Hyesung Kang

TL;DR: In this article, the authors studied the properties of cosmological shock waves identified in high-resolution, N-body/hydrodynamic simulations of a ΛCDM universe and their role on thermalization of gas and acceleration of nonthermal, cosmic-ray (CR) particles.

TL;DR: This model presents a physical mechanism that transfers the gravitational energy to the turbulence and magnetic field energies in the large-scale structure of the universe.

TL;DR: In a growing number of galaxy clusters diffuse extended radio sources have been found. as mentioned in this paper classified diffuse cluster radio sources into radio halos, cluster radio shocks (relics), and revived AGN fossil plasma sources.

TL;DR: In this paper, detailed results for the hydrodynamical, thermal, ionization, and molecular formation history of post-shock cooling flows behind steady state shocks in a primordial gas at redshifts z = 5, 10, and 20 are presented and analyzed for a wide range of shock velocities from 50 to 400 km/s.

TL;DR: In this article, the authors examined the properties of large-scale structure formation in simulations of large scale structure formation and found that the topology of the shocks is very complex and highly connected, and that the amount of inflowing kinetic energy across the shocks around clusters, which represents the power available for cosmic-ray acceleration, is comparable to the cluster X-ray luminosity emitted from a central region of radius 0.5 h-1 Mpc.