activity
20232026
most citedThe Cosmological Simulation Code OpenGadget3 -- Implementation of Meshless Finite Mass

34 citations · 56 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.IM2026

The OpenGadget3 Code for Cosmological Simulations

Klaus Dolag, Geray S. Karademir, Luca Tornatore +28

We present the public release of OpenGadget3 (OG3), a substantially extended and re-organised version of the widely used Gadget-2/3 family of cosmological simulation codes. Since G…

astro-ph.CO2026

The Quiescent Sloshing Core of Abell 496 with XRISM

Angie Veronica, Thomas H. Reiprich, Naomi Ota +9

Gas motions provide insight into the dynamical history and physical processes within galaxy clusters. We investigate the kinematics of the ICM in the core of A496, a nearby, X-ray…

astro-ph.IM2026

OpenGadget3 GPU solver tests

A. Ragagnin, G. S. Karademir, F. Groth +6

We present an in-depth evaluation of the scalability and accuracy of the GPU porting of the N-body code for hydrodynamic cosmological simulations \og. While technical details of ou…

astro-ph.CO2025★ 3 cited

Turbulence in Simulated Local Cluster Analogs: One-to-one comparisons between SLOW and XRISM/Hitomi

Frederick Groth, Milena Valentini, Benjamin A. Seidel +4

The XRISM Resolve X-ray spectrometer allows to gain detailed insight into gas motions of the intra cluster medium (ICM) of galaxy clusters. Current simulation studies focus mainly…

astro-ph.CO2025★ 4 cited

N-body simulations of dark matter-baryon interactions

Moritz S. Fischer, Klaus Dolag, Mathias Garny +3

Dark matter (DM) particles can interact with particles of the standard model. Although there are a number of constraints derived from direct and indirect detection experiments, the…

astro-ph.CO2024★ 8 cited

Turbulent Pressure Support in Galaxy Clusters -- Impact of the Hydrodynamical Solver

Frederick Groth, Milena Valentini, Ulrich P. Steinwandel +2

The amount of turbulent pressure in galaxy clusters is still debated, especially as for the impact of the dynamical state and the hydro-method used for simulations. We study the tu…

astro-ph.IM2024★ 7 cited

Vortex-p: a Helmholtz-Hodge and Reynolds decomposition algorithm for particle-based simulations

David Vallés-Pérez, Susana Planelles, Vicent Quilis +3

Astrophysical turbulent flows display an intrinsically multi-scale nature, making their numerical simulation and the subsequent analyses of simulated data a complex problem. In par…

astro-ph.IM2023★ 34 cited

The Cosmological Simulation Code OpenGadget3 -- Implementation of Meshless Finite Mass

Frederick Groth, Ulrich P. Steinwandel, Milena Valentini +1

Subsonic turbulence plays a major role in determining properties of the intra cluster medium (ICM). We introduce a new Meshless Finite Mass (MFM) implementation in OpenGadget3 and…