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New Options for SUSY-Kind Dark Matter. / Arbuzova, Elena.

In: Moscow University Physics Bulletin, Vol. 77, No. 2, 04.2022, p. 288-290.

Research output: Contribution to journalArticlepeer-review

Harvard

Arbuzova, E 2022, 'New Options for SUSY-Kind Dark Matter', Moscow University Physics Bulletin, vol. 77, no. 2, pp. 288-290. https://doi.org/10.3103/S0027134922020084

APA

Arbuzova, E. (2022). New Options for SUSY-Kind Dark Matter. Moscow University Physics Bulletin, 77(2), 288-290. https://doi.org/10.3103/S0027134922020084

Vancouver

Arbuzova E. New Options for SUSY-Kind Dark Matter. Moscow University Physics Bulletin. 2022 Apr;77(2):288-290. doi: 10.3103/S0027134922020084

Author

Arbuzova, Elena. / New Options for SUSY-Kind Dark Matter. In: Moscow University Physics Bulletin. 2022 ; Vol. 77, No. 2. pp. 288-290.

BibTeX

@article{61f6406c8aee4863b5991cb52672f678,
title = "New Options for SUSY-Kind Dark Matter",
abstract = "In the conventional cosmology masses of the stable supersymmetric relics, candidates for the dark matter (DM) particles, should be typically below 1 TeV. This is in conflict with the LHC bounds on the low energy SUSY. However, in $$R^{2}$$-gravity the masses of the stable particles with the interaction strength typical for SUSY could be much higher depending upon the dominant decay mode of the scalaron. We discuss the bounds on the masses of DM particles for the following dominant decay modes: to minimally coupled massless scalars, to massive fermions, and to gauge bosons.",
keywords = "$R^{2}$-cosmology, dark matter, scalaron decay",
author = "Elena Arbuzova",
note = "Funding Information: The work was supported by the Russian Science Foundation, project no. 20-42-09010. Publisher Copyright: {\textcopyright} 2022, Allerton Press, Inc.",
year = "2022",
month = apr,
doi = "10.3103/S0027134922020084",
language = "English",
volume = "77",
pages = "288--290",
journal = "Moscow University Physics Bulletin (English Translation of Vestnik Moskovskogo Universiteta, Fizika)",
issn = "0027-1349",
publisher = "Allerton Press Inc.",
number = "2",

}

RIS

TY - JOUR

T1 - New Options for SUSY-Kind Dark Matter

AU - Arbuzova, Elena

N1 - Funding Information: The work was supported by the Russian Science Foundation, project no. 20-42-09010. Publisher Copyright: © 2022, Allerton Press, Inc.

PY - 2022/4

Y1 - 2022/4

N2 - In the conventional cosmology masses of the stable supersymmetric relics, candidates for the dark matter (DM) particles, should be typically below 1 TeV. This is in conflict with the LHC bounds on the low energy SUSY. However, in $$R^{2}$$-gravity the masses of the stable particles with the interaction strength typical for SUSY could be much higher depending upon the dominant decay mode of the scalaron. We discuss the bounds on the masses of DM particles for the following dominant decay modes: to minimally coupled massless scalars, to massive fermions, and to gauge bosons.

AB - In the conventional cosmology masses of the stable supersymmetric relics, candidates for the dark matter (DM) particles, should be typically below 1 TeV. This is in conflict with the LHC bounds on the low energy SUSY. However, in $$R^{2}$$-gravity the masses of the stable particles with the interaction strength typical for SUSY could be much higher depending upon the dominant decay mode of the scalaron. We discuss the bounds on the masses of DM particles for the following dominant decay modes: to minimally coupled massless scalars, to massive fermions, and to gauge bosons.

KW - $R^{2}$-cosmology

KW - dark matter

KW - scalaron decay

UR - http://www.scopus.com/inward/record.url?scp=85138275661&partnerID=8YFLogxK

UR - https://www.mendeley.com/catalogue/71224d3d-f71e-37db-964a-bdf947f04d51/

U2 - 10.3103/S0027134922020084

DO - 10.3103/S0027134922020084

M3 - Article

AN - SCOPUS:85138275661

VL - 77

SP - 288

EP - 290

JO - Moscow University Physics Bulletin (English Translation of Vestnik Moskovskogo Universiteta, Fizika)

JF - Moscow University Physics Bulletin (English Translation of Vestnik Moskovskogo Universiteta, Fizika)

SN - 0027-1349

IS - 2

ER -

ID: 38035377