution. In this context, as happens for photons in a medium, the effective phase velocity %$v_g%$ of these massless excitations is not given by the speed of light c but it is suppressed by a factor depending on the number of quanta present in the universe at the apparent horizon. We found interesting formulas relating the cosmological constant, the number of quanta N and the mean value %$\overline{\lambda }%$ of the wavelength of the gravitons. In this context, we study the possibility to look to the gravitons system so obtained as being very near to be a Bose–Einstein condensate. Finally, an attempt is done to write down the Friedmann flat equations in terms of N and %$\overline{\lambda }%$. Cosmological constant (dpeaa)DE-He213 Gravitons (dpeaa)DE-He213 Apparent horizon (dpeaa)DE-He213 Bose–Einstein condensation (dpeaa)DE-He213 Enthalten in General relativity and gravitation New York, NY [u.a.] : Springer Science + Business Media B.V., 1970 48(2016), 7 vom: 21. Juni (DE-627)320528928 (DE-600)2015524-4 1572-9532 nnns volume:48 year:2016 number:7 day:21 month:06 https://dx.doi.org/10.1007/s10714-016-2095-5 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 48 2016 7 21 06
allfieldsSound	10.1007/s10714-016-2095-5 doi (DE-627)SPR012693561 (SPR)s10714-016-2095-5-e DE-627 ger DE-627 rakwb eng 530 ASE 33.00 bkl Viaggiu, Stefano verfasserin aut A statistical representation of the cosmological constant from finite size effects at the apparent horizon 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract In this paper we present a statistical description of the cosmological constant in terms of massless bosons (gravitons). To this purpose, we use our recent results implying a non vanishing temperature %${T_{\Lambda }}%$ for the cosmological constant. In particular, we found that a non vanishing %$T_{\Lambda }%$ allows us to depict the cosmological constant %$\Lambda %$ as composed of elementary oscillations of massless bosons of energy %$\hbar \omega %$ by means of the Bose–Einstein distribution. In this context, as happens for photons in a medium, the effective phase velocity %$v_g%$ of these massless excitations is not given by the speed of light c but it is suppressed by a factor depending on the number of quanta present in the universe at the apparent horizon. We found interesting formulas relating the cosmological constant, the number of quanta N and the mean value %$\overline{\lambda }%$ of the wavelength of the gravitons. In this context, we study the possibility to look to the gravitons system so obtained as being very near to be a Bose–Einstein condensate. Finally, an attempt is done to write down the Friedmann flat equations in terms of N and %$\overline{\lambda }%$. Cosmological constant (dpeaa)DE-He213 Gravitons (dpeaa)DE-He213 Apparent horizon (dpeaa)DE-He213 Bose–Einstein condensation (dpeaa)DE-He213 Enthalten in General relativity and gravitation New York, NY [u.a.] : Springer Science + Business Media B.V., 1970 48(2016), 7 vom: 21. Juni (DE-627)320528928 (DE-600)2015524-4 1572-9532 nnns volume:48 year:2016 number:7 day:21 month:06 https://dx.doi.org/10.1007/s10714-016-2095-5 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.00 ASE AR 48 2016 7 21 06
language	English
source	Enthalten in General relativity and gravitation 48(2016), 7 vom: 21. Juni volume:48 year:2016 number:7 day:21 month:06
sourceStr	Enthalten in General relativity and gravitation 48(2016), 7 vom: 21. Juni volume:48 year:2016 number:7 day:21 month:06
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Cosmological constant Gravitons Apparent horizon Bose–Einstein condensation
dewey-raw	530
isfreeaccess_bool	false
container_title	General relativity and gravitation
authorswithroles_txt_mv	Viaggiu, Stefano @@aut@@
publishDateDaySort_date	2016-06-21T00:00:00Z
hierarchy_top_id	320528928
dewey-sort	3530
id	SPR012693561
language_de	englisch
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author	Viaggiu, Stefano
spellingShingle	Viaggiu, Stefano ddc 530 bkl 33.00 misc Cosmological constant misc Gravitons misc Apparent horizon misc Bose–Einstein condensation A statistical representation of the cosmological constant from finite size effects at the apparent horizon
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topic_title	530 ASE 33.00 bkl A statistical representation of the cosmological constant from finite size effects at the apparent horizon Cosmological constant (dpeaa)DE-He213 Gravitons (dpeaa)DE-He213 Apparent horizon (dpeaa)DE-He213 Bose–Einstein condensation (dpeaa)DE-He213
topic	ddc 530 bkl 33.00 misc Cosmological constant misc Gravitons misc Apparent horizon misc Bose–Einstein condensation
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title	A statistical representation of the cosmological constant from finite size effects at the apparent horizon
