 |
1 |
Abrahams, A.M., Bernstein, D.H., Hobill, D.W., Seidel, E., and Smarr, L.L., “Numerically
generated black-hole spacetimes: Interaction with gravitational waves”, Phys. Rev. D, 45,
3544–3558, (1992).
|
|
2 |
Abrahams, A.M., and Evans, C.R., “Critical behavior and scaling in vacuum axisymmetric
gravitational collapse”, Phys. Rev. Lett., 70, 2980–2983, (1993).
|
|
3 |
Abrahams, A.M., and Price, R.H., “Black-hole collisions from Brill-Lindquist initial data:
Predictions of perturbation theory”, Phys. Rev. D, 53, 1972–1976, (1996). [ gr-qc/9509020].
|
|
4 |
Anderson, A., and York Jr, J.W., “Hamiltonian Time Evolution for General Relativity”, Phys.
Rev. Lett., 81, 1154–1157, (1998). [gr-qc/9807041].
|
|
5 |
Arbona, A., Bona, C., Carot, J., Mas, L., Massó, J., and Stella, J., “Stuffed black holes”,
Phys. Rev. D, 57, 2397–2402, (1998). [gr-qc/9710111].
|
|
6 |
Arnowitt, R., Deser, S., and Misner, C.W., “The dynamics of general relativity”, in Witten, L.,
ed., Gravitation: An Introduction to Current Research, pp. 227–265, (Wiley, New York, 1962).
[DOI], [ADS].
|
|
7 |
Asada, H., “Formulation for the internal motion of quasiequilibrium configurations in general
relativity”, Phys. Rev. D, 57, 7292–7298, (1998). [gr-qc/9804003].
|
|
8 |
Bardeen, J.M., “A Variational Principle for Rotating Stars in General Relativity”, Astrophys.
J., 162, 71–95, (1970).
|
|
9 |
Bardeen, J.M., and Wagoner, R.V., “Relativistic Disks. I. Uniform Rotation”, Astrophys. J.,
167, 359–423, (1971).
|
|
10 |
Baumgarte, T.W., “Innermost stable circular orbit of binary black holes”, Phys. Rev. D, 62,
024018, 1–8, (2000). [DOI], [ADS].
|
|
11 |
Baumgarte, T.W., Cook, G.B., Scheel, M.A., Shapiro, S.L., and Teukolsky, S.A., “Binary
Neutron Stars in General Relativity: Quasi-Equilibrium Models”, Phys. Rev. Lett., 79,
1182–1185, (1997). [gr-qc/9704024].
|
|
12 |
Baumgarte, T.W., Cook, G.B., Scheel, M.A., Shapiro, S.L., and Teukolsky, S.A., “General
relativistic models of binary neutron stars in quasiequilibrium”, Phys. Rev. D, 57, 7299–7311,
(1998). [DOI], [ADS], [gr-qc/9709026].
|
|
13 |
Baumgarte, T.W., Cook, G.B., Scheel, M.A., Shapiro, S.L., and Teukolsky, S.A., “The
Stability of Relativistic Neutron Stars in Binary Orbit”, Phys. Rev. D, 57, 6181–6184, (1998).
[gr-qc/9705023].
|
|
14 |
Bildsten, L., and Cutler, C., “Tidal interactions of inspiraling compact binaries”, Astrophys.
J., 400, 175–180, (1992).
|
|
15 |
Bishop, N.T., Isaacson, R.A., Maharaj, M., and Winicour, J., “Black hole data via a Kerr–Schild
approach”, Phys. Rev. D, 57, 6113–6118, (1998). [gr-qc/9711076].
|
|
16 |
Bocquet, M., Bonazzola, S., Gourgoulhon, E., and Novak, J., “Rotating neutron star models
with a magnetic field”, Astron. Astrophys., 301, 757–775, (1995). [ADS], [gr-qc/9503044].
|
|
17 |
Bona, C., and Massó, J., “Harmonic synchronizations of spacetime”, Phys. Rev. D, 38,
2419–2422, (1988).
|
|
18 |
Bonazzola, S., Gourgoulhon, E., and Marck, J.-A., “A relativistic formalism to compute
quasi-equilibrium configurations of non-synchronized neutron star binaries”, Phys. Rev. D, 56,
7740–7749, (1997). [gr-qc/9710031].
|
|
19 |
Bonazzola, S., Gourgoulhon, E., and Marck, J.-A., “Numerical approach for high precision
3D relativistic star models”, Phys. Rev. D, 58, 104020, 1–14, (1998). [DOI], [ADS],
[astro-ph/9803086].
