| Issue |
A&A
Volume 444, Number 3, December IV 2005
|
|
|---|---|---|
| Page(s) | 913 - 929 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361:20052799 | |
| Published online | 05 December 2005 | |
Medium effects in cooling of neutron stars and the 3P
neutron gap
1
Institut für Physik, Universität Rostock, Universitätsplatz 3, 18051 Rostock, Germany e-mail: hovik.grigorian@uni-rostock.de
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: d.voskresensky@gsi.de
4
Moscow Institute for Physics and Engineering, Kashirskoe sh. 31, 115409 Moscow, Russia
Received:
31
January
2005
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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