activity
20242026
collaborators

6 papers

astro-ph.GA2026

Interpretable machine learning of halo gas density profiles: a sensitivity analysis of cosmological hydrodynamical simulations

Daniele Sorini, Sownak Bose, Mathilda Denison +1

Stellar and AGN-driven feedback processes affect the distribution of gas on a wide range of scales, from within galaxies well into the intergalactic medium. Yet, it remains unclear…

astro-ph.CO2026

Simba Simulation: The Effect of Feedback Physics on Matter Distribution in the Cosmic Web

Chenze Dong, Florian Dedieu, Daniela Galárraga-Espinosa +3

The discrepancy between the early-time estimation and late-time observation on the cosmic baryon content - the 'missing baryon problem' - is a longstanding problem in cosmology. Al…

astro-ph.CO2026

Modelling the expulsion of baryons from haloes from first principles: the role of feedback and of the cosmological constant

Oscar Veenema, Daniele Sorini, Sownak Bose

The extent to which galactic-scale astrophysical processes conspire with the underlying cosmological model to expel baryons from haloes remains a central question in galaxy formati…

astro-ph.GA2025

Quantifying Observational Projection Effects with a Simulation-based hot CGM model

Soumya Shreeram, Johan Comparat, Andrea Merloni +11

The hot phase of the circumgalactic medium (CGM) allows us to probe the inflow and outflow of gas within a galaxy, which is responsible for dictating the evolution of the galaxy. S…

astro-ph.CO2025

The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7

Daniele Sorini, Sownak Bose, Rüdiger Pakmor +5

We investigate the redshift evolution of the concentration-mass relationship of dark matter haloes in state-of-the-art cosmological hydrodynamic simulations and their dark-matter-o…

astro-ph.GA2024

The impact of feedback on the evolution of gas density profiles from galaxies to clusters: a universal fitting formula from the Simba suite of simulations

Daniele Sorini, Sownak Bose, Romeel Davé +1

The radial distribution of gas within galactic haloes is connected to the star formation rate and the nature of baryon-driven feedback processes. Using six variants of the hydrodyn…