Radiation pressure supported stars in Einstein gravity: eternally collapsing objects

@article{Mitra2006RadiationPS,
  title={Radiation pressure supported stars in Einstein gravity: eternally collapsing objects},
  author={A. Mitra},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2006},
  volume={369},
  pages={492-496}
}
  • A. Mitra
  • Published 2006
  • Physics
  • Monthly Notices of the Royal Astronomical Society
  • Even when we consider Newtonian stars, that is, stars with surface gravitational redshift z « 1, it is well known that, theoretically, it is possible to have stars supported against self-gravity almost entirely by radiation pressure. However, such Newtonian stars must necessarily be supermassive. We point out that this requirement for excessively large M in the Newtonian case is a consequence of the occurrence of low z « 1. However, if we remove such restrictions, and allow for the possible… CONTINUE READING
    27 Citations
    Masses of radiation pressure supported stars in extreme relativistic realm
    • 1
    • Highly Influenced
    • PDF
    The fallacy of Oppenheimer Snyder collapse: no general relativistic collapse at all, no black hole, no physical singularity
    • 20
    • Highly Influenced
    • PDF

    References

    SHOWING 1-10 OF 11 REFERENCES
    A generic relation between baryonic and radiative energy densities of stars
    • 17
    • PDF
    NON-OCCURRENCE OF TRAPPED SURFACES AND BLACK HOLES IN SPHERICAL GRAVITATIONAL COLLAPSE
    • 30
    • PDF
    On the final state of spherical gravitational collapse
    • 21
    • PDF
    The gravitational field of a radiating star
    • 417
    An Introduction to the Study of Stellar Structure
    • 1,324
    Dynamics of dissipative gravitational collapse
    • 114
    • PDF
    Gravitation and Cosmology: Principles and Applications of the General Theory of Relativity
    • 3,966
    • Highly Influential
    • PDF
    The stability of supermassive stars.
    • 90
    Les Méthodes nouvelles de la Mécanique céleste and An Introduction to the Study of Stellar Structure
    • 1,652
    • Highly Influential