Theory of cooling neutron stars versus observations

2); 4) ((1) Ioffe Institute; A. D. Kaminker (1); A. Y. Potekhin (1; D. G. Yakovlev (1; ENS-Lyon); Notre Dame; (3) University of Michigan; (4) CRAL; O. Y. Gnedin (3); St. Petersburg; (2) JINA

arxiv: 0710.2047 · v2 · submitted 2007-10-10 · 🌌 astro-ph

Theory of cooling neutron stars versus observations

D. G. Yakovlev (1 , 2) , O. Y. Gnedin (3) , A. D. Kaminker (1) , A. Y. Potekhin (1 , 4) ((1) Ioffe Institute , St. Petersburg; (2) JINA , Notre Dame; (3) University of Michigan; (4) CRAL

show 1 more author

ENS-Lyon)

This is my paper

classification 🌌 astro-ph

keywords neutroncoolingtheoryobservationsstarstarsstatecomparing

0 comments

read the original abstract

We review current state of neutron star cooling theory and discuss the prospects to constrain the equation of state, neutrino emission and superfluid properties of neutron star cores by comparing the cooling theory with observations of thermal radiation from isolated neutron stars.

This paper has not been read by Pith yet.

Theory of cooling neutron stars versus observations

discussion (0)