1.
Phys Rev Lett
; 85(10): 2048-51, 2000 Sep 04.
Article
in English
| MEDLINE
| ID: mdl-10970460
ABSTRACT
Baryon and quark superfluidity in the cooling of neutron stars are investigated. Future observations will allow us to constrain combinations of the neutron or Lambda-hyperon pairing gaps and the star's mass. However, in a hybrid star with a mixed phase of hadrons and quarks, quark gaps larger than a few tenths of an MeV render quark matter virtually invisible for cooling. If the quark gap is smaller, quark superfluidity could be important, but its effects will be nearly impossible to distinguish from those of other baryonic constituents.
2.
Phys Rev D Part Fields
; 52(2): 661-665, 1995 Jul 15.
Article
in English
| MEDLINE
| ID: mdl-10019287
3.
4.
Phys Rev D Part Fields
; 40(2): 309-314, 1989 Jul 15.
Article
in English
| MEDLINE
| ID: mdl-10011820
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