COSMOLOGICAL BLACK HOLES

The concept of cosmological black holes (CBHs) is intriguing but remains firmly in the realm of theoretical speculation, lacking any empirical grounding. These proposed entities, vastly exceeding the scale of supermassive black holes like TON 618 or Phoenix A, are hypothesized to contain the mass of entire galaxies—on the order of 100 trillion solar masses. The suggestion that CBHs formed shortly after cosmic inflation and consumed matter destined for galaxies, thereby creating vast intergalactic voids, is a bold attempt to explain large-scale cosmic structures. But without observational evidence—such as gravitational wave signatures or anomalous lensing effects—this idea remains a mathematical curiosity rather than a substantiated model. It’s an ambitious hypothesis, but until data emerges to support it, CBHs are little more than a provocative thought experiment.