SIMBAD references

2015MNRAS.452..540B - Mon. Not. R. Astron. Soc., 452, 540-548 (2015/September-1)

Statistical theory of thermal evolution of neutron stars - II. Limitations on direct Urca threshold.

BEZNOGOV M.V. and YAKOVLEV D.G.

Abstract (from CDS):

We apply our recently suggested statistical approach to thermal evolution of isolated neutron stars and accreting quasi-stationary neutron stars in X-ray transients for constraining the position and relative broadening α of the direct Urca threshold of powerful neutrino emission in neutron star cores. We show that most likely explanation of observations corresponds to α ~ 0.08-0.10 and to the neutron star mass, at which the direct Urca process is open, MD ~ 1.6-1.8M.

Abstract Copyright: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2015)

Journal keyword(s): dense matter - equation of state - neutrinos - stars: neutron

Simbad objects: 48

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2021.06.13-08:29:12

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