Standard

Dark matter in R+R2 cosmology. / Arbuzova, E. V.; Dolgov, A. D.; Singh, R. S.

In: Journal of Cosmology and Astroparticle Physics, Vol. 2019, No. 4, 014, 08.04.2019.

Research output: Contribution to journal › Article › peer-review

Harvard

Arbuzova, EV, Dolgov, AD & Singh, RS 2019, 'Dark matter in R+R2 cosmology', Journal of Cosmology and Astroparticle Physics, vol. 2019, no. 4, 014. https://doi.org/10.1088/1475-7516/2019/04/014

APA

Arbuzova, E. V., Dolgov, A. D., & Singh, R. S. (2019). Dark matter in R+R2 cosmology. Journal of Cosmology and Astroparticle Physics, 2019(4), [014]. https://doi.org/10.1088/1475-7516/2019/04/014

Vancouver

Arbuzova EV, Dolgov AD, Singh RS. Dark matter in R+R2 cosmology. Journal of Cosmology and Astroparticle Physics. 2019 Apr 8;2019(4):014. doi: 10.1088/1475-7516/2019/04/014

Author

Arbuzova, E. V. ; Dolgov, A. D. ; Singh, R. S. / Dark matter in R+R2 cosmology. In: Journal of Cosmology and Astroparticle Physics. 2019 ; Vol. 2019, No. 4.

BibTeX

@article{e917c02f270b489bbed98c14beb84201,
title = "Dark matter in R+R2 cosmology",
abstract = "Production of massive stable relics in R2-modified gravity is considered. It is shown that the cosmological evolution and kinetics of massive species differs significantly from those in the conventional cosmology. The results are applied to the lightest supersymmetric particles and it is argued that they are viable candidates for the constituents of dark matter, if their mass is about 1000 TeV.",
keywords = "dark matter theory, modified gravity, particle physics - cosmology connection, physics of the early universe, MOTION",
author = "Arbuzova, {E. V.} and Dolgov, {A. D.} and Singh, {R. S.}",
year = "2019",
month = apr,
day = "8",
doi = "10.1088/1475-7516/2019/04/014",
language = "English",
volume = "2019",
journal = "Journal of Cosmology and Astroparticle Physics",
issn = "1475-7516",
publisher = "IOP Publishing Ltd.",
number = "4",

}

RIS

TY - JOUR

T1 - Dark matter in R+R2 cosmology

AU - Arbuzova, E. V.

AU - Dolgov, A. D.

AU - Singh, R. S.

PY - 2019/4/8

Y1 - 2019/4/8

N2 - Production of massive stable relics in R2-modified gravity is considered. It is shown that the cosmological evolution and kinetics of massive species differs significantly from those in the conventional cosmology. The results are applied to the lightest supersymmetric particles and it is argued that they are viable candidates for the constituents of dark matter, if their mass is about 1000 TeV.

AB - Production of massive stable relics in R2-modified gravity is considered. It is shown that the cosmological evolution and kinetics of massive species differs significantly from those in the conventional cosmology. The results are applied to the lightest supersymmetric particles and it is argued that they are viable candidates for the constituents of dark matter, if their mass is about 1000 TeV.

KW - dark matter theory

KW - modified gravity

KW - particle physics - cosmology connection

KW - physics of the early universe

KW - MOTION

UR - http://www.scopus.com/inward/record.url?scp=85070732781&partnerID=8YFLogxK

U2 - 10.1088/1475-7516/2019/04/014

DO - 10.1088/1475-7516/2019/04/014

M3 - Article

AN - SCOPUS:85070732781

VL - 2019

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

SN - 1475-7516

IS - 4

M1 - 014

ER -

ID: 21255015