|
|
20 |
Bonazzola, S., Gourgoulhon, E., and Marck, J.-A., “Numerical Models of Irrotational Binary
Neutron Stars in General Relativity”, Phys. Rev. Lett., 82, 892–895, (1999). [DOI], [ADS],
[gr-qc/9810072].
|
|
21 |
Bonazzola, S., Gourgoulhon, E., Salgado, M., and Marck, J.-A., “Axisymmetric rotating
relativistic bodies: A new numerical approach for ‘exact’ solutions”, Astron. Astrophys., 278,
421–443, (1993). [ADS].
|
|
22 |
Bonazzola, S., and Schneider, J., “An Exact Study of Rigidly and Rapidly Rotating Stars in
General Relativity with Application to the Crab Pulsar”, Astrophys. J., 191, 273–286, (1974).
|
|
23 |
Bowen, J.M., “General form for the longitudinal momentum of a spherically symmetric source”,
Gen. Relativ. Gravit., 11, 227–231, (1979).
|
|
24 |
Bowen, J.M., “General solution for flat-space longitudinal momentum”, Gen. Relativ. Gravit.,
14, 1183–1191, (1982).
|
|
25 |
Bowen, J.M., and York Jr, J.W., “Time-asymmetric initial data for black holes and black-hole
collisions”, Phys. Rev. D, 21, 2047–2056, (1980).
|
|
26 |
Bowen, J.W., Rauber, J., and York Jr, J.W., “Two black holes with axisymmetric parallel
spins: Initial data”, Class. Quantum Grav., 1, 591–610, (1984).
|
|
27 |
Brandt, S., and Brügmann, B., “A simple construction of initial data for multiple black holes”,
Phys. Rev. Lett., 78, 3606–3609, (1997). [gr-qc/9703066].
|
|
28 |
Brandt, S.R., and Seidel, E., “Evolution of distorted rotating black holes. I: Methods and tests”,
Phys. Rev. D, 52, 856–869, (1995). [gr-qc/9412072].
|
|
29 |
Brandt, S.R., and Seidel, E., “Evolution of distorted rotating black holes. II: Dynamics and
analysis”, Phys. Rev. D, 52, 870–886, (1995). [gr-qc/9412073].
|
|
30 |
Brandt, S.R., and Seidel, E., “Evolution of distorted rotating black holes. III: Initial data”,
Phys. Rev. D, 54, 1403–1416, (1996). [gr-qc/9601010].
|
|
31 |
Brill, D.R., and Lindquist, R.W., “Interaction Energy in Geometrostatics”, Phys. Rev., 131,
471–476, (1963). [DOI], [ADS].
|
|
32 |
Butterworth, E.M., “On the structure and stability of rapidly rotating fluid bodies in general
relativity. II. The structure of uniformly rotating pseudopolytropes”, Astrophys. J., 204,
561–572, (1976).
|
|
33 |
Butterworth, E.M., “On the Structure and Stability of Rapidly Rotating Fluid Bodies in
General Relativity. III. Beyond the Angular Velocity Peak”, Astrophys. J., 231, 219–223,
(1979).
|
|
34 |
Butterworth, E.M., and Ipser, J.R., “Rapidly Rotating Fluid Bodies in General Relativity”,
Astrophys. J. Lett., 200, L103–L106, (1975).
|
|
35 |
Butterworth, E.M., and Ipser, J.R., “On the structure and stability of rapidly rotating fluid
bodies in general relativity. I. The numerical method for computing structure and its application
to uniformly rotating homogeneous bodies”, Astrophys. J., 204, 200–233, (1976).
|
|
36 |
Cantor, M., and Kulkarni, A.D., “Physical distinctions between normalized solutions of the
two-body problem of general relativity”, Phys. Rev. D, 25, 2521–2526, (1982).
|
|
37 |
Choquet-Bruhat, Y., and York, J.W., “The Cauchy problem”, in Held, A., ed., General
Relativity and Gravitation: One Hundred Years After the Birth of Albert Einstein, vol. 1, pp.
