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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

Harvard

Misyura, MA 2018, 'Graviatom of Superheavy Dark Matter as a Source of Gravitational Radiation', Gravitation and Cosmology, vol. 24, no. 3, pp. 289-291. https://doi.org/10.1134/S0202289318030118

APA

Misyura, M. A. (2018). Graviatom of Superheavy Dark Matter as a Source of Gravitational Radiation. Gravitation and Cosmology, 24(3), 289-291. https://doi.org/10.1134/S0202289318030118

Vancouver

Misyura MA. Graviatom of Superheavy Dark Matter as a Source of Gravitational Radiation. Gravitation and Cosmology. 2018 Jul 1;24(3):289-291. https://doi.org/10.1134/S0202289318030118

Author

Misyura, M. A. / Graviatom of Superheavy Dark Matter as a Source of Gravitational Radiation. In: Gravitation and Cosmology. 2018 ; Vol. 24, No. 3. pp. 289-291.

BibTeX

@article{d15c71da61b240919a368612f070493a,
title = "Graviatom of Superheavy Dark Matter as a Source of Gravitational Radiation",
abstract = "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.",
author = "Misyura, {M. A.}",
year = "2018",
month = jul,
day = "1",
doi = "10.1134/S0202289318030118",
language = "English",
volume = "24",
pages = "289--291",
journal = "Gravitation and Cosmology",
issn = "0202-2893",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "3",

}

RIS

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