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Journal Article PUBDB-2025-04228

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Preheating Axions in String Cosmology

 ;  ;  ;

2025
Springer Heidelberg

Journal of high energy physics 04(4), 095 () [10.1007/JHEP04(2025)095]
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Report No.: DESY-24-163; KCL-PH-TH/2024-60; arXiv:2411.18496

Abstract: Certain inflationary models can feature periods of preheating - an era preceding reheating during which parametric resonance triggers an exponential production of bosons. This non-perturbative process can have significant impact on the history of our universe, with consequences ranging from altered reheating channels to overproduction of dark radiation to overclosure. In this work, we study parametric resonance production of axions in string models of inflation. We find that the kinetic couplings and moduli-dependent axion masses give rise to generalizations of the Mathieu equation. We study these generalizations and determine the strength of parametric resonance created by such couplings. We then apply this technology to fibre inflation models in Type IIB orientifold compactifications. We find that heavy axions can be copiously produced and avoidance of overclosure results in constraints on the typical fibre inflation parameter space.

Keyword(s): Axions and ALPs ; Early Universe Particle Physics ; String and Brane Phenomenology ; Superstring Vacua

Classification:

Note: 48 pages, 10 figures, v2: several important references added

Contributing Institute(s):
  1. Theorie-Gruppe (T)
Research Program(s):
  1. 611 - Fundamental Particles and Forces (POF4-611) (POF4-611)
  2. DFG project G:(GEPRIS)390833306 - EXC 2121: Das Quantisierte Universum II (390833306) (390833306)
  3. SFB 1624 B03 - Modulräume und Quantengravitation (B03) (531727554) (531727554)
Experiment(s):
  1. No specific instrument

Appears in the scientific report 2025
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Preheating Axions in String Cosmology
[10.3204/PUBDB-2024-06495]  GO OpenAccess  Download fulltext Files  Download fulltextFulltext by arXiv.org BibTeX | EndNote: XML, Text | RIS


 Record created 2025-10-07, last modified 2026-04-14


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