The Cosmological Dynamics of String Theory Axion Strings
Joshua N. Benabou, Quentin Bonnefoy, Malte Buschmann, Soubhik Kumar,, Benjamin R. Safdi

TL;DR
This paper explores the unique behavior of string theory axions in the early universe, showing they generally do not form strings and overproduce dark matter unless specific conditions like large warping are met, with implications for gravitational wave signals.
Contribution
It demonstrates that string theory axions differ from field theory axions in string formation and dark matter production, highlighting scenarios where axion strings can form and impact cosmological observations.
Findings
String theory axions rarely form strings in the early universe.
QCD axion strings tend to overproduce dark matter, ruling them out in most scenarios.
Heavier axion eigenstates can alter string network evolution and produce gravitational waves.
Abstract
The quantum chromodynamics (QCD) axion may solve the strong CP problem and explain the dark matter (DM) abundance of our Universe. The axion was originally proposed to arise as the pseudo-Nambu Goldstone boson of global Peccei-Quinn (PQ) symmetry breaking, but axions also arise generically in string theory as zero modes of higher-dimensional gauge fields. In this work we show that string theory axions behave fundamentally differently from field theory axions in the early Universe. Field theory axions may form axion strings if the PQ phase transition takes place after inflation. In contrast, we show that string theory axions do not generically form axion strings. In special inflationary paradigms, such as D-brane inflation, string theory axion strings may form; however, their tension is parametrically larger than that of field theory axion strings. We then show…
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Taxonomy
TopicsComputational Physics and Python Applications · Cosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena
