Speaker
Ludwig Böss
(University Observatory Munich)
Description
We present a part of the Simulating the LOcal Web (SLOW) project consisting of a cosmological non-radiative MHD simulation of a 500 Mpc h^-1 box including the spectral Cosmic Ray (CR) model presented in Böss et. al. (2022). I will briefly introduce the solver and show its application to predicting synchrotron emission from cosmic web filaments and accretion shocks around clusters, as well as implications of different magnetic field models on this emission.
