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