Active galactic nuclei influencing galaxy evolution through energy and matter outflows.Black hole feedback refers to the process by which a supermassive black hole at the center of a galaxy injects energy and momentum into its surroundings, profoundly influencing the galaxy's evolution. This feedback can heat or expel gas, suppress star formation, and shape the intergalactic medium. It is a central ingredient in modern models of galaxy formation, explaining why large galaxies have fewer stars than expected from simple gravitational collapse.
The term 'feedback' was borrowed from engineering and applied to black holes in the 1990s, but the idea that active galactic nuclei could affect their host galaxies dates back to the 1970s. Observations of cavities in galaxy clusters in the early 2000s provided direct evidence.
As matter falls toward a black hole, it forms an accretion disk that can launch relativistic jets and fast winds. These outflows carry enormous kinetic energy, which is deposited into the surrounding gas over millions of years. The energy can heat the gas to temperatures so high that it cannot cool and collapse to form stars, or it can physically push gas out of the galaxy. The efficiency of this process depends on the black hole's accretion rate and the density of the surrounding medium.
Black hole feedback is essential for cosmological simulations of galaxy formation and for interpreting observations of galaxy clusters, where it explains the balance between cooling and heating of the hot gas.
The energy released by a single supermassive black hole outburst can exceed the combined energy of all the stars in its host galaxy.




