Rotochemical heating of neutron stars: Rigorous formalism with electrostatic potential perturbations

Reisenegger, A.; Jofré P.; Fernandez, R.; Kantor, E

Abstract

The 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 Fernández 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. © 2006. The American Astronomical Society. All rights reserved.

Más información

Título según WOS: Rotochemical heating of neutron stars: Rigorous formalism with electrostatic potential perturbations
Título según SCOPUS: Rotochemical heating of neutron stars: Rigorous formalism with electrostatic potential perturbations
Título de la Revista: ASTROPHYSICAL JOURNAL
Volumen: 653
Número: 1
Editorial: IOP PUBLISHING LTD
Fecha de publicación: 2006
Página de inicio: 568
Página final: 572
Idioma: English
URL: http://stacks.iop.org/0004-637X/653/i=1/a=568
DOI:

10.1086/506601

Notas: ISI, SCOPUS