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Literature Catalog: White Dwarf / Neutron Star / Black Hole Mergers: Quasiequilibrium sequences

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Last updated Mar 26, 2005.

2005

M. Ishii, M. Shibata, and Y. Mino, Black hole tidal problem in the Fermi normal coordinates, Phys. Rev. D 71, 044017 (2005).

M. Bejger, D. Gondek-Rosinska, E. Gourgoulhon, P. Haensel, K. Taniguchi, and J.L. Zdunik, , Astron. Astrophys. 431, 297 (2005).

2004

T.W. Baumgarte, M.L. Skoge, and S.L. Shapiro, Black hole-neutron star binaries in general relativity: Quasiequilibrium formulation, Phys. Rev. D 70, 064040 (2004).

M. Shibata, K. Uryu, and J.L. Friedman, Deriving formulations for numerical computation of binary neutron stars in quasicircular orbits, Phys. Rev. D 70, 044044 (2004).
Erratum: Phys. Rev. D 70, 129901 (2004).

T. Mora and C.M. Will, Post-Newtonian diagnostic of quasiequilibrium binary configurations of compact objects, Phys. Rev. D 69, 104021 (2004).

M. Ishii and M. Shibata, Numerical Study of the Tidal Disruption of Neutron Stars Moving around a Black Hole - Compressible Jeans and Roche Problems, Prog. Theoret. Phys. 112, 399 (2004).

M. Prakash and J.M. Lattimer, A tale of two mergers: searching for strangeness in compact stars, J. Phys. G: Nucl. Part. Phys. 30, S451 (2004).

2003

K. Taniguchi and E. Gourgoulhon, Various features of quasiequilibrium sequences of binary neutron stars in general relativity, Phys. Rev. D 68, 124025 (2003).

P. Marronetti and S.L. Shapiro, Relativistic models for binary neutron stars with arbitrary spins, Phys. Rev. D 68, 104024 (2003).

2002

K. Taniguchi and 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).

J.A. Faber, P. Grandclement, F.A. Rasio, and K. Taniguchi, Measuring Neutron Star Radii with Gravitational Wave Detectors, Phys. Rev. Lett. 89, 231102 (2002).

F. Usui and 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).

K. Taniguchi and E. Gourgoulhon, Equilibrium sequences of synchronized and irrotational binary systems composed of different mass stars in Newtonian gravity, Phys. Rev. D 65, 044027 (2002).

M.D. Duez, T.W. Baumgarte, S.L. Shapiro, M. Shibata, and K. Uryu, Comparing the inspiral of irrotational and corotational binary neutron stars, Phys. Rev. D 65, 024016 (2002).

2001

K. Taniguchi, E. Gourgoulhon, and S. Bonazzola, Quasiequilibrium sequences of synchronized and irrotational binary neutron stars in general relativity. II. Newtonian limits, Phys. Rev. D 64, 064012 (2001).

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

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

M. Shibata and K. Uryu, Computation of gravitational waves from inspiraling binary neutron stars in quasiequilibrium circular orbits: Formulation and calibration, Phys. Rev. D 64, 104017 (2001).

2000

K. Taniguchi and T. Nakamura, Equilibrium sequences of irrotational binary polytropic stars: The case of double polytropic stars, Phys. Rev. D 62, 044040 (2000).

K. Taniguchi and T. Nakamura, Almost Analytic Solutions to Equilibrium Sequences of Irrotational Binary Polytropic Stars for n = 1, Phys. Rev. Lett. 84, 581 (2000).

F. Usui, K. Uryu, and Y. Eriguchi, New numerical scheme to compute three-dimensional configurations of quasiequilibrium compact stars in general relativity: Application to synchronously rotating binary star systems, Phys. Rev. D 61, 024039 (2000).

P. Wiggins and D. Lai, Tidal Interaction between a Fluid Star and a Kerr Black Hole in Circular Orbit, Astrophys. J. 532, 530 (2000).

M. Vallisneri, Prospects for Gravitational-Wave Observations of Neutron-Star Tidal Disruption in Neutron-Star-Black-Hole Binaries, Phys. Rev. Letters 84, 3519 (2000).

K. Uryu, M. Shibata, and Y. Eriguchi, Properties of general relativistic, irrotational binary neutron stars in close quasiequilibrium orbits: Polytropic equations of state. Phys. Rev. D 62, 104015 (2000).

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

1999

K. Uryu and Y. Eriguchi, Newtonian models for black hole-gaseous star close binary systems, Monthly Notices of the RAS 303, 329 (1999).

K. Taniguchi, Irrotational and Incompressible Binary Systems in the First Post-Newtonian Approximation of General Relativity, Prog. Theoret. Phys. 101, 283 (1999).

