Entropy, complexity and disequilibrium in compact stars

dc.creatorAvellar, M. G. B. de
dc.creatorHorvath, J. E.
dc.date.accessioned2013-11-06T12:49:00Z
dc.date.accessioned2018-07-04T16:17:22Z
dc.date.available2013-11-06T12:49:00Z
dc.date.available2018-07-04T16:17:22Z
dc.date.created2013-11-06T12:49:00Z
dc.date.issued2012
dc.identifierPHYSICS LETTERS A, AMSTERDAM, v. 376, n. 12-13, pp. 1085-1089, FEB, 2012
dc.identifier0375-9601
dc.identifierhttp://www.producao.usp.br/handle/BDPI/41999
dc.identifierdoi:10.1016/j.physleta.2012.02.012
dc.identifierhttp://www.sciencedirect.com/science/article/pii/S0375960112001223
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1633928
dc.description.abstractWe 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.
dc.languageeng
dc.publisherELSEVIER SCIENCE BV
dc.publisherAMSTERDAM
dc.relationPHYSICS LETTERS A
dc.rightsCopyright ELSEVIER SCIENCE BV
dc.rightsclosedAccess
dc.subjectINFORMATION ENTROPY
dc.subjectCOMPLEXITY
dc.subjectSELF-ORGANIZATION
dc.subjectNEUTRON STARS
dc.subjectSTRANGE STARS
dc.subjectEQUATION OF STATE
dc.titleEntropy, complexity and disequilibrium in compact stars
dc.typeArtículos de revistas


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