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arxiv: 1501.04455 · v2 · pith:KDDDCUOOnew · submitted 2015-01-19 · ✦ hep-ph · astro-ph.CO· gr-qc· hep-th

Eternal Higgs inflation and cosmological constant problem

classification ✦ hep-ph astro-ph.COgr-qchep-th
keywords higgsstringfieldscalebehaviorconstantcosmologicalenergy
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We investigate the Higgs potential beyond the Planck scale in the superstring theory, under the assumption that the supersymmetry is broken at the string scale. We identify the Higgs field as a massless state of the string, which is indicated by the fact that the bare Higgs mass can be zero around the string scale. We find that, in the large field region, the Higgs potential is connected to a runaway vacuum with vanishing energy, which corresponds to opening up an extra dimension. We verify that such universal behavior indeed follows from the toroidal compactification of the non-supersymmetric $SO(16)\times SO(16)$ heterotic string theory. We show that this behavior fits in the picture that the Higgs field is the source of the eternal inflation. The observed small value of the cosmological constant of our universe may be understood as the degeneracy with this runaway vacuum, which has vanishing energy, as is suggested by the multiple point criticality principle.

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

  1. Dark Horse, Dark Matter: Revisiting the SO(16)x SO(16)' Nonsupersymmetric Model in the LHC and Dark Energy Era

    hep-th 2019-07 unverdicted novelty 2.0

    Reexamination of the SO(16)xSO(16)' nonsupersymmetric model for implications on dark energy, vacuum stabilization, dark matter candidates, and gauge-Higgs unification in light of LHC and dark energy data.