Gravitational Radiation from Minihole Coalescence and Quadrupole Transitions of Hydrogen-Like Atoms

The minihole coalescences and quadrupole transitions of hydrogen atoms and hydrogen-like graviatoms are considered to be sources of the gravitational background radiation. The total energies of the gravitational radiation of these microsystems have been calculated. This gravitational background proves to be comparable with the observed gravitational radiation from the coalescence of stellar mass black holes. © Published under licence by IOP Publishing Ltd.

Conference proceedings
Publisher
Institute of Physics Publishing
Number of issue
1
Language
English
Status
Published
Number
012018
Volume
1557
Year
2020
Organizations
  • 1 Peoples' Friendship University of Russia, Moscow, Russian Federation
Keywords
Atoms; Coalescence; Hydrogen; Radiation; Relativity; Stars; Background radiation; Gravitational radiation; Hydrogen atoms; Hydrogen-like atoms; Quadrupole transition; Stellar-mass black holes; Total energy; Gravitation
Date of creation
02.11.2020
Date of change
02.11.2020
Short link
https://repository.rudn.ru/en/records/article/record/64637/
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