Neutrino emission from collapsed objects

Details Neutrino emission from collapsed objects Neutrino emission from collapsed objects

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ncimc...9..435t&link_type=abstract

(Symposium on Underground Physics, 1st, Saint Vincent, Italy, Apr. 25-28, 1985) Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol.

Astronomy and Astrophysics

Astronomy

2

Accretion Disks, Black Holes (Astronomy), Cosmic Rays, Galactic Nuclei, Gamma Ray Astronomy, Gravitational Collapse, Neutrinos, Quasars, Background Radiation, Energy Spectra, High Energy Interactions, Milky Way Galaxy, Particle Flux Density, Particle Production, Schwarzschild Metric, Stellar Mass Accretion

Scientific paper

The possible emission fluxes from matter spherically accreting onto a massive object (Schwarzschild black hole) are discussed. Assuming that the observed high-energy gamma-rays from point sources have hadronic origin, the expected neutrino flux from the quasar 3C 273 and from the galactic center is evaluated. The accretion process onto a massive object is found to produce neutrinos in the low-energy region (15 MeV).

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