Quantum contribution to luminosity of quasars
Janusz E. Jacak

TL;DR
This paper explores a quantum physics mechanism involving fermion degeneracy and Pauli principle violations near black holes to explain the high luminosity of quasars, proposing a novel quantum contribution to their energy output.
Contribution
It introduces a new quantum statistical model involving Fermi spheres and Pauli principle revocation to explain quasar luminosity, extending traditional gravitational energy conversion theories.
Findings
Quantum effects of fermions near black holes could significantly enhance luminosity.
Collapse of Fermi spheres releases large amounts of energy as photons.
Proposes a quantum process supplementing gravitational energy conversion in quasars.
Abstract
The accretion of galactic gas is regarded as the source of the giant luminosity of quasars. The gravitational energy converts itself into radiation close to the Schwarzschild horizon of the central supermassive black hole with efficiency of ca. 30% mass to radiation energy conversion rate. Particularities of such an extremely effective mechanism of mass to energy conversion are, however, still obscure. We propose to take into account quantum statistics properties of fermions, which could emit in close outer vicinity of the Schwarzschild zone a giant energy accumulated in the Fermi spheres of electrons and protons in degenerate quantum collective state created in this region by the gravitational compression of plasma. The release of photons is possible due to the local revoking of Pauli exclusion principle constraint induced by the rapid change of the homotopy of multiparticle…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Relativity and Gravitational Theory
