1 S 0 Nucleon Superfluidity in Neutron Star Matter
Author:
Publisher
IOP Publishing
Subject
General Physics and Astronomy
Link
https://iopscience.iop.org/article/10.1088/0256-307X/30/6/062101/pdf
Reference38 articles.
1. 1S0 proton and neutron superfluidity in β-stable neutron star matter
2. S01proton superfluidity in neutron star matter: Impact of bulk properties
3. Three types of cooling superfluid neutron stars: Theory and observations
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1. Study of tidal deformabilities of neutron stars using relativistic mean field theory containing <i>δ</i> mesons;Acta Physica Sinica;2023
2. The influence of antikaon condensations on nucleon 1S0 superfluidity in neutron star matter;Monthly Notices of the Royal Astronomical Society;2017-11-23
3. Effects of tensor couplings of ω and ρ mesons on 1S0 nucleon superfluidity in neutron star matter;International Journal of Modern Physics D;2016-04
4. Effects of δ mesons on baryonic direct Urca processes in neutron star matter;Chinese Physics C;2015-10
5. Singlet pairing gaps of neutrons and protons in hyperonic neutron stars;Research in Astronomy and Astrophysics;2015-04-29
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