On the Habitability of Universes without Stable Deuterium
Fred C. Adams, Evan Grohs

TL;DR
This paper demonstrates that universes lacking stable deuterium can still support habitable stars through alternative nuclear processes and gravitational contraction, challenging previous assumptions about habitability constraints.
Contribution
It introduces mechanisms like gravitational contraction, explosive nucleosynthesis, and the triple-nucleon reaction as pathways for star formation and element production without stable deuterium.
Findings
Stars can form and remain luminous without stable deuterium.
Explosive nucleosynthesis can produce heavy elements in such universes.
Stars can operate via the CNO cycle with trace heavy elements.
Abstract
In both stars and in the early universe, the production of deuterium is the first step on the way to producing heavier nuclei. If the strong force were slightly weaker, deuterium would not be stable, and many authors have noted that nuclesynthesis would be compromised so that helium production could not proceed through standard reaction chains. Motivated by the possibility that other regions of space-time could have different values for the fundamental constants, this paper considers stellar evolution in universes without stable deuterium and argues that such universes can remain habitable. Even in universes with no stellar nucleosynthesis, stars can form and will generate energy through gravitational contraction. We show that such stars can be sufficiently luminous and long-lived to support life. Stars with initial masses that exceed the Chandrasekhar mass cannot be supported by…
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