Hawking Copy
In physics, Hawking radiation or Beckenstein-Hawking radiation is a thermal radiation that a black hole emits due to quantum mechanical effects. To put it simply, according to the principle of uncertainty, a quantum fluctuation occurs in a vacuum, resulting in the creation of a pair of particles and an attractor near the horizon of the thought of a black hole. Among the two particles generated at that time, the importer falls toward the horizon of the thought of the black hole, and the particles are released to the outside. Entrants that fall into the black hole collide with the particles inside the black hole and die out, releasing energy and reducing the mass. At this time, the radiation of the particles emitted outside the black hole is Hawking radiation. In the case of hocking radiation, the black hole loses its mass in this process, so that the black hole with a larger mass loss than the absorbing mass will gradually decrease and eventually disappear. According to the theory, the smaller the black hole, the more heat radiation it releases. Hawking radiation is considered to be an important first step toward quantum gravity theory.