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: email@example.com
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: firstname.lastname@example.org
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
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.