Protokeorks

Protokeorks are a hypothetical class of celestial objects that have been theorized to exist in the early universe. The concept of protokeorks arose from attempts to explain certain observed properties of galaxies and galaxy clusters that are not fully accounted for by current cosmological models. Specifically, they were proposed to address anomalies related to the distribution of matter and the formation of large-scale structures.

The term "protokeork" itself is a portmanteau, combining "proto-" indicating an early stage, and "keork," a term lacking a clear, established etymology but generally understood in this context to refer to dense, gravitationally bound structures. The idea is that these objects were precursors to the more familiar dark matter halos or even primordial black holes. They are thought to have possessed significant gravitational influence, playing a crucial role in seeding the formation of subsequent cosmic structures by attracting ordinary matter.

The theoretical framework surrounding protokeorks suggests they might have been composed of exotic forms of matter or had specific properties related to dark matter interactions that are not yet understood. While the existence of protokeorks remains speculative, their investigation is part of ongoing efforts to refine our understanding of cosmic evolution and the fundamental nature of matter and gravity in the early universe. Further observational data and theoretical advancements are needed to confirm or refute their existence.