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Volumn 61, Issue 12, 2000, Pages

Revised relativistic hydrodynamical model for neutron-star binaries

Author keywords

[No Author keywords available]

Indexed keywords


EID: 3242668994     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.61.127304     Document Type: Article
Times cited : (37)

References (26)
  • 18
    • 0004251401 scopus 로고
    • C. R. Evans, Ph.D. thesis, University of Texas, 1985., L. Smarr
    • J. W. York, Jr., in Sources of Gravitational Radiation, edited by L. Smarr (Cambridge University Press, Cambridge, England, 1979), p. 83;C. R. Evans, Ph.D. thesis, University of Texas, 1985.
    • (1979) Sources of Gravitational Radiation , pp. 83
    • York, J.W.1
  • 19
    • 85037190997 scopus 로고    scopus 로고
    • S. Bonazzola, E. Gourgoulhon, and J.-A. Marck, in Proceedings of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, Paris, France, 1998, edited by J. Paul, T. Montmerle, and E. Aubourg (CEA, Saclay, 1999)
    • Bonazzola, S.1    Gourgoulhon, E.2    Marck, J.-A.3
  • 23
    • 85037222125 scopus 로고    scopus 로고
    • The equation of state utilized in the present simulation gives a gravitational mass which differs by (Formula presented) from the calculations of
    • The equation of state utilized in the present simulation gives a gravitational mass which differs by (Formula presented) from the calculations of 4. This difference is insignificant for purposes of the present comparison.


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