Maximum mass of neutron stars

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Título:	Maximum mass of neutron stars
Autor/a:	Schulze, H.-J.; Polls Martí, Artur; Ramos Gómez, Àngels; Vidaña Haro, Isaac
Otros autores:	Universitat de Barcelona
Abstract:	We determine the structure of neutron stars within a Brueckner-Hartree-Fock approach based on realistic nucleon-nucleon, nucleon-hyperon, and hyperon-hyperon interactions. Our results indicate rather low maximum masses below 1.4 solar masses. This feature is insensitive to the nucleonic part of the EOS due to a strong compensation mechanism caused by the appearance of hyperons and represents thus strong evidence for the presence of nonbaryonic "quark" matter in the interior of heavy stars.
Materia(s):	-Astrofísica nuclear -Reaccions nuclears -Nuclear astrophysics -Nuclear reactions
Derechos:	(c) The American Physical Society, 2006
Tipo de documento:	Artículo Artículo - Versión publicada
Editor:	The American Physical Society
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Vidaña Haro, Isaac; Polls Martí, Artur; Ramos Gómez, Àngels; Schulze, H.-J.

Zhou, Xian-Rong; Polls Martí, Artur; Schulze, H.-J.; Vidaña Haro, Isaac

Schulze, H.-J.; Polls Martí, Artur; Ramos Gómez, Àngels

Vidaña Haro, Isaac; Polls Martí, Artur; Ramos Gómez, Àngels; Stoks, V. G. J.; Hjorth-Jensen, M.

Vidaña Haro, Isaac; Polls Martí, Artur; Ramos Gómez, Àngels; Engvik, L.; Hjorth-Jensen, M.

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