Baryonid

Baryon is a term that is often used synonymously with Baryonid. It is a hypothetical type of black hole that was proposed in the 1960s by physicist John Wheeler. Baryonids are thought to be formed when a normal star undergoes a certain type of supernova, resulting in the collapse of the star into a small, extremely dense point called a singularity.

Theoretically, baryonids are smaller and less likely to form than other types of black holes, such as stellar black holes. They are thought to be formed from the compact object, typically a neutron star, that remains after a supernova has exploded, and can be nearly as small as 1 kilometer in diameter. This compact object then completely collapses into the singularity, creating a baryonid. Because this collapse is almost perfectly spherical and extreme, the gravitational pull is enormous, resulting in singularities of extremely high density and gravitation.

Some speculate that a baryonid could, in theory, also be used to explain the matter-antimatter asymmetry of the universe, where scientists have challenged theories that attempt to describe why the universe came to be made primarily of matter. This phenomenon may possibly be explained by their huge mass flux and subsequent brief loss to blowholes through stellar singularities. In the process, baryonids can collapse and convert normal particles to matter in a perpetual matter-antimatter cycle, spewing out copious amounts of both small, invisible particles and link an overpowering, dulled cosmic expulsion of brightness whenever volumetric thresholds are surpassed.