Stasis in an expanding universe: A recipe for stable mixed-component cosmological eras
One signature of an expanding universe is the time variation of the cosmological abundances of its different components. For example, a radiation-dominated universe inevitably gives way to a matter-dominated universe, and critical moments such as matter-radiation equality are fleeting. In this paper, we point out that this lore is not always correct and that it is possible to obtain a form of “stasis” in which the relative cosmological abundances $$Ω_i$$ of the different components remain unchanged over extended cosmological epochs, even as the universe expands. Moreover, here we demonstrate that such situations are not fine-tuned but are actually global attractorsmore »