Cooling of neutron stars. Hadronic model

Astronomy and Astrophysics

Volumn 424, Issue 3, 2004, Pages 979-992

  Blaschke, D ^a,b,c   Grigorian, H ^a,d   Voskresensky, D N ^e,f  

^a UNIVERSITY OF ROSTOCK   (Germany)

^b JOINT INSTITUTE FOR NUCLEAR RESEARCH   (Russian Federation)

^c BIELEFELD UNIVERSITY   (Germany)

^d YEREVAN STATE UNIVERSITY   (Armenia)

^e GSI HELMHOLTZZENTRUM FÜR SCHWERIONENFORSCHUNG GMBH   (Germany)

^f NATIONAL RESEARCH NUCLEAR UNIVERSITY MEPHI   (Russian Federation)

Author keywords

Dense matter; Equation of state; Neutrinos; Stars: evolution; Stars: neutron; Stars: pulsars: general

Indexed keywords

COOLING; DATA REDUCTION; EQUATIONS OF STATE; NEUTRONS; PHOTONS; SPECIFIC HEAT; X RAYS;

DENSE MATTER; NEUTRINOS; STARS: EVOLUTION; STARS: NEUTRON; STARS: PULSARS: GENERAL;

ASTROPHYSICS;

EID: 4644293706     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20040404     Document Type: Article

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