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Title: Fate of electroweak vacuum during preheating

Journal Article · · Journal of Cosmology and Astroparticle Physics
 [1];  [2];  [1]
  1. Department of Physics, Faculty of Science, The University of Tokyo,Bunkyo-ku, Tokyo 133-0033 (Japan)
  2. Kavli IPMU (WPI), UTIAS, The University of Tokyo,Kashiwa, Chiba 277-8583 (Japan)

Our electroweak vacuum may be metastable in light of the current experimental data of the Higgs/top quark mass. If this is really the case, high-scale inflation models require a stabilization mechanism of our vacuum during inflation. A possible candidate is the Higgs-inflaton/-curvature coupling because it induces an additional mass term to the Higgs during the slow roll regime. However, after inflation, the additional mass term oscillates, and it can destabilize our electroweak vacuum via production of large Higgs fluctuations during the inflaton oscillation era. In this paper, we study whether or not the Higgs-inflaton/-curvature coupling can save our vacuum by properly taking account of Higgs production during the preheating stage. We put upper bounds on the Higgs-inflaton and -curvature couplings, and discuss possible dynamics that might relax them.

Sponsoring Organization:
SCOAP3, CERN, Geneva (Switzerland)
OSTI ID:
22572177
Journal Information:
Journal of Cosmology and Astroparticle Physics, Vol. 2016, Issue 10; Other Information: PUBLISHER-ID: JCAP10(2016)043; OAI: oai:repo.scoap3.org:17882; cc-by Article funded by SCOAP3. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 License. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.; Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
Country of Publication:
United States
Language:
English

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