99–172, (Plenum, New York, 1980).
|
|
38 |
Cook, G.B., “Initial data for axisymmetric black-hole collisions”, Phys. Rev. D, 44, 2983–3000,
(1991).
|
|
39 |
Cook, G.B., “Three-dimensional initial data for the collision of two black holes. II. Quasicircular
orbits for equal-mass black holes”, Phys. Rev. D, 50, 5025–5032, (1994). [DOI], [ADS].
|
|
40 |
Cook, G.B., and Abrahams, A.M., “Horizon Structure of Initial-Data Sets for Axisymmetric
Two-Black-Hole Collisions”, Phys. Rev. D, 46, 702–713, (1992).
|
|
41 |
Cook, G.B., Choptuik, M.W., Dubal, M.R., Klasky, S.A., Matzner, R.A., and Oliveira, S.R.,
“Three-dimensional initial data for the collision of two black holes”, Phys. Rev. D, 47,
1471–1490, (1993).
|
|
42 |
Cook, G.B., and Scheel, M.A., “Well-behaved harmonic time slices of a charged, rotating,
boosted black hole”, Phys. Rev. D, 56, 4775–4781, (1997).
|
|
43 |
Cook, G.B., Shapiro, S.L., and Teukolsky, S.A., “Spin-up of a rapidly rotating star by angular
momentum loss: Effects of general relativity”, Astrophys. J., 398, 203–223, (1992).
|
|
44 |
Cook, G.B., Shapiro, S.L., and Teukolsky, S.A., “Rapidly rotating neutron stars in general
relativity: Realistic equations of state”, Astrophys. J., 424, 823–845, (1994). [DOI], [ADS].
|
|
45 |
Cook, G.B., Shapiro, S.L., and Teukolsky, S.A., “Rapidly rotating polytropes in general
relativity”, Astrophys. J., 422, 227–242, (1994).
|
|
46 |
Cook, G.B., Shapiro, S.L., and Teukolsky, S.A., “Testing a simplified version of Einstein’s
equations for numerical relativity”, Phys. Rev. D, 53, 5533–5540, (1996). [gr-qc/9512009].
|
|
47 |
Damour, T., Jaranowski, P., and Schäfer, G., “On the determination of the last stable orbit for
circular general relativistic binaries at the third post-Newtonian approximation”, Phys. Rev.
D, 62, 084011, 1–21, (2000). [ADS].
|
|
48 |
Doran, C., “A new form of the Kerr solution”, Phys. Rev. D, 61, 067503, 1–4, (2000).
[gr-qc/9910099].
|
|
49 |
Flanagan, É.É., “Possible Explanation for Star-Crushing Effect in Binary Neutron Star
Simulations”, Phys. Rev. Lett., 82, 1354–1357, (1999). [astro-ph/9811132].
|
|
50 |
Friedman, J.L., and Ipser, J.R., “Erratum: Rapidly rotating relativistic stars”, Philos. Trans.
R. Soc. London, Ser. A, 341(1662), 561, (1992).
|
|
51 |
Friedman, J.L., and Ipser, J.R., “Rapidly rotating relativistic stars”, Philos. Trans. R. Soc.
London, Ser. A, 340(1658), 391–422, (1992).
|
|
52 |
Friedman, J.L., Ipser, J.R., and Parker, L., “Rapidly rotating neutron star models”, Astrophys.
J., 304, 115–139, (1986).
|
|
53 |
Friedman, J.L., Ipser, J.R., and Sorkin, R.D., “Turning-point method for axisymmetric stability
of rotating relativistic stars”, Astrophys. J., 325, 722–274, (1988).
|
|
54 |
Garat, A., and Price, R.H., “Nonexistence of conformally flat slices of the Kerr spacetime”,
Phys. Rev. D, 61, 124011, 1–4, (2000). [gr-qc/0002013].
|
|
55 |
Gourgoulhon, E., “Relations between three formalisms for irrotational binary neutron stars in
general relativity”, arXiv e-print, (1998). [gr-qc/9804054].
|
|
56 |
Gourgoulhon, E., and Bonazzola, S., “Noncircular axisymmetric stationary spacetimes”, Phys.
Rev. D, 48, 2635–2652, (1993).
|
|
57 |
Gourgoulhon, E., Grandclément, P., Taniguchi, K., Marck, J.-A., and Bonazzola, S.,
“Quasiequilibrium sequences of synchronized and irrotational binary neutron stars in general
relativity: Method and tests”, Phys. Rev. D, 63, 064029, 1–27, (2001). [DOI], [ADS],
[gr-qc/0007028].
|
|
58 |
Grandclément, P., Bonazzola, S., Gourgoulhon, E., and Marck, J.-A., “A Multidomain
Spectral Method for Scalar and Vectorial Poisson Equations with Noncompact Sources”, J.
