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(Reference retrieved automatically from Web of Science through information on FAPESP grant and its corresponding number as mentioned in the publication by the authors.)

Di-Higgs blind spots in gravitational wave signals

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Author(s):
Alves, Alexandre [1] ; Goncalves, Dorival [2] ; Ghosh, Tathagata [3, 4, 5] ; Guo, Huai-Ke [6] ; Sinha, Kuver [6]
Total Authors: 5
Affiliation:
[1] Univ Fed Sao Paulo, UNIFESP, Dept Fis, BR-09972270 Diadema - Brazil
[2] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 - USA
[3] Univ Sao Paulo, Inst Fis, BR-05508090 Sao Paulo - Brazil
[4] Univ Hawaii, Dept Phys & Astron, Honolulu, HI 96822 - USA
[5] Univ Pittsburgh, PITT PACC, Dept Phys & Astron, 3941 OHara St, Pittsburgh, PA 15260 - USA
[6] Univ Oklahoma, Dept Phys & Astron, Norman, OK 73019 - USA
Total Affiliations: 6
Document type: Journal article
Source: Physics Letters B; v. 818, JUL 10 2021.
Web of Science Citations: 2
Abstract

Conditions for strong first-order phase transition and generation of observable gravitational wave (GW) signals are very restrictive to the profile of the Higgs potential. Working in the minimal extension of the SM with a new gauge singlet real scalar, we show that the production of signals relevant for future GW experiments, such as LISA, can favor depleted resonant and non-resonant di-Higgs rates at colliders for phenomenologically relevant regimes of scalar mixing angles and masses for the heavy scalar. We perform a comprehensive study on the emergence of these di-Higgs blind spot configurations in GWs and also show that di-boson channels, ZZ and WW, can restore the phenomenological complementarities between GW and collider experiments in these parameter space regimes. (C) 2021 The Author(s). Published by Elsevier B.V. (AU)

FAPESP's process: 19/17182-0 - Particle Physics Phenomenology
Grantee:Tathagata Ghosh
Support Opportunities: Scholarships in Brazil - Post-Doctoral