Graceful exit from inflation to radiation era with rapidly decreasing agegraphic potentials

Abstract. We present a class of models where both the primordial inflation and the late-time de Sitter phase are driven by simple phenomenological agegraphic potentials. In this context, a possible new scenario for a smooth exit from inflation to the radiation era is discussed by resorting the kinat...
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Gespeichert in:

Autor*in:	Viaggiu, Stefano [verfasserIn] Montuori, Marco

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2014

Schlagwörter:	Dark Energy Cosmological Constant Cosmic Time Agegraphic Dark Energy Planck Data

Anmerkung:	© Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014

Übergeordnetes Werk:	Enthalten in: The European physical journal - Berlin : Springer, 2011, 129(2014), 10 vom: 21. Okt.
Übergeordnetes Werk:	volume:129 ; year:2014 ; number:10 ; day:21 ; month:10

Links:	Volltext

DOI / URN:	10.1140/epjp/i2014-14224-x

Katalog-ID:	SPR031453155

Internformat


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520			\|a Abstract. We present a class of models where both the primordial inflation and the late-time de Sitter phase are driven by simple phenomenological agegraphic potentials. In this context, a possible new scenario for a smooth exit from inflation to the radiation era is discussed by resorting the kination (stiff) era but without the inefficient radiation production mechanism of these models. This is done by considering rapidly decreasing expressions for V(t) soon after inflation. We show that the parameters of our models can reproduce the scalar spectral parameter $ n_{s} $ predicted by Planck data in particular for models with concave potentials. Finally, according to the recent BICEP2 data, all our models allow a huge amount of primordial gravitational waves.
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publishDate	2014
allfields	10.1140/epjp/i2014-14224-x doi (DE-627)SPR031453155 (SPR)i2014-14224-x-e DE-627 ger DE-627 rakwb eng Viaggiu, Stefano verfasserin aut Graceful exit from inflation to radiation era with rapidly decreasing agegraphic potentials 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014 Abstract. We present a class of models where both the primordial inflation and the late-time de Sitter phase are driven by simple phenomenological agegraphic potentials. In this context, a possible new scenario for a smooth exit from inflation to the radiation era is discussed by resorting the kination (stiff) era but without the inefficient radiation production mechanism of these models. This is done by considering rapidly decreasing expressions for V(t) soon after inflation. We show that the parameters of our models can reproduce the scalar spectral parameter $ n_{s} $ predicted by Planck data in particular for models with concave potentials. Finally, according to the recent BICEP2 data, all our models allow a huge amount of primordial gravitational waves. Dark Energy (dpeaa)DE-He213 Cosmological Constant (dpeaa)DE-He213 Cosmic Time (dpeaa)DE-He213 Agegraphic Dark Energy (dpeaa)DE-He213 Planck Data (dpeaa)DE-He213 Montuori, Marco aut Enthalten in The European physical journal Berlin : Springer, 2011 129(2014), 10 vom: 21. Okt. (DE-627)647653958 (DE-600)2595693-0 2190-5444 nnns volume:129 year:2014 number:10 day:21 month:10 https://dx.doi.org/10.1140/epjp/i2014-14224-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER 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_65 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_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 AR 129 2014 10 21 10
spelling	10.1140/epjp/i2014-14224-x doi (DE-627)SPR031453155 (SPR)i2014-14224-x-e DE-627 ger DE-627 rakwb eng Viaggiu, Stefano verfasserin aut Graceful exit from inflation to radiation era with rapidly decreasing agegraphic potentials 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014 Abstract. We present a class of models where both the primordial inflation and the late-time de Sitter phase are driven by simple phenomenological agegraphic potentials. In this context, a possible new scenario for a smooth exit from inflation to the radiation era is discussed by resorting the kination (stiff) era but without the inefficient radiation production mechanism of these models. This is done by considering rapidly decreasing expressions for V(t) soon after inflation. We show that the parameters of our models can reproduce the scalar spectral parameter $ n_{s} $ predicted by Planck data in particular for models with concave potentials. Finally, according to the recent BICEP2 data, all our models allow a huge amount of primordial gravitational waves. Dark Energy (dpeaa)DE-He213 Cosmological Constant (dpeaa)DE-He213 Cosmic Time (dpeaa)DE-He213 Agegraphic Dark Energy (dpeaa)DE-He213 Planck Data (dpeaa)DE-He213 Montuori, Marco aut Enthalten in The European physical journal Berlin : Springer, 2011 129(2014), 10 vom: 21. Okt. (DE-627)647653958 (DE-600)2595693-0 2190-5444 nnns volume:129 year:2014 number:10 day:21 month:10 https://dx.doi.org/10.1140/epjp/i2014-14224-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER 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_65 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_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 AR 129 2014 10 21 10
