• Open Access

Prospects for light charged scalars in a three-Higgs-doublet model with Z3 symmetry

Manimala Chakraborti, Dipankar Das, Miguel Levy, Samadrita Mukherjee, and Ipsita Saha
Phys. Rev. D 104, 075033 – Published 26 October 2021

Abstract

The stringent constraints from the direct searches for exotic scalars at the LHC, as well as indirect bounds from flavor physics measurements, have imposed severe restrictions on the parameter space of new physics models featuring extended Higgs sectors. In the type-II two-Higgs-doublet model (2HDM), this implies a lower bound on the charged Higgs masses of O(600GeV). In this work we analyze the phenomenology of a Z3 symmetric three-Higgs-doublet model in the alignment limit focusing on the impact of flavor physics constraints on its parameter space. We show that the couplings of the two charged Higgs bosons in this model feature an additional suppression factor compared to type-II 2HDM. This gives rise to a significant relaxation of the flavor physics constraints in this model, allowing the charged Higgs masses to be as low as O(200GeV). We also consider the constraints coming from precision electroweak observables and the observed diphoton decay rate of the 125 GeV Higgs boson at the LHC. The bounds coming from the direct searches of nonstandard Higgs bosons at the LHC, particularly those from resonance searches in the ditau channel, prove to be very effective in constraining this scenario further.

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  • Received 21 April 2021
  • Accepted 30 September 2021

DOI:https://doi.org/10.1103/PhysRevD.104.075033

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Manimala Chakraborti1,*, Dipankar Das2,†, Miguel Levy3,‡, Samadrita Mukherjee4,§, and Ipsita Saha5,∥

  • 1Astrocent, Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences, ul.Rektorska 4, 00-614 Warsaw, Poland
  • 2Department of Physics, Indian Institute of Technology (Indore), Khandwa Road, Simrol, 453 552 Indore, India
  • 3Centro de Física Teórica de Partículas-CFTP and Departamento de Física, Instituto Superior Técnico, Universidade de Lisboa, Av Rovisco Pais, 1, P-1049-001 Lisboa, Portugal
  • 4School of Physical Sciences, Indian Association for the Cultivation of Science, Kolkata 700 032, India
  • 5Kavli IPMU (WPI), UTIAS, University of Tokyo, Kashiwa 277-8583, Japan

  • *mani.chakraborti@gmail.com
  • d.das@iiti.ac.in
  • miguelplevy@ist.utl.pt
  • §samadritamukherjee657@gmail.com
  • ipsita.saha@ipmu.jp

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Vol. 104, Iss. 7 — 1 October 2021

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