P. Marronetti, G.J. Mathews, and J.R. Wilson, Irrotational binary neutron stars in quasiequilibrium, Phys. Rev. D 60, 087301 (1999).

W.C.G. Ho and D. Lai, Resonant tidal excitations of rotating neutron stars in coalescing binaries, Monthly Notices of the RAS 308, 153 (1999).

S. Bonazzola, E. Gourgoulhon, and J.-A. Marck, Numerical Models of Irrotational Binary Neutron Stars in General Relativity, Phys. Rev. Letters 82, 892 (1999).

1998

S.A. Teukolsky, Irrotational Binary Neutron Stars in Quasi-Equilibrium in General Relativity, Astrophys. J. 504, 442 (1998).

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

T.W. Baumgarte, G.B. Cook, M.A. Scheel, S.L. Shapiro, and S.A. Teukolsky, General relativistic models of binary neutron stars in quasiequilibrium, Phys. Rev. D 57, 7299 (1998).

1997

K.C.B. New and J.E. Tohline, The Relative Stability against Merger of Close, Compact Binaries, Astrophys. J. 490, 311 (1997).

S. Bonazzola, E. Gourgoulhon, and J.-A. Marck, Relativistic formalism to compute quasiequilibrium configurations of nonsynchronized neutron star binaries, Phys. Rev. D 56, 7740 (1997).

J.C. Lombardi, Jr., F.A. Rasio, and S.L. Shapiro, Post-Newtonian models of binary neutron stars, Phys. Rev. D 56, 3416 (1997),

M. Shibata and K. Taniguchi, Solving the Darwin problem in the first post-Newtonian approximation of general relativity: Compressible model, Phys. Rev. D 56, 811 (1997).

K. Taniguchi and M. Shibata, Solving the Darwin problem in the first post-Newtonian approximation of general relativity, Phys. Rev. D 56, 798 (1997).

T.W. Baumgarte, G.B. Cook, M.A. Scheel, S.L. Shapiro, and S.A. Teukolsky, Binary Neutron Stars in General Relativity: Quasiequilibrium Models, Phys. Rev. Lett. 79, 1182 (1997).

M. Shibata, Numerical study of synchronized binary neutron stars in the post-Newtonian approximation of general relativity, Phys. Rev. D 55, 6019 (1997).

1996

D. Lai and A.G. Wiseman, Innermost stable circular orbit of inspiraling neutron-star binaries: Tidal effects, post-Newtonian effects, and the neutron-star equation of state, Phys. Rev. D 54, 3958 (1996).

K. Taniguchi and T. Nakamura, Innermost Stable Circular Orbit of Coalescing Neutron Star-Black Hole Binary - Generalized Pseudo-Newtonian Potential Approach, Prog. Theoret. Phys. 96, 693 (1996).

D. Lai, Tidal Stablization of Neutron Stars and White Dwarfs, Phys. Rev. Letters 76, 4878 (1996).

1995

D. Lai and S.L. Shapiro, Hydrodynamics of coalescing binary neutron stars: Ellipsoidal treatment, Astrophys. J. 443, 705 (1995).

1994

D. Lai, F.A. Rasio, and S.L. Shapiro, Hydrodynamics of rotating stars and close binary interactions: Compressible ellipsoid models, Astrophys. J. 437, 742 (1994).

D. Lai, F.A. Rasio, and S.L. Shapiro, Equilibrium, stability, and orbital evolution of close binary systems, Astrophys. J. 423, 344 (1994).

D. Lai, F.A. Rasio, and S.L. Shapiro, Hydrodynamic instability and coalescence of binary neutron stars, Astrophys. J. 420, 811 (1994).

1993

D. Lai, F.A. Rasio, and S.L. Shapiro, Hydrodynamic instability and coalescence of close binary systems, Astrophys. J. Letters 406, L63 (1993).

D. Lai, F.A. Rasio, and S.L. Shapiro, Ellipsoidal figures of equilibrium - Compressible models, Astrophys. J. Suppl. 88, 205 (1993).

1992

L. Bildsten and C. Cutler, Tidal interactions of inspiraling compact binaries, Astrophys. J. 400, 175 (1992).

C.S. Kochanek, Coalescing binary neutron stars, Astrophys. J. 398, 234 (1992).

P. Jaranowski and A. Krolak, Detectability of the gravitational wave signal from a close neutron star binary with mass transfer, Astrophys. J. 394, 586 (1992).

1986

I. Hachisu, A versatile method for obtaining structures of rapidly rotating stars. II - Three-dimensional self-consistent field method, Astrophys. J. Supplement 62, 461 (1986).

1977

J.P.A. Clark and D.M. Eardley, Evolution of close neutron star binaries, Astrophys. J. 215, 311 (1977).