Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977svphu.121q.319r&link_type=abstract
Uspekhi Fizicheskikh Nauk, vol. 121, Feb. 1977, p. 319-329. In Russian.
Astronomy and Astrophysics
Astronomy
Black Holes (Astronomy), Neutron Stars, Quantum Mechanics, Stellar Evolution, White Dwarf Stars, Cosmology, Elementary Particles, Stellar Gravitation, Stellar Mass, Stellar Models
Scientific paper
An attempt is made to develop the analog of a quantum-mechanical approach to the physics of stellar objects (main-sequence stars, red dwarfs, white dwarfs, neutron stars, black holes) and relate the parameters of elementary particles and those of large masses of gas radiating in their own gravitational field. Mass, radius, and density of stars are taken as basic parameters, and the duration, radiation, and position on the HR diagram of stars are taken as basic observables. Attention is given to the inevitable aging and collapse of stars, nonnegligible radiation by black holes, and radiation by a particle-antiparticle pair in vacuum in a gravitational field. An empirical numerical sequence relating nucleon mass and universal fundamental constants (gravitational constant, Planck's constant, speed of light, proton mass) is advanced, and some cosmic 'magic' numbers are proposed.
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