Research output: Contribution to journal › Article › peer-review
Graviatom of Superheavy Dark Matter as a Source of Gravitational Radiation. / Misyura, M. A.
In: Gravitation and Cosmology, Vol. 24, No. 3, 01.07.2018, p. 289-291.Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - Graviatom of Superheavy Dark Matter as a Source of Gravitational Radiation
AU - Misyura, M. A.
PY - 2018/7/1
Y1 - 2018/7/1
N2 - The nature of dark matter (DM) in modern physics is an important problem. We consider a quantum system consisting of two identical particles which are candidates for the role of DM.We call them graviatoms, and they could be formed in the early Universe. We find the energy spectrum of the gravitatom from DM particles, the Bohr radius, the intensity and frequency of gravitational radiation, and the lifetime of a state. This lifetime is large for superheavy particles. Estimates of these values for different masses of DM particles are given. The amplitude of a gravitational wave from a cloud of dark matter in the Milky Way is also estimated.
AB - The nature of dark matter (DM) in modern physics is an important problem. We consider a quantum system consisting of two identical particles which are candidates for the role of DM.We call them graviatoms, and they could be formed in the early Universe. We find the energy spectrum of the gravitatom from DM particles, the Bohr radius, the intensity and frequency of gravitational radiation, and the lifetime of a state. This lifetime is large for superheavy particles. Estimates of these values for different masses of DM particles are given. The amplitude of a gravitational wave from a cloud of dark matter in the Milky Way is also estimated.
UR - http://www.scopus.com/inward/record.url?scp=85052133373&partnerID=8YFLogxK
U2 - 10.1134/S0202289318030118
DO - 10.1134/S0202289318030118
M3 - Article
AN - SCOPUS:85052133373
VL - 24
SP - 289
EP - 291
JO - Gravitation and Cosmology
JF - Gravitation and Cosmology
SN - 0202-2893
IS - 3
ER -
ID: 49588377