activity
20182025
most citedConstraints on warm dark matter from UV luminosity functions of high-z galaxies with Bayesian model comparison

39 citations · 143 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2025

Sensitivity of the redshifted 21 cm signal from the Dark Ages to parameters of primordial magnetic fields

Bohdan Novosyadlyj, Yurii Kulinich, Nazar Fortuna +1

We analyse the impact of the decaying magnetic turbulence of primordial magnetic fields (PMFs) and ambipolar diffusion on the ionisation and thermal history of the Dark Ages Univer…

astro-ph.CO2024★ 3 cited

SPARC galaxies prefer Dark Matter over MOND

Mariia Khelashvili, Anton Rudakovskyi, Sabine Hossenfelder

We currently have two different hypotheses to solve the missing mass problem: dark matter (DM) and modified Newtonian dynamics (MOND). In this work, we use Bayesian inference appli…

astro-ph.CO2022★ 27 cited

Dark matter profiles of SPARC galaxies: a challenge to fuzzy dark matter

Mariia Khelashvili, Anton Rudakovskyi, Sabine Hossenfelder

Stellar and gas kinematics of galaxies are a sensitive probe of the dark matter distribution in the halo. The popular fuzzy dark matter models predict the peculiar shape of density…

astro-ph.CO2021★ 39 cited

Constraints on warm dark matter from UV luminosity functions of high-z galaxies with Bayesian model comparison

Anton Rudakovskyi, Andrei Mesinger, Denys Savchenko +1

The number density of small dark matter (DM) halos hosting faint high-redshift galaxies is sensitive to the DM free-streaming properties. However, constraining these DM properties…

astro-ph.CO2019★ 6 cited

Can EDGES observation favour any dark matter model?

Anton Rudakovskyi, Denys Savchenko, Maksym Tsizh

The recent detection of the 21-cm absorption signal by the EDGES collaboration has been widely used to constrain the basic properties of dark matter particles. However, extracting…

astro-ph.GA2019★ 1 cited

New model of density distribution for fermionic dark matter halos

A. Rudakovskyi, D. Savchenko

In this paper, we formulate a new model of density distribution for halos made of warm dark matter (WDM) particles. The model is described by a single microphysics parameter - the…

astro-ph.CO2019★ 26 cited

21-cm observations and warm dark matter models

Alexey Boyarsky, Dmytro Iakubovskyi, Oleg Ruchayskiy +2

Observations of the redshifted 21-cm signal (in absorption or emission) allow us to peek into the epoch of "dark ages" and the onset of reionization. These data can provide a novel…

astro-ph.CO2019★ 37 cited

New mass bound on fermionic dark matter from a combined analysis of classical dSphs

Denys Savchenko, Anton Rudakovskyi

Dwarf spheroidal galaxies (dSphs) are the most compact dark matter-dominated objects observed so far. The Pauli exclusion principle limits the number of fermionic dark matter parti…

astro-ph.CO2018★ 4 cited

Dark matter model favoured by reionization data: 7 keV sterile neutrino vs cold dark matter

Anton Rudakovskyi, Dmytro Iakubovskyi

One of possible explanations of a faint narrow emission line at 3.5 keV reported in our Galaxy, Andromeda galaxy and a number of galaxy clusters is the dark matter made of 7 keV st…