📝 SummarXiv

Abstract

In the multiverse hypothesis, a range of universes exist with differing values of our physical constants. Here, we investigate how the probabilities of observing our values of these constants depend on the assumptions made about the theories governing particle physics and cosmology, along with habitability. The particle physics effects we consider include constraints on the Higgs vacuum expectation value from big bang nucleosynthesis and supernovae, grand unified theories (GUTs), and standard model stability. Cosmology effects we consider are different theories of dark matter and baryogenesis, and for galactic habitability effects we include star formation efficiency, stellar encounters, supernova explosions, and active galactic nuclei. We find the following to be disfavored in the multiverse scenario: flexible GUTs, pessimistic galactic disruption rates, some origin of life theories, and freeze-out dark matter with high energy baryogenesis. These predictions can be tested in future experiments to either confirm or rule out the multiverse.