Volume 444, Number 3, December IV 2005
|Page(s)||913 - 929|
|Section||Stellar structure and evolution|
|Published online||05 December 2005|
Medium effects in cooling of neutron stars and the 3P neutron gap
Institut für Physik, Universität Rostock, Universitätsplatz 3, 18051 Rostock, Germany e-mail: firstname.lastname@example.org
2 Department of Physics, Yerevan State University, Alex Manoogian Str. 1, 375025 Yerevan, Armenia
3 Gesellschaft für Schwerionenforschung mbH, Planckstr. 1, 64291 Darmstadt, Germany e-mail: email@example.com
4 Moscow Institute for Physics and Engineering, Kashirskoe sh. 31, 115409 Moscow, Russia
Accepted: 2 August 2005
We study the dependence of the cooling of isolated neutron stars on the magnitude of the neutron gap. Our “nuclear medium cooling” scenario favors a suppressed value of the neutron gap.
Key words: dense matter / neutrinos / nuclear reactions, nucleosynthesis, abundances / ISM: evolution
© ESO, 2005
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