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Null geodesic expansion in spherical gravitational collapse

T. P. Singh*

  • Theoretical Astrophysics Group, Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400 005, India

  • *Email address: tpsingh@tifrvax.tifr.res.in

Phys. Rev. D 58, 024004 – Published 8 June, 1998

DOI: https://doi.org/10.1103/PhysRevD.58.024004

Abstract

We derive an expression for the expansion of outgoing null geodesics in spherical dust collapse and compute the limiting value of the expansion in the approach to singularity formation. An analogous expression is derived for the spherical collapse of a general form of matter. We argue on the basis of these results that the covered as well as the naked singularity solutions arising in spherical dust collapse are stable under small changes in the equation of state.

References (4)

  1. For a general account of the Tolman-Bondi metric, see, e.g., L. D. Landau and E. M. Lifshitz,  Classical Theory of Fields, 4th ed. (Pergamon, New York, 1975), Secs. 100 and 103.
  2. D. M. Eardley and L. Smarr, Phys. Rev. D 19, 2239 (1979); D. Christodoulou, Commun. Math. Phys. 93, 171 (1984); R. P. A. C. Newman, Class. Quantum Grav. 3, 527 (1986); ibid.I. H. Dwivedi and P. S. Joshi, 9, L69 (1992); P. S. Joshi and I. H. Dwivedi, Phys. Rev. D 47, 5357 (1993).
  3. T. P. Singh and P. S. Joshi, Class. Quantum Grav. 13, 559 (1996).
  4. I. H. Dwivedi and P. S. Joshi, Commun. Math. Phys. 166, 117 (1994).

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