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Literature Catalog: Numerical Relativity Quasi-Equilibrium Approximations to Compact Binary Systems

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Last updated March 21, 2003.

T. Baumgarte, G. Cook, M. Scheel, S. Shapiro, S. Teukolsky, " General relativistic models of binary neutron stars in quasiequilibrium", Phys. Rev. D 57, 7299-7311 (1998).

T. Baumgarte, G. Cook, M. Scheel, S. Shapiro, S. Teukolsky, " Stability of relativistic neutron stars in binary orbit", Phys. Rev. D 57, 6181-6184 (1998).

T. Baumgarte, G. Cook, M. Scheel, S. Shapiro, S. Teukolsky, " Binary Neutron Stars in General Relativity: Quasiequilibrium Models", Phys. Rev. Lett. 79, 1182-1185 (1997).

T. Baumgarte, " Innermost stable circular orbit of binary black holes", Phys. Rev. D 62, 024018 (2000).

S. Bonazzola, E. Gourgoulhon, J.-A. Marack, " Numerical Models of Irrotational Binary Neutron Stars in General Relativity", Phys. Rev. Lett. 82, 892-895 (1999).

M. Duez, T. Baumgarte, S. Shapiro, M. Shibata, and K. Uryu, " Comparing the inspiral of irrotational and corotational binary neutron stars", Phys. Rev. D 65, 024016 (2001).

M. Duez, T. Baumgarte, S. Shapiro, " Computing the complete gravitational wavetrain from relativistic binary inspiral", Phys. Rev. D 63, 084030 (2001).

E. Gourgoulhon, P. Grandclement, S. Bonazzola, " Binary black holes in circular orbits. I. A global spacetime approach", Phys. Rev. D 65, 044020 (2002).

E. Gourgoulhon, P. Grandclement, K. Taniguchi, J.-A. Marck, S. Bonazzola, " Quasiequilibrium sequences of synchronized and irrotational binary neutron stars in general relativity: Method and tests", Phys. Rev. D 63, 064029 (2001).

T. Mora, C. Will " Numerically generated quasiequilibrium orbits of black holes: Circular or eccentric?", Phys. Rev. D 66, 101501(R) (2002).

M. Shibata, " Relativistic formalism for computation of irrotational binary stars in quasiequilibrium states", Phys. Rev. D 58, 024012 (1998).

M. Skoge, T. Baumgarte " Comparing criteria for circular orbits in general relativity" Phys. Rev. D 66, 107501 (2002).

K. Taniguchi, E. Gourgoulhon " Quasiequilibrium sequences of synchronized and irrotational binary neutron stars in general relativity. III. Identical and different mass stars with gamma=2", Phys. Rev. D 66, 104019 (2002).

K. Uryu, Y. Eriguchi, " New numerical method for constructing quasiequilibrium sequences of irrotational binary neutron stars in general relativity", Phys. Rev. D 61, 124023 (2000).

F. Usui, Y. Eriguchi, " Quasiequilibrium sequences of synchronously rotating binary neutron stars with constant rest masses in general relativity: Another approach without using the conformally flat condition", Phys. Rev. D 65, 064030 (2002).

 


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