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

Also sorted by date
Last updated Mar 26, 2005.

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).

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).

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

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

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

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

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).

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).

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).

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).

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).

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).

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

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).

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).

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).

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

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

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).

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).

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

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

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

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

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

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).

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).

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

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

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

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

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).

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).

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).

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

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).

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

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

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).

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).

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).

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