The equation of state of dense matter: from nuclear collisions to neutron stars
نویسندگان
چکیده
منابع مشابه
The Equation of State of Dense Matter: from Nuclear Collisions to Neutron Stars
The Equation of State (EoS) of dense matter represents a central issue in the study of compact astrophysical objects and heavy ion reactions at intermediate and relativistic energies. We have derived a nuclear EoS with nucleons and hyperons within the Brueckner-Hartree-Fock approach, and joined it with quark matter EoS. For that, we have employed the MIT bag model, as well as the Nambu–Jona-Las...
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Apparent (radiation) radius of neutron star, R∞, depends on the star gravitational mass in quite a different way than the standard coordinate radius in the Schwarzschild metric, R. We show that, for a broad set of equations of state of dense matter, R∞(Mmax) for the configurations with maximum allowable masses is very close to the absolute lower bound on R∞ at fixed M , resulting from the very ...
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ژورنال
عنوان ژورنال: Journal of Physics G: Nuclear and Particle Physics
سال: 2007
ISSN: 0954-3899,1361-6471
DOI: 10.1088/0954-3899/35/1/014048