Dark matter in R+R2 cosmology

E. V. Arbuzova; A. D. Dolgov; R. S. Singh

doi:10.1088/1475-7516/2019/04/014

Dark matter in R+R² cosmology

E. V. Arbuzova, A. D. Dolgov, R. S. Singh

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

7 Citations (Scopus)

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.

Original language	English
Article number	014
Number of pages	16
Journal	Journal of Cosmology and Astroparticle Physics
Volume	2019
Issue number	4
DOIs	https://doi.org/10.1088/1475-7516/2019/04/014
Publication status	Published - 8 Apr 2019

Keywords

dark matter theory
modified gravity
particle physics - cosmology connection
physics of the early universe
MOTION

Access to Document

10.1088/1475-7516/2019/04/014

Link to publication in Scopus

Cite this

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