Journal of Materials Science and Emerging Technologies
Research Article Volume: 2 & Issue: 1
Abstract
“Black holes” are stars that are believed to have such large masses and small sizes that light, consisting of photons, cannot overcome gravity and escape the star. Such a star becomes invisible. The condition, that one component escapes from a binary mass system is used to determine the parameters of a black hole. This condition is used in astronautics. However, it is questionable whether a star (for example, a quasar with a mass of mo = 1039 kg) and a photon of light (with a “mass of motion” of the order of mo = 10-35 kg) can be considered a binary mass system. Not to mention that any star simultaneously emits a huge number of photons in different directions, and before the photon is emitted from the star, the photon has no mass. A photon’s mass is related to its motion. In existing popular science literature, one can find the assertion that a star with the parameters of the Sun, having turned into a black hole, will collapse into a sphere with a tiny three-kilometer radius. This article draws the reader’s attention to the fact that a star with the mass of the Sun, having turned into a black hole, rotates rapidly and will be destroyed by centrifugal forces. Contrary to modern cosmological beliefs, the space around stars is not empty. It is filled with gaseous dark matter. Stars continuously absorb dark matter, increasing their mass. Therefore, photons emitted by the star at the speed of light are forced to overcome this oncoming current. If the speed of the counter-current of dark matter exceeds the speed of light, the star becomes invisible, that is, it turns into a black hole. A formula has been derived that determines this speed. Calculations using this formula have shown that stars with masses on the order of the Sun’s mass can, as a result of catastrophic compression (collapse), turn into black holes with parameters close to those of “white dwarfs.” Such stars, invisible black holes, should be at least as numerous in nature as white dwarfs. White dwarfs are close to the threshold of star visibility. It’s no wonder astronomers don’t see stars smaller than white dwarfs in the sky. This invisible mass is not taken into account by astrophysicists when estimating the masses of galaxies. This can lead to misconceptions about the structure, fate, and role of black holes in the dialectic of the Universe.