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Cosmological Implications of Radiatively Generated Axion Scale

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arxiv hep-ph/9608222 v1 pith:NHTOV4UX submitted 1996-08-03 hep-ph

classification hep-ph
keywords axioncosmologicalmodelsscalegeneratedimplicationsinflationnucleosynthesis
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We study cosmological implications of supersymmetric axion models in which the axion scale is generated radiatively. Such models lead to the so-called thermal inflation and subsequent reheating should be constrained not to yield a too large axion energy density at the time of nucleosynthesis. We examine how plausible it is that this nucleosynthesis constraint is satisfied for both hadronic and Dine-Fischler-Srednicki-Zhitnitskii type axion models. Baryogenesis and the possibility for raising up the cosmological upper bound on the axion scale in thermal inflation scenario are also discussed.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Aspects of the WIMP quality problem and R-parity violation in natural supersymmetry with all axion dark matter

    hep-ph 2025-05 conditional novelty 6.0 of 10

    In natural supersymmetry with discrete R-symmetries, R-parity violation at the 1e-7 level can make the lightest supersymmetric particle decay before nucleosynthesis, leaving only axion dark matter, and LHC non-observa...

  2. Decay rate of PQ-ball

    hep-ph 2025-04 conditional novelty 6.0 of 10

    PQ-balls, Q-balls in a spontaneously broken U(1) theory, are metastable in vacuum and decay at a rate proportional to the square of their asymptotic field value.

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