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title_full	A statistical representation of the cosmological constant from finite size effects at the apparent horizon
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title_sort	statistical representation of the cosmological constant from finite size effects at the apparent horizon
title_auth	A statistical representation of the cosmological constant from finite size effects at the apparent horizon
abstract	Abstract In this paper we present a statistical description of the cosmological constant in terms of massless bosons (gravitons). To this purpose, we use our recent results implying a non vanishing temperature %${T_{\Lambda }}%$ for the cosmological constant. In particular, we found that a non vanishing %$T_{\Lambda }%$ allows us to depict the cosmological constant %$\Lambda %$ as composed of elementary oscillations of massless bosons of energy %$\hbar \omega %$ by means of the Bose–Einstein distribution. In this context, as happens for photons in a medium, the effective phase velocity %$v_g%$ of these massless excitations is not given by the speed of light c but it is suppressed by a factor depending on the number of quanta present in the universe at the apparent horizon. We found interesting formulas relating the cosmological constant, the number of quanta N and the mean value %$\overline{\lambda }%$ of the wavelength of the gravitons. In this context, we study the possibility to look to the gravitons system so obtained as being very near to be a Bose–Einstein condensate. Finally, an attempt is done to write down the Friedmann flat equations in terms of N and %$\overline{\lambda }%$.
abstractGer	Abstract In this paper we present a statistical description of the cosmological constant in terms of massless bosons (gravitons). To this purpose, we use our recent results implying a non vanishing temperature %${T_{\Lambda }}%$ for the cosmological constant. In particular, we found that a non vanishing %$T_{\Lambda }%$ allows us to depict the cosmological constant %$\Lambda %$ as composed of elementary oscillations of massless bosons of energy %$\hbar \omega %$ by means of the Bose–Einstein distribution. In this context, as happens for photons in a medium, the effective phase velocity %$v_g%$ of these massless excitations is not given by the speed of light c but it is suppressed by a factor depending on the number of quanta present in the universe at the apparent horizon. We found interesting formulas relating the cosmological constant, the number of quanta N and the mean value %$\overline{\lambda }%$ of the wavelength of the gravitons. In this context, we study the possibility to look to the gravitons system so obtained as being very near to be a Bose–Einstein condensate. Finally, an attempt is done to write down the Friedmann flat equations in terms of N and %$\overline{\lambda }%$.
abstract_unstemmed	Abstract In this paper we present a statistical description of the cosmological constant in terms of massless bosons (gravitons). To this purpose, we use our recent results implying a non vanishing temperature %${T_{\Lambda }}%$ for the cosmological constant. In particular, we found that a non vanishing %$T_{\Lambda }%$ allows us to depict the cosmological constant %$\Lambda %$ as composed of elementary oscillations of massless bosons of energy %$\hbar \omega %$ by means of the Bose–Einstein distribution. In this context, as happens for photons in a medium, the effective phase velocity %$v_g%$ of these massless excitations is not given by the speed of light c but it is suppressed by a factor depending on the number of quanta present in the universe at the apparent horizon. We found interesting formulas relating the cosmological constant, the number of quanta N and the mean value %$\overline{\lambda }%$ of the wavelength of the gravitons. In this context, we study the possibility to look to the gravitons system so obtained as being very near to be a Bose–Einstein condensate. Finally, an attempt is done to write down the Friedmann flat equations in terms of N and %$\overline{\lambda }%$.
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container_issue	7
title_short	A statistical representation of the cosmological constant from finite size effects at the apparent horizon
url	https://dx.doi.org/10.1007/s10714-016-2095-5
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doi_str	10.1007/s10714-016-2095-5
up_date	2024-07-03T14:40:02.568Z
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A statistical representation of the cosmological constant from finite size effects at the apparent horizon

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