A relative black hole is a type of black hole that is formed by the collapse of a large star. It is characterized by its strong gravitational pull, which is so strong that not even light can escape from it. This makes it invisible to the naked eye, but its presence can be detected through its effects on surrounding matter.
Particles can be influenced by the strong gravitational pull of a relative black hole. Depending on their trajectory and speed, they can either be captured by the black hole or be flung out into space. As they approach the event horizon (the point of no return), the particles experience extreme gravitational forces that can cause them to accelerate to high speeds and emit radiation.
There is currently no scientific evidence to suggest that particles can see other universes through relative black holes. The concept of parallel universes or multiple universes is still a subject of speculation and debate among scientists. However, some theories such as the holographic principle suggest that information about other universes may be encoded in the event horizon of a black hole.
Yes, there are several known examples of relative black holes in our universe. Some well-known examples include the black hole at the center of our galaxy, known as Sagittarius A*, and the black hole in the galaxy Messier 87, which was recently captured in the first-ever image of a black hole. These black holes are formed from the collapse of massive stars.
Studying relative black holes can help us better understand the laws of physics and the behavior of matter under extreme conditions. It may also provide insights into the formation and evolution of galaxies, as black holes are thought to play a crucial role in shaping the structure of the universe. Additionally, the study of black holes can also lead to advancements in technology, such as the development of more accurate gravitational wave detectors.