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