Hypothetical black holes shaped within the very early universe, probably earlier than the formation of stars and galaxies, might possess a property analogous to electrical cost, however associated to the sturdy nuclear power. This “coloration cost,” a attribute of quarks and gluons described by quantum chromodynamics (QCD), might considerably affect these early-universe objects’ interactions and evolution. Not like stellar-mass black holes shaped from collapsing stars, these objects might have a variety of plenty, presumably even smaller than a single atom.
The existence of such objects might have profound implications for our understanding of the early universe, darkish matter, and the evolution of cosmic constructions. These small, charged black holes may need performed a task within the formation of bigger constructions, served as seeds for galaxy formation, and even represent a portion of darkish matter. Their potential discovery would supply invaluable insights into the situations of the early universe and the character of basic forces. Investigating these hypothetical objects may also make clear the interaction between normal relativity and quantum area idea, two cornerstones of recent physics which are notoriously troublesome to reconcile.
