activity
20182025
most citedThe DAMPE excess and gamma-ray constraints

19 citations · 47 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2025

Reconstruction of the dark matter density profile from cosmic positron anomaly data

K. M. Belotsky, F. V. Kostromin, M. L. Solovyov

In this work we continue our investigations of the possibility of explanation of the positron anomaly (PA) in cosmic rays with the help of annihilating or decaying dark matter (DM)…

hep-ph2023

On the Possible Asymmetry in Gamma Rays from Andromeda Due to Inverse Compton Scattering of Star Light on Electrons from Dark Matter Annihilation

Konstantin Belotsky, Maxim Solovyov

Dark matter is a popular candidate to a new source of primary-charged particles, especially positrons in cosmic rays, which are proposed to account for observable anomalies. While…

astro-ph.CO2022★ 2 cited

Hot primordial regions with anomalous hydrogenless chemical composition

K. M. Belotsky, M. M. El Kasmi, S. G. Rubin +1

We study primordial nucleosynthesis in hypothetical hot regions that could be formed by the primordial density inhomogeneities. It is shown that the regions survived up to the pres…

astro-ph.HE2020★ 1 cited

The "Dark disk" model in the light of DAMPE experiment

M. L. Solovyov, M. A. Rakhimova, K. M. Belotsky

There are a lot of models considering the Dark Matter (DM) to be the origin of cosmic ray (CR) positron excess. However, they face an obstacle in the form of gamma-rays. Simple DM…

hep-ph2020★ 3 cited

Cosmic Gamma Ray Constraints on the Indirect Effects of Dark Matter

Konstantin M. Belotsky, Airat Kh. Kamaletdinov, Ekaterina S. Shlepkina +1

The observed anomalous excess of high-energy cosmic ray (CR) positrons is widely discussed as possible indirect evidence for dark matter (DM). However, any source of cosmic positro…

hep-ph2019★ 11 cited

Indirect effects of dark matter

K. M. Belotsky, E. A. Esipova, A. Kh. Kamaletdinov +2

Here we briefly review possible indirect effects of dark matter (DM) of the Universe. It includes effects in cosmic rays (CR): first of all, the positron excess at 500 GeV a…