Rotochemical heating of neutron stars

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dc.contributor.authorReisenegger, Andreas
dc.contributor.authorJofre, Paula
dc.contributor.authorFernandez, Rodrigo
dc.contributor.authorKantor, Elena
dc.date.accessioned2025-01-21T01:05:47Z
dc.date.available2025-01-21T01:05:47Z
dc.date.issued2006
dc.description.abstractThe electrostatic potential that keeps approximate charge neutrality in neutron star matter is self-consistently introduced into the formalism for "rotochemical heating" presented in a previous paper by Fernandez and Reisenegger. Although the new formalism is more rigorous, we show that its observable consequences are indistinguishable from those of the previous one, leaving the conclusions of the previous paper unchanged.
dc.fuente.origenWOS
dc.identifier.eissn1538-4357
dc.identifier.issn0004-637X
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/96015
dc.identifier.wosidWOS:000242913800046
dc.issue.numero1
dc.language.isoen
dc.pagina.final572
dc.pagina.inicio568
dc.revistaAstrophysical journal
dc.rightsacceso restringido
dc.subjectdense matter
dc.subjectpulsars : general
dc.subjectrelativity
dc.subjectstars : neutron
dc.subjectstars : rotation
dc.titleRotochemical heating of neutron stars
dc.typeartículo
dc.volumen653
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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