Published 2018 | Version v1
Journal article

Light signals from a lighter Higgs

  • 1. Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
  • 2. Flatiron Institute, New York, NY (United States)
  • 3. New York University (NYU), New York, NY (United States)

Description

Here, with the Higgs search program already quite mature, there is the exciting possibility of discovering a new particle with rates near that of the SM Higgs. We consider models with a signal in γγ below the SM Higgs mass, taking the recent 2.9σ (local) CMS excess at 95 GeV as a target. We discuss singlet models with additional vectorlike matter, but argue that a Type-I two Higgs doublet model provides a more economical scenario. In such a setup, going into regions of moderate-to-strong fermiophobia, the enhanced γγ branching ratio allows signals from VH+VBF production to yield σ×BRγγ comparable to total SM rates. Light H production can be dominated via rare top decays tbH+bWH, which provides an alternate explanation of the excess. We consider this in the context of other Higgs anomalies, namely the LEP Higgs excess near the same mass, and excesses in tt¯h searches at Tevatron and LHC. We find that with 140GeV<mH+<160GeV, tanβ5 and a coupling to gauge bosons of sin2δ0.1, such a scenario can produce all the excesses simultanously, where tth arise from contamination from the rare top decays, as previously proposed. An implication of the Type-I scenario is that any γγ excess should be associated with additional elements that could reduce background, including b-jets, forward jets or signs of vector boson production.

Availability note (English)

Available from https://www.osti.gov/servlets/purl/1463681; https://www.osti.gov/biblio/1463681; DOE Accepted Manuscript full text, or the publishers Best Available Version will be available free of charge after the embargo period

Additional details

Publishing Information

Journal Title
Journal of High Energy Physics (Online)
Journal Volume
2018
Journal Issue
8
Journal Page Range
14 p.
ISSN
1029-8479

Optional Information