Artículo

El editor solo permite decargar el artículo en su versión post-print desde el repositorio. Por favor, si usted posee dicha versión, enviela a
Consulte el artículo en la página del editor
Consulte la política de Acceso Abierto del editor

Abstract:

We obtain an explicit solution of the momentum constraint for conformally flat, maximal slicing, initial data which gives an alternative to the purely longitudinal extrinsic curvature of Bowen and York. The new solution is related, in a precise form, with the extrinsic curvature of a Kerr slice. We study these new initial data representing spinning black holes by numerically solving the Hamiltonian constraint. They have the following features: (i) they contain less radiation, for all allowed values of the rotation parameter, than the corresponding single spinning Bowen-York black hole; (ii) the maximum rotation parameter J/m 2 reached by this solution is higher than that of the purely longitudinal solution, allowing us thus to describe holes closer to a maximally rotating Kerr one. We discuss the physical interpretation of these properties and their relation with the weak cosmic censorship conjecture. Finally, we generalize the data for multiple black holes using the "puncture" and isometric formulations. ©2002 The American Physical Society.

Registro:

Documento: Artículo
Título:New conformally flat initial data for spinning black holes
Autor:Dain, S.; Lousto, C.O.; Takahashi, R.
Filiación:Albert-Einstein Institut, Max-Planck Institut für Gravitationsphysik, Am Mühlenberg 1, D-14476 Golm, Germany
Department of Physics and Astronomy, University of Texas at Brownsville, Brownsville, TX 78520, United States
Instituto de Astronomía y Física del Espacio-CONICET, Buenos Aires, Argentina
Theoretical Astrophysics Center, Juliane Maries Vej 30, 2100 Copenhagen, Denmark
Palabras clave:accuracy; article; calculation; cosmos; energy; molecular evolution; physics; velocity
Año:2002
Volumen:65
Número:10
DOI: http://dx.doi.org/10.1103/PhysRevD.65.104038
Título revista:Physical Review D
Título revista abreviado:-
ISSN:05562821
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05562821_v65_n10_p_Dain

Referencias:

  • Penrose, R., (1969) Riv. Nuovo Cimento, 1, p. 252
  • Wald, R., (1999) Fundamental Theories of Physics, pp. 69-85. , Black Holes, Gravitational Radiation and the Universe, edited by B. R. Iyer and B. Bhawal (Kluwer Academic, Dordrecht)
  • Christodoulou, D., (1999) Ann. Math., 149, p. 183
  • Hawking, S.W., Ellis, G.F.R., (1973) The Large Scale Structure of Space-time, , Cambridge University Press, Cambridge, England
  • Wald, R.M., (1984) General Relativity, , The University of Chicago Press, Chicago
  • Penrose, R., (1973) Ann. N.Y. Acad. Sci., 224, p. 125
  • G. Huisken and T. Ilmanen, J. Diff. Geometry (to be pub lished); H.L. Bray, math.DG/9911173; Komar, A., (1959) Phys. Rev., 119, p. 934
  • Hawking, S.W., (1972) Commun. Math. Phys., 25, p. 152
  • York Jr., J.W., Piran, T., (1982) Spacetime and Geometry: The Alfred Schild Lectures, pp. 147-176. , edited by R. A. Matzner and L. C. Shepley (University of Texas Press, Austin, Texas)
  • Choptuik, M.W., Unruh, W.O., (1986) Gen. Relativ. Gravit., 18, p. 818
  • Cook, G., York, J.W., (1990) Phys. Rev. D, 41, p. 1077
  • Cook, G.B., (1991) Phys. Rev. D, 44, p. 2983
  • Bowen, J.M., York Jr., J.W., (1980) Phys. Rev. D, 21, p. 2047
  • Garat, A., Price, R., (2000) Phys. Rev. D, 61, p. 124011
  • Dain, S., Friedrich, H., (2001) Commun. Math. Phys., 222, p. 569
  • Baker, J., Brügmann, B., Campanelli, M., Lousto, C.O., Takahashi, R., (2001) Phys. Rev. Lett., 87, p. 121103
  • Dain, S., (2001) Phys. Rev. Lett., 87, p. 121102
  • Dain, S., (2001) Phys. Rev. D, 64, p. 124002
  • Bishop, N., Isaacson, R., Maharaj, M., Winicour, J., (1998) Phys. Rev. D, 57, p. 6113
  • Marronetti, P., Matzner, R.A., (2000) Phys. Rev. Lett., 85, p. 5500
  • Choquet-Bmhat, Y., Isenberg, J., York Jr., J.W., (2000) Phys. Rev. D, 61, p. 084034
  • Choquet-Bruhat, Y., York Jr., J.W., (1980) General Relativity and Gravitation, 1, pp. 99-172. , edited by A. Held (Plenum, New York)
  • Brandt, S., Seidel, E., (1996) Phys. Rev. D, 54, p. 1403
  • Baker, J., Puzio, R., (1999) Phys. Rev. D, 59, p. 044030
  • Brill, D., (1959) Ann. Phys. (Leipzig), 7, p. 466
  • Cantor, M., Brill, D., (1981) Compos. Math., 43, p. 317
  • Friedrich, H., (1988) Commun. Math. Phys., 119, p. 51
  • Beig, R., (1991) Class. Quantum Grav., 8, pp. L205
  • Brandt, S., Brügmann, B., (1997) Phys. Rev. Lett., 78, p. 3606
  • Brandt, S., Seidel, E., (1995) Phys. Rev. D, 52, p. 856

Citas:

---------- APA ----------
Dain, S., Lousto, C.O. & Takahashi, R. (2002) . New conformally flat initial data for spinning black holes. Physical Review D, 65(10).
http://dx.doi.org/10.1103/PhysRevD.65.104038
---------- CHICAGO ----------
Dain, S., Lousto, C.O., Takahashi, R. "New conformally flat initial data for spinning black holes" . Physical Review D 65, no. 10 (2002).
http://dx.doi.org/10.1103/PhysRevD.65.104038
---------- MLA ----------
Dain, S., Lousto, C.O., Takahashi, R. "New conformally flat initial data for spinning black holes" . Physical Review D, vol. 65, no. 10, 2002.
http://dx.doi.org/10.1103/PhysRevD.65.104038
---------- VANCOUVER ----------
Dain, S., Lousto, C.O., Takahashi, R. New conformally flat initial data for spinning black holes. -. 2002;65(10).
http://dx.doi.org/10.1103/PhysRevD.65.104038