Influence of σ* and φ Mesons on Λ Hyperon 1 S 0 Superfluidity in Neutron Star Matter
Author:
Publisher
IOP Publishing
Subject
General Physics and Astronomy
Link
https://iopscience.iop.org/article/10.1088/0256-307X/29/5/059701/pdf
Reference31 articles.
1. Temperature effects on hyperon superfluids in neutron stars
2. Baryon superfluidity and neutrino emissivity of neutron stars
3. Occurrence of Hyperon Superfluidity in Neutron Star Cores
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1. Direct Urca Processes Involving Proton 1 S 0 Superfluidity in Neutron Star Cooling;Communications in Theoretical Physics;2018-04
2. Reinvestigation of the electron fraction and electron Fermi energy of neutron star;Astronomische Nachrichten;2017-12
3. The influence of antikaon condensations on nucleon 1S0 superfluidity in neutron star matter;Monthly Notices of the Royal Astronomical Society;2017-11-23
4. Effects of Tensor Couplings on Nucleonic Direct URCA Processes in Neutron Star Matter;Chinese Physics Letters;2016-09
5. Numerically fitting the electron Fermi energy and the electron fraction in a neutron star;International Journal of Modern Physics D;2016-01
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