Comput. Phys., 170, 231–260, (2001). [DOI], [ADS], [gr-qc/0003072].
|
|
59 |
Gullstrand, A., “Allgemeine Lösung des statischen Einkörperproblems in der Einsteinschen
Gravitationstheorie”, Ark. Mat. Astron. Fys., 16, 1–15, (1922).
|
|
60 |
Hough, J., and Rowan, S., “Gravitational Wave Detection by Interferometry (Ground and
Space)”, Living Rev. Relativity, 3, lrr-2000-3, (2000). URL (cited on 31 October 2000):
http://www.livingreviews.org/lrr-2000-3.
|
|
61 |
Kley, W., and Schäfer, G., “Relativistic dust disks and the Wilson–Mathews approach”, Phys.
Rev. D, 60, 027501, 1–4, (1999). [gr-qc/9812068].
|
|
62 |
Kochanek, C.S., “Coalescing Binary Neutron Stars”, Astrophys. J., 398, 234–247, (1992).
|
|
63 |
Komatsu, H., Eriguchi, Y., and Hachisu, I., “Rapidly rotating general relativistic stars – I.
Numerical method and its application to uniformly rotating polytropes”, Mon. Not. R. Astron.
Soc., 237, 355–379, (1989).
|
|
64 |
Komatsu, H., Eriguchi, Y., and Hachisu, I., “Rapidly rotating general relativistic stars – II.
Differentially rotating polytropes”, Mon. Not. R. Astron. Soc., 239, 153–171, (1989).
|
|
65 |
Kraus, P., and Wilczek, F., “Some applications of a simple stationary line element for the
Schwarzschild geometry”, Mod. Phys. Lett. A, 9, 3713–3719, (1994). [gr-qc/9406042].
|
|
66 |
Kulkarni, A.D., “Time-asymmetric initial data for the N black hole problem in general
relativity”, J. Math. Phys., 25, 1028–1034, (1984).
|
|
67 |
Kulkarni, A.D., Shepley, L.C., and York Jr, J.W., “Initial data for N black holes”, Phys. Lett.
A, 96, 228–230, (1983).
|
|
68 |
Lake, K., “A Class of Quasi-Stationary Regular Line Elements for the Schwarzschild
Geometry”, arXiv e-print, (1994). [gr-qc/9407005].
|
|
69 |
Lichnerowicz, A., “L’integration des équations de la gravitation relativiste et le problème
des n corps”, J. Math. Pures Appl., 23, 37–63, (1944).
|
|
70 |
Lindquist, R.W., “Initial-Value Problem on Einstein-Rosen Manifolds”, J. Math. Phys., 4,
938–950, (1963). [DOI], [ADS].
|
|
71 |
Lousto, C.O., and Price, R.H., “Improved initial data for black hole collisions”, Phys. Rev. D,
57, 1073–1083, (1998). [gr-qc/9708022].
|
|
72 |
Marronetti, P., Mathews, G.J., and Wilson, J.R., “Binary neutron-star systems: From
the Newtonian regime to the last stable orbit”, Phys. Rev. D, 58, 107503, 1–4, (1998).
[gr-qc/9803093].
|
|
73 |
Marronetti, P., Mathews, G.J., and Wilson, J.R., “Irrotational binary neutron stars in
quasiequilibrium”, Phys. Rev. D, 60, 087301, 1–4, (1999). [gr-qc/9906088].
|
|
74 |
Marsa, R.L., and Choptuik, M.W., “Black-hole-scalar-field interactions in spherical symmetry”,
Phys. Rev. D, 54, 4929–4943, (1996). [DOI], [ADS], [gr-qc/9607034].
|
|
75 |
Martel, K., and Poisson, E., “Regular coordinate systems for Schwarzschild and other spherical
spacetimes”, Am. J. Phys., 69, 476–480, (2001). [gr-qc/0001069].
|
|
76 |
Mathews, G.J., Marronetti, P., and Wilson, J.R., “Relativistic hydrodynamics in close
binary systems: Analysis of neutron-star collapse”, Phys. Rev. D, 58, 043003, 1–13, (1998).
