Neutrino Processes in Neutron Stars
The aim of these lectures is to introduce basic processes responsible for cooling of neutron stars and to show how to calculate the neutrino production rate in dense strongly interacting nuclear medium. The formalism is presented that treats on equal footing one-nucleon and multiple-nucleon proce...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
EDP Sciences
2010-10-01
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Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/20100703003 |