Cooling of neutron stars in “nuclear medium cooling scenario” with stiff equation of state including hyperons-Reference-Cited by-同舟云学术

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Cooling of neutron stars in “nuclear medium cooling scenario” with stiff equation of state including hyperons

Published:2018-12 Issue: Volume:980 Page:105-130
ISSN:0375-9474
Container-title:Nuclear Physics A
language:en
Short-container-title:Nuclear Physics A

Author:

Grigorian H.,Voskresensky D.N.,Maslov K.A.^ORCID

Funder

Ministry of Education and Science of the Russian Federation

Russian Science Foundation

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics

Reference126 articles.

1. Neutron stars. 2. Neutrino-cooling and observability;Bahcall;Phys. Rev.,1965

2. Thermal properties and detectability of neutron stars. I. Cooling and heating of neutron stars;Tsuruta;Phys. Rep.,1979

3. Black Holes, White Dwarfs and Neutron Stars: The Physics of Compact Objects;Shapiro,1983

4. Pion degrees of freedom in nuclear matter;Migdal;Phys. Rep.,1990

5. Neutrino emission from neutron stars;Yakovlev;Phys. Rep.,2001

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