New numerical scheme to compute three-dimensional configurations of quasiequilibrium compact stars in general relativity: Application to synchronously rotating binary star systems

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 61, Issue 2, 2000, Pages

  Eriguchi, Yoshiharu ^a  

^a UNIVERSITY OF TOKYO   (Japan)

^b SISSA   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 17044411742     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.61.024039     Document Type: Article

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