paper

On the Nature of the Compact Objects in the AGNs

arXiv:astro-ph/9812135

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 , and highly supermassive stars are likely to generate their luminosity, slow gravitational contraction. We show that for such massive Newtonian SMSs, both the value of and the the accretion luminosity, , could be much less than the appropriate Eddington value. Such highly SMSs will have a surface density as low as g/cm and they will not behave like a compact object with a ``hard surface'. For all such reasons, it is indeed possible to have . 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).

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