Supermassive neutrino stars and galactic nuclei

Details Supermassive neutrino stars and galactic nuclei Supermassive neutrino stars and galactic nuclei

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993phlb..306...79v&link_type=abstract

Physics Letters B, Volume 306, Issue 1-2, p. 79-85.

Physics

36

Scientific paper

The characteristics of supermassive `stars' consisting of self-gravitating degenerate neutrino (or neutralino) matter are studied with particular emphasis on fermion masses around 17 keV/c2. Such compact dark objects could be as massive as 109.5 to 1o6.5 solar masses, with radii of about one to ten light days; they might thus mimic phenomena that are expected around the supermassive black holes recently purported at the centres of some galaxies and quasi-stellar objects.
Present address: Institute of Theoretical Nuclear Physics, University of Stellenbosch, Stellenbosch 7600, South Africa.

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