Title of article
Neutron star cooling Original Research Article
Author/Authors
D.G. Yakovlev، نويسنده , , O.Y. Gnedin، نويسنده , , M.E. Gusakov، نويسنده , , A.D. Kaminker، نويسنده , , K.P. Levenfish، نويسنده , , A.Y. Potekhin، نويسنده ,
Issue Information
هفته نامه با شماره پیاپی سال 2005
Pages
10
From page
590
To page
599
Abstract
The impact of nuclear physics theories on cooling of isolated neutron stars is analyzed. Physical properties of neutron star matter important for cooling are reviewed such as composition, the equation of state, superfluidity of various baryon species, neutrino emission mechanisms. Theoretical results are compared with observations of thermal radiation from neutron stars. Current constraints on theoretical models of dense matter, derived from such a comparison, are formulated.
Journal title
Nuclear physics A
Serial Year
2005
Journal title
Nuclear physics A
Record number
1202270
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