allfields_unstemmed	10.1140/epjp/i2014-14224-x doi (DE-627)SPR031453155 (SPR)i2014-14224-x-e DE-627 ger DE-627 rakwb eng Viaggiu, Stefano verfasserin aut Graceful exit from inflation to radiation era with rapidly decreasing agegraphic potentials 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014 Abstract. We present a class of models where both the primordial inflation and the late-time de Sitter phase are driven by simple phenomenological agegraphic potentials. In this context, a possible new scenario for a smooth exit from inflation to the radiation era is discussed by resorting the kination (stiff) era but without the inefficient radiation production mechanism of these models. This is done by considering rapidly decreasing expressions for V(t) soon after inflation. We show that the parameters of our models can reproduce the scalar spectral parameter $ n_{s} $ predicted by Planck data in particular for models with concave potentials. Finally, according to the recent BICEP2 data, all our models allow a huge amount of primordial gravitational waves. Dark Energy (dpeaa)DE-He213 Cosmological Constant (dpeaa)DE-He213 Cosmic Time (dpeaa)DE-He213 Agegraphic Dark Energy (dpeaa)DE-He213 Planck Data (dpeaa)DE-He213 Montuori, Marco aut Enthalten in The European physical journal Berlin : Springer, 2011 129(2014), 10 vom: 21. Okt. (DE-627)647653958 (DE-600)2595693-0 2190-5444 nnns volume:129 year:2014 number:10 day:21 month:10 https://dx.doi.org/10.1140/epjp/i2014-14224-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER 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_65 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_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 AR 129 2014 10 21 10
allfieldsGer	10.1140/epjp/i2014-14224-x doi (DE-627)SPR031453155 (SPR)i2014-14224-x-e DE-627 ger DE-627 rakwb eng Viaggiu, Stefano verfasserin aut Graceful exit from inflation to radiation era with rapidly decreasing agegraphic potentials 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014 Abstract. We present a class of models where both the primordial inflation and the late-time de Sitter phase are driven by simple phenomenological agegraphic potentials. In this context, a possible new scenario for a smooth exit from inflation to the radiation era is discussed by resorting the kination (stiff) era but without the inefficient radiation production mechanism of these models. This is done by considering rapidly decreasing expressions for V(t) soon after inflation. We show that the parameters of our models can reproduce the scalar spectral parameter $ n_{s} $ predicted by Planck data in particular for models with concave potentials. Finally, according to the recent BICEP2 data, all our models allow a huge amount of primordial gravitational waves. Dark Energy (dpeaa)DE-He213 Cosmological Constant (dpeaa)DE-He213 Cosmic Time (dpeaa)DE-He213 Agegraphic Dark Energy (dpeaa)DE-He213 Planck Data (dpeaa)DE-He213 Montuori, Marco aut Enthalten in The European physical journal Berlin : Springer, 2011 129(2014), 10 vom: 21. Okt. (DE-627)647653958 (DE-600)2595693-0 2190-5444 nnns volume:129 year:2014 number:10 day:21 month:10 https://dx.doi.org/10.1140/epjp/i2014-14224-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER 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_65 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_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 AR 129 2014 10 21 10
allfieldsSound	10.1140/epjp/i2014-14224-x doi (DE-627)SPR031453155 (SPR)i2014-14224-x-e DE-627 ger DE-627 rakwb eng Viaggiu, Stefano verfasserin aut Graceful exit from inflation to radiation era with rapidly decreasing agegraphic potentials 2014 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014 Abstract. We present a class of models where both the primordial inflation and the late-time de Sitter phase are driven by simple phenomenological agegraphic potentials. In this context, a possible new scenario for a smooth exit from inflation to the radiation era is discussed by resorting the kination (stiff) era but without the inefficient radiation production mechanism of these models. This is done by considering rapidly decreasing expressions for V(t) soon after inflation. We show that the parameters of our models can reproduce the scalar spectral parameter $ n_{s} $ predicted by Planck data in particular for models with concave potentials. Finally, according to the recent BICEP2 data, all our models allow a huge amount of primordial gravitational waves. Dark Energy (dpeaa)DE-He213 Cosmological Constant (dpeaa)DE-He213 Cosmic Time (dpeaa)DE-He213 Agegraphic Dark Energy (dpeaa)DE-He213 Planck Data (dpeaa)DE-He213 Montuori, Marco aut Enthalten in The European physical journal Berlin : Springer, 2011 129(2014), 10 vom: 21. Okt. (DE-627)647653958 (DE-600)2595693-0 2190-5444 nnns volume:129 year:2014 number:10 day:21 month:10 https://dx.doi.org/10.1140/epjp/i2014-14224-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER 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_65 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_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 AR 129 2014 10 21 10
language	English
source	Enthalten in The European physical journal 129(2014), 10 vom: 21. Okt. volume:129 year:2014 number:10 day:21 month:10
sourceStr	Enthalten in The European physical journal 129(2014), 10 vom: 21. Okt. volume:129 year:2014 number:10 day:21 month:10
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Dark Energy Cosmological Constant Cosmic Time Agegraphic Dark Energy Planck Data
isfreeaccess_bool	false
container_title	The European physical journal
