English

On the Nature of the Compact Objects in the AGNs

Astrophysics 2007-05-23 v1

Abstract

If the cores of Galaxies and AGNs comprise Supermassive Stars (SMSs) (Hoyle and Fowler 1963), nuclear energy generation may not be ignited for masses M>6×104MM > 6\times 10^4 M_\odot, and highly supermassive stars are likely to generate their luminosity, LKHL_{KH} slow gravitational contraction. We show that for such massive Newtonian SMSs, both the value of LKHL_{KH} and the the accretion luminosity, LaccL_{acc}, could be much less than the appropriate Eddington value. Such highly SMSs will have a surface density as low as 101410^{-14} g/cm3^3 and they will not behave like a compact object with a ``hard surface'. For all such reasons, it is indeed possible to have LSMSLedL_{SMS} \ll L_{ed}. And this effect may be incorrectly interpreted as the evidence for the existence of central Super Massive Black Holes with Event Horizons. In fact, in a very detailed work, and from various angles, we have recently shown that, the General Theory of Relativity does not permit the occurrenes of ``trapped surfaces'' and Black Holes (Mitra 1998a, gr-qc/9810038).

Keywords

Cite

@article{arxiv.astro-ph/9812135,
  title  = {On the Nature of the Compact Objects in the AGNs},
  author = {Abhas Mitra},
  journal= {arXiv preprint arXiv:astro-ph/9812135},
  year   = {2007}
}

Comments

Preliminary draft of paper to be presented in the 19th Texas Symp, 4 pages, additional e-address: [email protected]