# Dark matter in $R+R^2$ cosmology

Source: [Dark matter in $R+R^2$ cosmology](<https://www.sota2.com/research/paper/68fa39851e209131ce8c312a>)

Collection index: [llms.txt](<https://www.sota2.com/research/llms.txt>)

Data updated: 2025-10-24T23:33:11.663Z

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

Published: 2018-11-13T16:47:27.000Z

## Abstract

Production of massive stable relics in $R^2$-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.

## Recorded benchmark results

A research result applies to its stated dataset, split, metric and evaluation configuration. Compare like-for-like settings, preserve the metric's unit and direction, and distinguish paper-reported results from independent reproduction. The best result recorded here is not a claim of exhaustive, current global coverage.

## Original sources and implementation

[Original paper](<https://arxiv.org/abs/1811.05399>)

[PDF](<https://arxiv.org/pdf/1811.05399.pdf>)
