Neutron stars: probes for high density baryon pairing

Details Neutron stars: probes for high density baryon pairing Neutron stars: probes for high density baryon pairing

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995rmxfs..41..178p&link_type=abstract

Revista Mexicana de Fisica, vol. 41, Suplemento 1, pp. 178 - 184

Other

Neutron Stars, Baryons, Neutrinos, Superfluidity, Stellar Interiors

Scientific paper

We consider, in general terms, the early thermal evolution of an isolated neutron star, i.e., during the first 10^5 yrs after the supernova explosion when the cooling is driven by neutrino emission from the core. It is shown that, if fast neutrino emission is occuring, the surface temperature is actually determined by the critical temperature T_c at which the core baryons become superfluid and almost nothing else. In particular, the dependence on the actual neutrino emission process is very weak. In other terms, fast neutrino cooling neutron stars are thermometers for the highest T_c superfluid (superconductor) in the Universe. The observational data are briefly presented.

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