[gr-qc/9710140].
|
|
77 |
Mathews, G.J., and Wilson, J.R., “Revised relativistic hydrodynamical model for neutron-star
binaries”, Phys. Rev. D, 61, 127304, 1–4, (2000). [gr-qc/9911047].
|
|
78 |
Matzner, R.A., Huq, M.F., and Shoemaker, D., “Initial Data and Coordinates for Multiple
Black Hole Systems”, Phys. Rev. D, 59, 024015, 1–6, (1999). [gr-qc/9805023].
|
|
79 |
Misner, C.W., “The Method of Images in Geometrostatics”, Ann. Phys. (N.Y.), 24, 102–117,
(1963). [DOI], [ADS].
|
|
80 |
Misner, C.W., Thorne, K.S., and Wheeler, J.A., Gravitation, (W.H. Freeman, San Francisco,
1973).
|
|
81 |
Ó Murchadha, N., and York Jr, J.W., “Existence and uniqueness of solutions of the
Hamiltonian constraint of general relativity on compact manifolds”, J. Math. Phys., 14,
1551–1557, (1973).
|
|
82 |
Ó Murchadha, N., and York Jr, J.W., “Initial-value problem of general relativity. I. General
formulation and physical interpretation”, Phys. Rev. D, 10, 428–436, (1974).
|
|
83 |
Ó Murchadha, N., and York Jr, J.W., “Initial-value problem of general relativity. II. Stability
of solution of the initial-value equations”, Phys. Rev. D, 10, 437–446, (1974).
|
|
84 |
Ó Murchadha, N., and York Jr, J.W., “Gravitational Potentials: A Constructive Approach
to General Relativity”, Gen. Relativ. Gravit., 7, 257–261, (1976).
|
|
85 |
Oppenheimer, J.R., and Volkoff, G.M., “On Massive Neutron Cores”, Phys. Rev., 55, 374–381,
(1939).
|
|
86 |
Painlevé, P., “La mécanique classique et la theorie de la relativité”, C. R. Acad. Sci., 173,
677–680, (1921).
|
|
87 |
Pfeiffer, H.P., Teukolsky, S.A., and Cook, G.B., “Quasi-circular orbits for spinning binary black
holes”, Phys. Rev. D, 62, 104018, 1–11, (2000). [DOI], [ADS], [gr-qc/0006084].
|
|
88 |
Rieth, R., “On the validity of Wilson’s approach to general relativity”, in Królak, A.,
ed., Mathematics of Gravitation. Part II: Gravitational Wave Detection, Proceedings of the
Workshop on Mathematical Aspects of Theories of Gravitation, held in Warsaw, February 29 -
March 30, 1996, Banach Center Publications, vol. 41, pp. 71–74, (Polish Academy of Sciences,
Institute of Mathematics, Warsaw, Poland, 1997).
|
|
89 |
Robertson, H.P., and Noonan, T.W., Relativity and Cosmology, (Saunders, Philadelphia, 1968).
|
|
90 |
Shapiro, S.L., and Teukolsky, S.A., “Gravitational Collapse to Neutron Stars and Black Holes:
Computer Generation of Spherical Spacetimes”, Astrophys. J., 235, 199–215, (1980). [ADS].
|
|
91 |
Shapiro, S.L., and Teukolsky, S.A., “Gravitational collapse of rotating spheroids and the
formation of naked singularities”, Phys. Rev. D, 45, 2006–2012, (1992).
|
|
92 |
Shibata, M., “A relativistic formalism for computation of irrotational binary stars in
quasiequilibrium states”, Phys. Rev. D, 58, 024012, 1–5, (1998). [gr-qc/9803085].
|
|
93 |
Smarr, L.L., Čadež, A., DeWitt, B., and Eppley, K., “Collision of two black holes: Theoretical
framework”, Phys. Rev. D, 14, 2443–2452, (1976).
|
|
94 |
Smarr, L.L., and York Jr, J.W., “Kinematical conditions in the construction of spacetime”,
Phys. Rev. D, 17, 2529–2551, (1978). [DOI].
|
|
95 |
Sorkin, R.D., “A Criterion for the Onset of Instability at a Turning Point”, Astrophys. J., 249,
254–257, (1981). [DOI], [ADS].
|
|
96 |
Sorkin, R.D., “A Stability Criterion for Many-Parameter Equilibrium Families”, Astrophys. J.,
257, 847–854, (1982).
|
|
97 |
Stergioulas, N., “Rotating Stars in Relativity”, Living Rev. Relativity, 1, lrr-1998-8, (1998).
URL (cited on 18 July 2000):
http://www.livingreviews.org/lrr-1998-8.
|
|
98 |
Stergioulas, N., and Friedman, J.L., “Comparing models of rapidly rotating relativistic
stars constructed by two numerical methods”, Astrophys. J., 444, 306–311, (1995).
