Quantum mechanism of extremely high energy processes at neutron star collapse and of quasar luminosity
arXiv:2111.01530 · doi:10.1007/JHEP03(2022)002
Abstract
Using the braid group topological approach to quantum statistics we demonstrate that for strong gravitational field occurring in neutron star merger with mass exceeding the Tolman, Oppenheimer and Volkoff limit the quantum statistics of particles beneath the photon sphere decays, which results in an instant relief of quantum degeneracy pressure in the star. This causes a rapid shrink of the matter to a black hole with quite different quantum collective character of particles. The scheme of neutron Fermi sphere collapse is proposed as the possible isotropic source of short giant gamma-ray bursts. The similar quantum mechanism of collapse of Fermi spheres of electrons and protons in plasma of accretion disc in vicinity of the Schwarzschild horizon of galactic black hole is able to elucidate the giant luminosity of remote quasars. The efficiency of the mass to energy conversion via collapse of the Fermi sphere is ca. 30%, not reachable for any other known physical process except of the matter-antimatter annihilation.
arXiv commentarXiv admin note: text overlap with arXiv:2110.13651
References in corpus (10)
- Topological Insulators
- Constraining the Maximum Mass of Neutron Stars From Multi-Messenger Observations of GW170817
- Using gravitational-wave observations and quasi-universal relations to constrain the maximum mass of neutron stars
- The Maximum Mass of a Neutron Star
- On the interpretation of the multicolour disc model for black hole candidates
- Fractional Quantum Hall Effect of Composite Fermions
- Tunable Fractional Quantum Hall Phases in Bilayer Graphene
- Advection Dominated Accretion Flows Around Kerr Black Holes
- Lev Landau and the conception of neutron stars
- Application of path-integral quantization to indistinguishable particle systems topologically confined by a magnetic field