Theory, phenomenology, and experimental avenues for dark showers: a Snowmass 2021 report

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Abstract

In this work, we consider the case of a strongly coupled dark/hidden sector, which extends the Standard Model (SM) by adding an additional non-Abelian gauge group. These extensions generally contain matter fields, much like the SM quarks, and gauge fields similar to the SM gluons. We focus on the exploration of such sectors where the dark particles are produced at the LHC through a portal and undergo rapid hadronization within the dark sector before decaying back, at least in part and potentially with sizeable lifetimes, to SM particles, giving a range of possibly spectacular signatures such as emerging or semi-visible jets. Other, non-QCD-like scenarios leading to soft unclustered energy patterns or glueballs are also discussed. After a review of the theory, existing benchmarks and constraints, this work addresses how to build consistent benchmarks from the underlying physical parameters and present new developments for the PYTHIA Hidden Valley module, along with jet substructure studies. Finally, a series of improved search strategies is presented in order to pave the way for a better exploration of the dark showers at the LHC.
Original languageEnglish
Article number1132
Number of pages66
JournalThe European Physical Journal C
Volume82
Issue number12
DOIs
Publication statusPublished - 14 Dec 2022

Bibliographical note

Funding Information:
H. Beauchesne’s work was supported by the Ministry of Science and Technology, National Center for Theoretical Sciences of Taiwan. T. Cohen is supported by the U.S. Department of Energy, under grant number DE-SC0011640. The research of D. Curtin was supported in part by a Discovery Grant from the Natural Sciences and Engineering Research Council of Canada, the Canada Research Chair program, the Alfred P. Sloan Foundation, and the Ontario Early Researcher Award. M-H. Genest acknowledges the support of the French Agence Nationale de la Recherche (ANR), under grant ANR-21-CE31-0013 (project DMwithLLPatLHC). G. Grilli di Cortona is supported by the INFN Iniziativa Specifica Theoretical Astroparticle Physics (TAsP) and by the Frascati National Laboratories (LNF) through a Cabibbo Fellowship call 2019. T. Holmes’s research is supported by U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences Energy Frontier Research Centers program under Award Number DE-SC0020267. S. Kulkarni is supported by Austrian Science Fund Elise Richter Fellowship V592-N27. S. Mee is supported by Austrian Science Fund research group funding FG1. S. Kulkarni and S. Mee thank Biagio Lucini, Axel Maas, Simon Plätzer and Fabian Zierler for numerous discussions. K. Pedro, S. Mrenna, K. Folan DiPetrillo and E. Bernreuther are supported by the Fermi National Accelerator Laboratory, managed and operated by Fermi Research Alliance, LLC under Contract No. DE-AC02-07CH11359 with the U.S. Department of Energy. A. Peixoto acknowledges funding from the French Programme d’investissements d’avenir through the Enigmass Labex. The work of J. Shelton was supported in part by the Binational Science Foundation and DOE grant DE-SC0017840. S. Sinha’s work is based on the research supported wholly by the National Research Foundation of South Africa (Extension Support Doctoral Scholarship). T. Sjöstrand is supported by the Swedish Research Council, contract number 2016-05996. The work of D. Stolarski and A. Spourdalakis is supported in part by the Natural Sciences and Engineering Research Council of Canada (NSERC). Work in Mainz was supported by the Cluster of Excellence Precision Physics, Fundamental Interactions, and Structure of Matter (PRISMA+ EXC 2118/1) funded by the German Research Foundation(DFG) within the German Excellence Strategy (Project ID 39083149), and by grant 05H18UMCA1 of the German Federal Ministry for Education and Research (BMBF).

Publisher Copyright:
© 2022, The Author(s).

Copyright:
Copyright 2022 Elsevier B.V., All rights reserved.

Keywords

  • hep-ph
  • hep-ex

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