Entropy, complexity and disequilibrium in compact stars


Autoria(s): Avellar, M. G. B. de; Horvath, J. E.
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

06/11/2013

06/11/2013

2012

Resumo

We used the statistical measurements of information entropy, disequilibrium and complexity to infer a hierarchy of equations of state for two types of compact stars from the broad class of neutron stars, namely, with hadronic composition and with strange quark composition. Our results show that, since order costs energy. Nature would favor the exotic strange stars even though the question of how to form the strange stars cannot be answered within this approach. (C) 2012 Elsevier B.V. All rights reserved.

CAPES

FAPESP

CNPq Agency (Brazil)

Identificador

PHYSICS LETTERS A, AMSTERDAM, v. 376, n. 12-13, pp. 1085-1089, FEB, 2012

0375-9601

http://www.producao.usp.br/handle/BDPI/41999

doi:10.1016/j.physleta.2012.02.012

http://www.sciencedirect.com/science/article/pii/S0375960112001223

Idioma(s)

eng

Publicador

ELSEVIER SCIENCE BV

AMSTERDAM

Relação

PHYSICS LETTERS A

Direitos

closedAccess

Copyright ELSEVIER SCIENCE BV

Palavras-Chave #INFORMATION ENTROPY #COMPLEXITY #SELF-ORGANIZATION #NEUTRON STARS #STRANGE STARS #EQUATION OF STATE #NEUTRON-STAR #STRANGE STARS #MATTER #EQUATION #PHYSICS, MULTIDISCIPLINARY
Tipo

article

original article

publishedVersion