Astronomy and Astrophysics – Astronomy
Scientific paper
May 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..254..101a&link_type=abstract
In: Testing the AGN paradigm; Proceedings of the 2nd Annual Topical Astrophysics Conference, Univ. of Maryland, College Park, Oc
Astronomy and Astrophysics
Astronomy
Active Galactic Nuclei, Black Holes (Astronomy), Gravitational Collapse, Relativistic Particles, Schwarzschild Metric, Spectral Energy Distribution, Energy Sources, Neutron Stars, Stellar Evolution, Stellar Mass
Scientific paper
It is proposed that the source of AGN is the decay of the energy of strong black holes (SBHs) via a Hawking-like mechanism leading to pion emission (at ordinary matter densities) or to baryons only at much higher energy densities (or hot spots) needed to collapse the matter into its strong Schwarzschild radius. The decay of these hadrons into leptons constitutes the secondary emission responsible for the whole spectrum - radio to X-ray - that is observed in many AGN. The decaying hadrons are associated with SBH solutions of a unified theory of strong and gravitational interactions and to their possible evaporation.
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