2004A&A...424..979B


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.13CEST23:59:41

2004A&A...424..979B - Astronomy and Astrophysics, volume 424, 979-992 (2004/9-4)

Cooling of neutron stars. Hadronic model.

BLASCHKE D., GRIGORIAN H. and VOSKRESENSKY D.N.

Abstract (from CDS):

We study the cooling of isolated neutron stars. The main cooling regulators are introduced: equation of state (EoS), thermal transport, heat capacity, neutrino and photon emissivity, superfluid nucleon gaps. The neutrino emissivity includes the main processes. A strong impact of medium effects on the cooling rates is demonstrated. Taking into account medium effects on reaction rates and on nucleon superfluid gaps modern experimental data can be well explained.

Abstract Copyright:

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

CDS comments: JC737-3C3J is a misprint for PSR J0737-3039.

Simbad objects: 2

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Number of rows : 2

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 PSR B1055-52 Psr 10 57 58.970 -52 26 56.52           ~ 681 0
2 PSR J1915+1606 Psr 19 15 27.99999 +16 06 27.4034     22.5     ~ 920 1

    Equat.    Gal    SGal    Ecl

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2020.07.13-23:59:41

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