Constraints on Alternate Universes: Stars and habitable planets with different fundamental constants
Fred C. Adams (University of Michigan)

TL;DR
This paper identifies the range of fundamental constants, specifically the fine structure constant and gravitational constant, that allow for habitable universes with stars and planets, revealing a vast but constrained parameter space.
Contribution
It delineates the parameter space of fundamental constants that support habitable universes, providing new constraints and upper bounds on their ratios for the first time.
Findings
Viable habitable universes exist with constants varying over several orders of magnitude.
The ratio of gravitational to electromagnetic force constants must be less than 10^{-34}.
Large hierarchies between fundamental forces are necessary for habitability.
Abstract
This paper develops constraints on the values of the fundamental constants that allow universes to be habitable. We focus on the fine structure constant and the gravitational structure constant , and find the region in the - plane that supports working stars and habitable planets. This work is motivated, in part, by the possibility that different versions of the laws of physics could be realized within other universes. The following constraints are enforced: [A] long-lived stable nuclear burning stars exist, [B] planetary surface temperatures are hot enough to support chemical reactions, [C] stellar lifetimes are long enough to allow biological evolution, [D] planets are massive enough to maintain atmospheres, [E] planets are small enough in mass to remain non-degenerate, [F] planets are massive enough to support sufficiently complex biospheres, [G]…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
