Quintessence dissipative superattractor cosmology
We investigate the simplest quintessence dissipative dark matter attractor cosmology characterized by a constant quintessence baryotropic index and a power-law expansion. We show a class of accelerated coincidence-solving attractor solutions converging to this asymptotic behavior. Despite its simpli...
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todo:paper_05562821_v63_n10_p_Chimento2023-10-03T15:35:41Z Quintessence dissipative superattractor cosmology Chimento, L.P. Jakubi, A.S. Zuccalâ, N.A. article cosmos entropy luminance mathematical analysis molecular model We investigate the simplest quintessence dissipative dark matter attractor cosmology characterized by a constant quintessence baryotropic index and a power-law expansion. We show a class of accelerated coincidence-solving attractor solutions converging to this asymptotic behavior. Despite its simplicity, such a "superattractor" regime provides a model of the recent universe that also exhibits an excellent fit to supernovae luminosity observations and no age conflict. Our best fit gives a= 1.71 ±0.29 for the power-law exponent. We calculate for this regime the evolution of density and entropy perturbations. ©2001 The American Physical Society. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_05562821_v63_n10_p_Chimento |
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Universidad de Buenos Aires |
institution_str |
I-28 |
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R-134 |
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
topic |
article cosmos entropy luminance mathematical analysis molecular model |
spellingShingle |
article cosmos entropy luminance mathematical analysis molecular model Chimento, L.P. Jakubi, A.S. Zuccalâ, N.A. Quintessence dissipative superattractor cosmology |
topic_facet |
article cosmos entropy luminance mathematical analysis molecular model |
description |
We investigate the simplest quintessence dissipative dark matter attractor cosmology characterized by a constant quintessence baryotropic index and a power-law expansion. We show a class of accelerated coincidence-solving attractor solutions converging to this asymptotic behavior. Despite its simplicity, such a "superattractor" regime provides a model of the recent universe that also exhibits an excellent fit to supernovae luminosity observations and no age conflict. Our best fit gives a= 1.71 ±0.29 for the power-law exponent. We calculate for this regime the evolution of density and entropy perturbations. ©2001 The American Physical Society. |
format |
JOUR |
author |
Chimento, L.P. Jakubi, A.S. Zuccalâ, N.A. |
author_facet |
Chimento, L.P. Jakubi, A.S. Zuccalâ, N.A. |
author_sort |
Chimento, L.P. |
title |
Quintessence dissipative superattractor cosmology |
title_short |
Quintessence dissipative superattractor cosmology |
title_full |
Quintessence dissipative superattractor cosmology |
title_fullStr |
Quintessence dissipative superattractor cosmology |
title_full_unstemmed |
Quintessence dissipative superattractor cosmology |
title_sort |
quintessence dissipative superattractor cosmology |
url |
http://hdl.handle.net/20.500.12110/paper_05562821_v63_n10_p_Chimento |
work_keys_str_mv |
AT chimentolp quintessencedissipativesuperattractorcosmology AT jakubias quintessencedissipativesuperattractorcosmology AT zuccalana quintessencedissipativesuperattractorcosmology |
_version_ |
1782028719983951872 |