Luminosity Limit of Super-Eddington Accretion onto Black Holes

Details Luminosity Limit of Super-Eddington Accretion onto Black Holes Luminosity Limit of Super-Eddington Accretion onto Black Holes

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999chphl..16..467w&link_type=abstract

Chinese Physics Letters, Volume 16, Issue 6, pp. 467-468 (1999).

Physics

2

Scientific paper

The luminosity limit is derived for the super-Eddington accretion by obtaining the self-similar solution. The maximum luminosity is about 4.0 × 1037 erg/s(M/Modot) or so (significantly less than the Eddington luminosity) due to photon trapping although the accretion rate is super-Eddington. The radiation spectrum is found to be universal as Fν ~ ν-1.

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