Artículo

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Abstract:

A method is proposed of finding approximately the equilibrium configurations of nonrotating neutron stars without choosing any particular field equation for the metric. The method consists in choosing interpolation functions for the metric coefficients inside the star and matching them to that of the external metric at the body surface. In particular, the maximum mass a neutron star may have against gravitational collapse is studied, and a good agreement is found when compared with general relativistic results. © 1987 Plenum Publishing Corporation.

Registro:

Documento: Artículo
Título:Maximum mass of a Neutron star in metric theories of gravitation
Autor:Lousto, C.O.
Filiación:Instituto de Astronomía y Física del Espacio, Cas. Corr. 67 Suc. 28, Buenos Aires, 1428, Argentina
Año:1987
Volumen:19
Número:6
Página de inicio:637
Página de fin:642
DOI: http://dx.doi.org/10.1007/BF00762559
Título revista:General Relativity and Gravitation
Título revista abreviado:Gen Relat Gravit
ISSN:00017701
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00017701_v19_n6_p637_Lousto

Referencias:

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  • Castagnino, M. A. and Lousto, C. O. (1986). Il Nuovo Cim

Citas:

---------- APA ----------
(1987) . Maximum mass of a Neutron star in metric theories of gravitation. General Relativity and Gravitation, 19(6), 637-642.
http://dx.doi.org/10.1007/BF00762559
---------- CHICAGO ----------
Lousto, C.O. "Maximum mass of a Neutron star in metric theories of gravitation" . General Relativity and Gravitation 19, no. 6 (1987) : 637-642.
http://dx.doi.org/10.1007/BF00762559
---------- MLA ----------
Lousto, C.O. "Maximum mass of a Neutron star in metric theories of gravitation" . General Relativity and Gravitation, vol. 19, no. 6, 1987, pp. 637-642.
http://dx.doi.org/10.1007/BF00762559
---------- VANCOUVER ----------
Lousto, C.O. Maximum mass of a Neutron star in metric theories of gravitation. Gen Relat Gravit. 1987;19(6):637-642.
http://dx.doi.org/10.1007/BF00762559