2020MNRAS.498..344W

Query : 2020MNRAS.498..344W

2020MNRAS.498..344W - Mon. Not. R. Astron. Soc., 498, 344-354 (2020/October-2)

Cooling of hybrid neutron stars with microscopic equations of state.

WEI J.-B., BURGIO G.F., SCHULZE H.-J. and ZAPPALA D.

Abstract (from CDS):

We model the cooling of hybrid neutron stars combining a microscopic nuclear equation of state in the Brueckner-Hartree-Fock approach with different quark models. We then analyse the neutron star cooling curves predicted by the different models and single out the preferred ones. We find that the possibility of neutron p-wave pairing can be excluded in our scenario.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

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

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 PSR J0030+0451 Psr 00 30 27.42348 +04 51 39.7144           ~ 596 1
2 PSR J0740+6620 Psr 07 40 45.799 +66 20 33.60           ~ 395 0
3 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0
4 NAME Cas A SNR 23 23 26.0 +58 48 41     14.30     ~ 3033 1

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