Numerical evolution of secular bar-mode instability induced by the gravitational radiation reaction in rapidly rotating neutron stars

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 70, Issue 8, 2004, Pages

  Shibata, Masaru ^a   Karino, Sigeyuki ^b  

^a UNIVERSITY OF TOKYO   (Japan)

^b SISSA   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

ARTICLE; ASTRONOMY; EVOLUTION; GRAVITY; INTERFEROMETRY; MAGNETIC FIELD; MATHEMATICAL MODEL; NEUTRON RADIATION;

EID: 84927701156     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.70.084022     Document Type: Article

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