Phantom accretion by black holes and the generalized second law of thermodynamics


Autoria(s): LIMA, J. A. S.; PEREIRA, S. H.; HORVATH, J. E.; GUARIENTO, Daniel C.
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

20/10/2012

20/10/2012

2010

Resumo

The accretion of a phantom fluid with non-zero chemical potential by black holes is discussed with basis on the generalized second law of thermodynamics. For phantom fluids with positive temperature and negative chemical potential we demonstrate that the accretion process is possible, and that the condition guaranteeing the positiveness of the phantom fluid entropy coincides with the one required by the generalized second law. (C) 2010 Elsevier B.V. All rights reserved.

Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)

CNPq[150920/2007-5]

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

FAPESP[04/13668-0]

Identificador

ASTROPARTICLE PHYSICS, v.33, n.5/Jun, p.292-295, 2010

0927-6505

http://producao.usp.br/handle/BDPI/29562

10.1016/j.astropartphys.2010.02.008

http://dx.doi.org/10.1016/j.astropartphys.2010.02.008

Idioma(s)

eng

Publicador

ELSEVIER SCIENCE BV

Relação

Astroparticle Physics

Direitos

restrictedAccess

Copyright ELSEVIER SCIENCE BV

Palavras-Chave #Phantom energy #Black holes #Black hole thermodynamics #PROBE WMAP OBSERVATIONS #EQUATION-OF-STATE #DARK ENERGY #COSMOLOGICAL CONSTANT #HIGH-REDSHIFT #OLD GALAXIES #ACCELERATING UNIVERSE #GAMMA-FLUIDS #ANGULAR SIZE #QUINTESSENCE #Astronomy & Astrophysics #Physics, Particles & Fields
Tipo

article

original article

publishedVersion