authorswithroles_txt_mv	Viaggiu, Stefano @@aut@@ Montuori, Marco @@aut@@
publishDateDaySort_date	2014-10-21T00:00:00Z
hierarchy_top_id	647653958
id	SPR031453155
language_de	englisch
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author	Viaggiu, Stefano
spellingShingle	Viaggiu, Stefano misc Dark Energy misc Cosmological Constant misc Cosmic Time misc Agegraphic Dark Energy misc Planck Data Graceful exit from inflation to radiation era with rapidly decreasing agegraphic potentials
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topic_title	Graceful exit from inflation to radiation era with rapidly decreasing agegraphic potentials Dark Energy (dpeaa)DE-He213 Cosmological Constant (dpeaa)DE-He213 Cosmic Time (dpeaa)DE-He213 Agegraphic Dark Energy (dpeaa)DE-He213 Planck Data (dpeaa)DE-He213
topic	misc Dark Energy misc Cosmological Constant misc Cosmic Time misc Agegraphic Dark Energy misc Planck Data
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title	Graceful exit from inflation to radiation era with rapidly decreasing agegraphic potentials
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title_full	Graceful exit from inflation to radiation era with rapidly decreasing agegraphic potentials
author_sort	Viaggiu, Stefano
journal	The European physical journal
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author_browse	Viaggiu, Stefano Montuori, Marco
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author-letter	Viaggiu, Stefano
doi_str_mv	10.1140/epjp/i2014-14224-x
title_sort	graceful exit from inflation to radiation era with rapidly decreasing agegraphic potentials
title_auth	Graceful exit from inflation to radiation era with rapidly decreasing agegraphic potentials
abstract	Abstract. We present a class of models where both the primordial inflation and the late-time de Sitter phase are driven by simple phenomenological agegraphic potentials. In this context, a possible new scenario for a smooth exit from inflation to the radiation era is discussed by resorting the kination (stiff) era but without the inefficient radiation production mechanism of these models. This is done by considering rapidly decreasing expressions for V(t) soon after inflation. We show that the parameters of our models can reproduce the scalar spectral parameter $ n_{s} $ predicted by Planck data in particular for models with concave potentials. Finally, according to the recent BICEP2 data, all our models allow a huge amount of primordial gravitational waves. © Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014
abstractGer	Abstract. We present a class of models where both the primordial inflation and the late-time de Sitter phase are driven by simple phenomenological agegraphic potentials. In this context, a possible new scenario for a smooth exit from inflation to the radiation era is discussed by resorting the kination (stiff) era but without the inefficient radiation production mechanism of these models. This is done by considering rapidly decreasing expressions for V(t) soon after inflation. We show that the parameters of our models can reproduce the scalar spectral parameter $ n_{s} $ predicted by Planck data in particular for models with concave potentials. Finally, according to the recent BICEP2 data, all our models allow a huge amount of primordial gravitational waves. © Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014
abstract_unstemmed	Abstract. We present a class of models where both the primordial inflation and the late-time de Sitter phase are driven by simple phenomenological agegraphic potentials. In this context, a possible new scenario for a smooth exit from inflation to the radiation era is discussed by resorting the kination (stiff) era but without the inefficient radiation production mechanism of these models. This is done by considering rapidly decreasing expressions for V(t) soon after inflation. We show that the parameters of our models can reproduce the scalar spectral parameter $ n_{s} $ predicted by Planck data in particular for models with concave potentials. Finally, according to the recent BICEP2 data, all our models allow a huge amount of primordial gravitational waves. © Società Italiana di Fisica and Springer-Verlag Berlin Heidelberg 2014
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title_short	Graceful exit from inflation to radiation era with rapidly decreasing agegraphic potentials
url	https://dx.doi.org/10.1140/epjp/i2014-14224-x
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author2	Montuori, Marco
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up_date	2024-07-03T23:47:44.238Z
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We present a class of models where both the primordial inflation and the late-time de Sitter phase are driven by simple phenomenological agegraphic potentials. In this context, a possible new scenario for a smooth exit from inflation to the radiation era is discussed by resorting the kination (stiff) era but without the inefficient radiation production mechanism of these models. This is done by considering rapidly decreasing expressions for V(t) soon after inflation. We show that the parameters of our models can reproduce the scalar spectral parameter $ n_{s} $ predicted by Planck data in particular for models with concave potentials. 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Graceful exit from inflation to radiation era with rapidly decreasing agegraphic potentials

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