Energy release due to antineutrino untrapping and diquark condensation in hot quark star evolution

Astronomy and Astrophysics

Volumn 416, Issue 3, 2004, Pages 991-996

  Aguilera, D N ^a,b   Blaschke, D ^a,c   Grigorian, H ^a,d  

^a UNIVERSITY OF ROSTOCK   (Germany)

^b INSTITUTO DE FÍSICA ROSARIO   (Argentina)

^c JOINT INSTITUTE FOR NUCLEAR RESEARCH   (Russian Federation)

^d YEREVAN STATE UNIVERSITY   (Armenia)

Author keywords

Dense matter; Stars: evolution; Stars: interiors; Stars: neutron

Indexed keywords

CONDENSATION; COOLING; ENERGY GAP; FERMI LEVEL; GAMMA RAYS; GRAVITATIONAL EFFECTS; SUPERCONDUCTING MATERIALS;

DENSE MATTERS; STARS;

ASTROPHYSICS;

EID: 1642588134     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031742     Document Type: Article

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