Gravitationally induced particle production and its impact on the WIMP abundance

A large set of independent astronomical observations have provided a strong evidence for nonbaryonic dark matter in the Universe. One of the most investigated candidates is an unknown long-lived Weakly Interacting Massive Particle (WIMP) which was in thermal equilibrium with the primeval plasma. Her...

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Main Authors: I. Baranov, J.A.S. Lima
Format: Article
Language:English
Published: Elsevier 2015-12-01
Series:Physics Letters B
Subjects:
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269315008138
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author I. Baranov
J.A.S. Lima
author_facet I. Baranov
J.A.S. Lima
author_sort I. Baranov
collection DOAJ
description A large set of independent astronomical observations have provided a strong evidence for nonbaryonic dark matter in the Universe. One of the most investigated candidates is an unknown long-lived Weakly Interacting Massive Particle (WIMP) which was in thermal equilibrium with the primeval plasma. Here we investigate the WIMP abundance based on the relativistic kinetic treatment for gravitationally induced particle production recently proposed in the literature (Lima and Baranov, 2014) [16]. The new evolution equation is deduced and solved both numerically and through a semi-analytical approach. The predictions of the WIMP observables are discussed and compared with the ones obtained in the standard approach.
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spelling doaj.art-36521e69c4aa49b6b246b019b502c2692022-12-21T20:30:03ZengElsevierPhysics Letters B0370-26931873-24452015-12-01751C33834210.1016/j.physletb.2015.10.054Gravitationally induced particle production and its impact on the WIMP abundanceI. Baranov0J.A.S. Lima1Departamento de Física Geral, Universidade de São Paulo, 05508-090 São Paulo, SP, BrazilDepartamento de Astronomia, Universidade de São Paulo, 05508-900 São Paulo, SP, BrazilA large set of independent astronomical observations have provided a strong evidence for nonbaryonic dark matter in the Universe. One of the most investigated candidates is an unknown long-lived Weakly Interacting Massive Particle (WIMP) which was in thermal equilibrium with the primeval plasma. Here we investigate the WIMP abundance based on the relativistic kinetic treatment for gravitationally induced particle production recently proposed in the literature (Lima and Baranov, 2014) [16]. The new evolution equation is deduced and solved both numerically and through a semi-analytical approach. The predictions of the WIMP observables are discussed and compared with the ones obtained in the standard approach.http://www.sciencedirect.com/science/article/pii/S0370269315008138CosmologyDark energyThermodynamics
spellingShingle I. Baranov
J.A.S. Lima
Gravitationally induced particle production and its impact on the WIMP abundance
Physics Letters B
Cosmology
Dark energy
Thermodynamics
title Gravitationally induced particle production and its impact on the WIMP abundance
title_full Gravitationally induced particle production and its impact on the WIMP abundance
title_fullStr Gravitationally induced particle production and its impact on the WIMP abundance
title_full_unstemmed Gravitationally induced particle production and its impact on the WIMP abundance
title_short Gravitationally induced particle production and its impact on the WIMP abundance
title_sort gravitationally induced particle production and its impact on the wimp abundance
topic Cosmology
Dark energy
Thermodynamics
url http://www.sciencedirect.com/science/article/pii/S0370269315008138
work_keys_str_mv AT ibaranov gravitationallyinducedparticleproductionanditsimpactonthewimpabundance
AT jaslima gravitationallyinducedparticleproductionanditsimpactonthewimpabundance