activity
20182026
most citedSOLAR: Deep Structured Representations for Model-Based Reinforcement Learning

132 citations · 885 across the 51 of their papers we have counts for

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6 papers · 1 filter

astro-ph.HE2025

Simulating the LOcal Web (SLOW) -- VI: Gamma-ray Emission in the Local Universe

Ludwig M. Böss, Ildar Khabibullin, Daniel Karner +4

Context: Diffuse -ray emission from cosmic-ray (CR) protons scattering off the gas in the intracluster and intergalactic medium remains out of reach for current observations. De…

astro-ph.HE2023★ 12 cited

A formation mechanism for "Wrong Way" Radio Relics

Ludwig M. Böss, Ulrich P. Steinwandel, Klaus Dolag

Radio Relics are typically found to be arc-like regions of synchrotron emission in the outskirts of merging galaxy clusters, bowing out from the cluster center. In most cases they…

astro-ph.HE2023★ 17 cited

An Analytic Model For Magnetically-Dominated Accretion Disks

Philip F. Hopkins, Jonathan Squire, Eliot Quataert +6

Recent numerical cosmological radiation-magnetohydrodynamic-thermochemical-star formation simulations have resolved the formation of quasar accretion disks with Eddington or super-…

astro-ph.HE2023★ 49 cited

FORGE'd in FIRE II: The Formation of Magnetically-Dominated Quasar Accretion Disks from Cosmological Initial Conditions

Philip F. Hopkins, Jonathan Squire, Kung-Yi Su +9

In a companion paper, we reported the self-consistent formation of quasar accretion disks with inflow rates down to <300 Schwarzschild radii fro…

astro-ph.HE2023

Galaxy Cluster simulations with a spectral Cosmic Ray model -- "Wrong Way" Radio Relics

Ludwig M. Böss, Ulrich P. Steinwandel, Klaus Dolag

Non-thermal emission from relativistic electrons gives insight into the strength and morphology of intra-cluster magnetic fields, as well as providing powerful tracers of structure…

astro-ph.HE2022★ 31 cited

CRESCENDO: An on-the-fly Fokker-Planck Solver for Spectral Cosmic Rays in Cosmological Simulations

Ludwig M. Böss, Ulrich P. Steinwandel, Klaus Dolag +1

Non-thermal emission from relativistic Cosmic Ray (CR) electrons gives insight into the strength and morphology of intra-cluster magnetic fields, as well as providing powerful trac…