Radiative Processes in Astrophysics

Radiative processes in astrophysics refer to the ways in which energy is emitted or absorbed as electromagnetic radiation, such as light. These processes, including thermal radiation, recombination, and scattering, are crucial for understanding the behavior of cosmic objects like stars, galaxies, and plasmas. In computational astrophysics, simulations model these processes to predict how matter interacts with radiation, helping scientists explore phenomena like star formation and the evolution of the universe. By analyzing how energy travels through space, researchers gain insights into the physical conditions of celestial environments and the fundamental laws governing them.