The line profile of a relativistic Keplerian ring in a massive neutrino halo

Details The line profile of a relativistic Keplerian ring in a massive neutrino halo The line profile of a relativistic Keplerian ring in a massive neutrino halo

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984acaps...4..184d&link_type=abstract

(Acta Astrophysica Sinica, vol. 4, no. 2-3, 1984, p. 184-190) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 8, Dec.

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Astronomical Models, Computational Astrophysics, Halos, Kepler Laws, Neutrinos, Black Holes (Astronomy), Galactic Nuclei, Gravitational Fields, Mass Distribution

Scientific paper

If a massive neutrino halo transparent to light surrounds a compact body (galactic nucleus or black hole), then the strong gravitational field inside the halo will radically alter the spectral line profiles of a light-emitting Keplerian ring. This paper gives precise solutions of the spectral profile in a core-halo structure of matter and neutrino, and the result is compared with the no-halo case. The distribution of the neutrino mass is also given under typical circumstances.

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