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Relaxation of Higgs mass and cosmological constant with four-form fluxes and reheating

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arxiv 1908.04252 v3 pith:SWBF5OTU submitted 2019-08-12 hep-ph hep-th

classification hep-phhep-th
keywords four-formhiggsconstantcosmologicalcouplingfieldfluxesgravity
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We consider the most general effective action for the four-form fluxes in the Standard Model coupled to gravity. The Higgs mass parameter can be relaxed to a correct value due to the four-form coupling to the Higgs field and it stops changing due to an extremely suppressed transition probability from the observed cosmological constant to AdS space. We first introduce a non-minimal four-form coupling to gravity and discuss the role of a new scalar field as the inflaton and the conditions for a successful reheating at the end of relaxation.

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    hep-ph 2024-12 conditional novelty 6.0 of 10

    An ALP-Higgs coupling can lower the vacuum instability scale to near the weak scale, predicting an axion-like particle between 1 MeV and 20 GeV that future experiments can fully probe.

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