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arxiv: astro-ph/9812135 · v1 · submitted 1998-12-08 · 🌌 astro-ph

On the Nature of the Compact Objects in the AGNs

classification 🌌 astro-ph
keywords smssagnsblackcompacthighlyholesluminositymassive
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If the cores of Galaxies and AGNs comprise Supermassive Stars (SMSs) (Hoyle and Fowler 1963), nuclear energy generation may not be ignited for masses $M > 6\times 10^4 M_\odot$, and highly supermassive stars are likely to generate their luminosity, $L_{KH}$ slow gravitational contraction. We show that for such massive Newtonian SMSs, both the value of $L_{KH}$ and the the accretion luminosity, $L_{acc}$, could be much less than the appropriate Eddington value. Such highly SMSs will have a surface density as low as $10^{-14}$ g/cm$^3$ and they will not behave like a compact object with a ``hard surface'. For all such reasons, it is indeed possible to have $L_{SMS} \ll L_{ed}$. 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).

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