[astro-ph/9411032].
|
|
99 |
Teukolsky, S.A., “Irrotational Binary Neutron Stars in Quasiequilibrium in General Relativity”,
Astrophys. J., 504, 442–449, (1998). [gr-qc/9803082].
|
|
100 |
Thornburg, J., “Coordinates and boundary conditions for the general relativistic initial data
problem”, Class. Quantum Grav., 4, 1119–1131, (1987).
|
|
101 |
Uryū, K., and Eriguchi, Y., “New numerical method for constructing quasiequilibrium
sequences of irrotational binary neutron stars in general relativity.”, Phys. Rev. D, 61, 124023,
1–19, (2000). [DOI], [ADS], [gr-qc/9908059].
|
|
102 |
Uryū, K., Shibata, M., and Eriguchi, Y., “Properties of general relativistic, irrotational binary
neutron stars in close quasiequilibrium orbits: Polytropic equations of state”, Phys. Rev. D,
62, 104015, 1–15, (2000). [gr-qc/0007042].
|
|
103 |
Wilson, J.R., “Models of Differentially Rotating Stars”, Astrophys. J., 176, 195–204, (1972).
|
|
104 |
Wilson, J.R., and Mathews, G.J., “Relativistic hydrodynamics”, in Evans, C.R., Finn, L.S.,
and Hobill, D.W., eds., Frontiers in Numerical Relativity, Proceedings of the International
Workshop on Numerical Relativity, University of Illinois at Urbana-Champaign, USA, 9 – 13
May 1988, pp. 306–314, (Cambridge University Press, Cambridge; New York, 1989).
|
|
105 |
Wilson, J.R., and Mathews, G.J., “Instabilities in Close Neutron Star Binaries”, Phys. Rev.
Lett., 75, 4161–4164, (1995).
|
|
106 |
Wilson, J.R., Mathews, G.J., and Marronetti, P., “Relativistic numerical model for close
neutron-star binaries”, Phys. Rev. D, 54, 1317–1331, (1996). [DOI], [ADS], [gr-qc/9601017].
|
|
107 |
York Jr, J.W., “Gravitational Degrees of Freedom and the Initial-Value Problem”, Phys. Rev.
Lett., 26, 1656–1658, (1971).
|
|
108 |
York Jr, J.W., “Role of Conformal Three-Geometry in the Dynamics of Gravitation”, Phys.
Rev. Lett., 28, 1082–1085, (1972). [DOI].
|
|
109 |
York Jr, J.W., “Conformally invariant orthogonal decomposition of symmetric tensors on
Riemannian manifolds and the initial-value problem of general relativity”, J. Math. Phys., 14,
456–464, (1973).
|
|
110 |
York Jr, J.W., “Covariant decompositions of symmetric tensors in the theory of gravitation”,
Ann. Inst. Henri Poincare A, 21, 319–332, (1974).
|
|
111 |
York Jr, J.W., “Kinematics and Dynamics of General Relativity”, in Smarr, L.L., ed., Sources
of Gravitational Radiation, Proceedings of the Battelle Seattle Workshop, July 24 – August 4,
1978, pp. 83–126, (Cambridge University Press, Cambridge; New York, 1979). [ADS].
|
|
112 |
York Jr, J.W., “Energy and Momentum of the Gravitational Field”, in Tipler, F.J., ed., Essays
in General Relativity: A Festschrift for Abraham Taub, pp. 39–58, (Academic Press, New York,
1980).
|
|
113 |
York Jr, J.W., “Initial data for N black holes”, Physica A, 124, 629–637, (1984).
|
|
114 |
York Jr, J.W., “Initial Data for Collisions of Black Holes and Other Gravitational Miscellany”,
in Evans, C.R., Finn, L.S., and Hobill, D.W., eds., Frontiers in Numerical Relativity,
Proceedings of the International Workshop on Numerical Relativity, University of Illinois
at Urbana-Champaign, U.S.A., May 9 – 13, 1988, pp. 89–109, (Cambridge University Press,
Cambridge; New York, 1989).
|
|
115 |
York Jr, J.W., “Conformal ‘Thin-Sandwich’ Data for the Initial-Value Problem of General
Relativity”, Phys. Rev. Lett., 82, 1350–1353, (1999). [gr-qc/9810051].
|
|
116 |
York Jr, J.W., and Piran, T., “The Initial Value Problem and Beyond”, in Matzner, R.A.,
and Shepley, L.C., eds., Spacetime and Geometry: The Alfred Schild Lectures, pp. 147–176,
(University of Texas Press, Austin, 1982).
|