The Mass of the Oppenheimer-Snyder Black Hole

@article{Mitra1999TheMO,
  title={The Mass of the Oppenheimer-Snyder Black Hole},
  author={A. Mitra},
  journal={arXiv: Astrophysics},
  year={1999}
}
  • A. Mitra
  • Published 1999
  • Physics
  • arXiv: Astrophysics
    • The only instance when the General Relativistic (GTR) collapse equations have been solved (almost) exactly to explicitly find the metric coefficients is the case of a homogeneous spherical dust (Oppenheimer and Snyder in 1939 in Phy. Rev. 56, 455). The equation (37) of their paper showed the formation of an event horizon for a collapsing homogeneous dust ball of mass M in that the circumference radius the outermost surface, r_b = r_0= 2M in a proper time proportional to r_0^{-1/2} in the limit… CONTINUE READING
    View PDF on arXiv
    12 Citations
    Background Citations
    3
    Methods Citations
    2
    Results Citations
    1
    12 Citations
    Citation Type

    Citation Type

    The fallacy of Oppenheimer Snyder collapse: no general relativistic collapse at all, no black hole, no physical singularity
    • 20
    • PDF
    Kruskal Coordinates and Mass of Schwarzschild Black Holes: No Finite Mass Black Hole at All
    • 14
    • PDF
    A Model of Dust-like Spherically Symmetric Gravitational Collapse without Event Horizon Formation
    • 2
    Modeling quasar central engine as a relativistic radiating star
    • 4
    A Model of Dustlike Spherically Symmetric Gravitational Collapse without Event Horizon Formation
    • 1
    • PDF
    Applications of Gravitational Model of Possible Final Unification in both Large & Small Scale Physics
    • 6
    Topology of Black Holes’ Horizons
    • PDF
    Horizon free eternally collapsing anisotropic radiating star
    • 15
    Topological Assessment of Entangled Particles on Black Hole Horizons
    • 1
    • PDF
    Entangled Antipodal Points on Black Hole Surfaces: the Borsuk-Ulam Theorem Comes Into Play
    • PDF