Abstract

We study discovery prospects for a real triplet extension of the Standard Model scalar sector at the Large Hadron Collider (LHC) and a possible future 100 TeV pp collider. We focus on the scenario in which the neutral triplet scalar is stable and contributes to the dark matter relic density. When produced in pp collisions, the charged triplet scalar decays to the neutral component plus a soft pion or soft lepton pair, yielding a disappearing charged track in the detector. We recast current 13 TeV LHC searches for disappearing tracks, and find that the LHC presently excludes a real triplet scalar lighter than 248 (275) GeV, for a mass splitting of 172 (160) MeV with ℒ = 36 fb1. The reach can extend to 497 (520) GeV with the collection of 3000 fb1. We extrapolate the 13 TeV analysis to a prospective 100 TeV pp collider, and find that a 3 TeV triplet scalar could be discoverable with ℒ = 30 ab1, depending on the degree to which pile up effects are under control. We also investigate the dark matter candidate in our model and corresponding present and prospective constraints from dark matter direct detection. We find that currently XENON1T can exclude a real triplet dark matter lighter than 3 TeV for a Higgs portal coupling of order one or larger, and the future XENON20T will cover almost the entire dark matter viable parameter space except for vanishingly small portal coupling.

Details

Title
Collider probes of real triplet scalar dark matter
Author
Cheng-Wei, Chiang 1 ; Cottin Giovanna 2 ; Du, Yong 3   VIAFID ORCID Logo  ; Fuyuto Kaori 4 ; Ramsey-Musolf, Michael J 5 

 National Taiwan University, Department of Physics, Taipei, Taiwan (GRID:grid.19188.39) (ISNI:0000 0004 0546 0241); Academia Sinica, Institute of Physics, Taipei, Taiwan (GRID:grid.28665.3f) (ISNI:0000 0001 2287 1366); Physics Division, National Center for Theoretical Sciences, Taipei, Taiwan (GRID:grid.468468.0) (ISNI:0000 0000 9060 5564) 
 Universidad Adolfo Ibáñez, Departamento de Ciencias, Facultad de Artes Liberales, Santiago, Chile (GRID:grid.440617.0) (ISNI:0000 0001 2162 5606); Pontificia Universidad Católica de Chile, Instituto de Física, Santiago, Chile (GRID:grid.7870.8) (ISNI:0000 0001 2157 0406) 
 University of Massachusetts, Amherst Center for Fundamental Interactions, Department of Physics, Amherst, USA (GRID:grid.266683.f) (ISNI:0000 0001 2184 9220) 
 Theoretical Division, Los Alamos National Laboratory, Los Alamos, USA (GRID:grid.148313.c) (ISNI:0000 0004 0428 3079) 
 Shanghai Jiao Tong University, Tsung-Dao Lee Institute and School of Physics and Astronomy, Shanghai, China (GRID:grid.16821.3c) (ISNI:0000 0004 0368 8293); University of Massachusetts, Amherst Center for Fundamental Interactions, Department of Physics, Amherst, USA (GRID:grid.266683.f) (ISNI:0000 0001 2184 9220); California Institute of Technology, Kellogg Radiation Laboratory, Pasadena, USA (GRID:grid.20861.3d) (ISNI:0000000107068890) 
Publication year
2021
Publication date
Jan 2021
Publisher
Springer Nature B.V.
e-ISSN
10298479
Source type
Scholarly Journal
Language of publication
English
ProQuest document ID
2494555318
Copyright
© The Author(s) 2021. This work is published under CC-BY 4.0 (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.