collaborators

5 papers

astro-ph.CO2026

Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model

Thomas Montandon, Vivian Poulin, Oliver Hahn +2

We present a semi-analytical framework for the halo mass function (HMF) in decaying dark matter (DDM) cosmologies, in which dark matter decays into a massive daughter particle inhe…

astro-ph.CO2026

Baryonification III: An accurate analytical model for the dispersion measure probability density function of fast radio bursts

MohammadReza Torkamani, Robert Reischke, Michael Kovač +6

We develop an analytical framework to predict the one-point probability distribution function (PDF) of dispersion measures (DMs) for fast radio bursts (FRBs) within the baryonifica…

astro-ph.CO2025

Baryonification: An alternative to hydrodynamical simulations for cosmological studies

Aurel Schneider, Michael Kovač, Jozef Bucko +8

We present an improved baryonification (BFC) model that modifies dark-matter-only -body simulations to generate particle-level outputs for gas, dark matter, and stars. Unlike pr…

astro-ph.CO2025

Baryonification II: Constraining feedback with X-ray and kinematic Sunyaev-Zel'dovich observations

Michael Kovač, Andrina Nicola, Jozef Bucko +6

Baryonic feedback alters the matter distribution on small and intermediate scales, posing a challenge for precision cosmology. The new, component-wise baryonification (BFC) approac…

astro-ph.CO2025

Constraining Hot Dark Matter Sub-Species with Weak Lensing and the Cosmic Microwave Background Radiation

Fabian Hervas Peters, Aurel Schneider, Jozef Bucko +2

Although it is well known that the bulk of dark matter (DM) has to be cold, the existence of an additional sub-dominant, hot species remains a valid possibility. In this paper we i…