SIMBAD references

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

goto Full paper

goto View the references in ADS

To bookmark this query, right click on this link: simbad:2020MNRAS.498..344W and select 'bookmark this link' or equivalent in the popup menu