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Towards better discrimination and improved modelling of dark-sector showers
by Andy Buckley, Deepak Kar, Sukanya Sinha
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Submission summary
Authors (as registered SciPost users): | Andy Buckley · Deepak Kar · Sukanya Sinha |
Submission information | |
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Preprint Link: | https://arxiv.org/abs/2209.14964v2 (pdf) |
Date accepted: | July 4, 2023 |
Date submitted: | Oct. 4, 2022, 9:42 a.m. |
Submitted by: | Sinha, Sukanya |
Submitted to: | SciPost Physics Proceedings |
Proceedings issue: | 51st International Symposium on Multiparticle Dynamics (ISMD2022) |
Ontological classification | |
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Academic field: | Physics |
Specialties: |
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Approaches: | Experimental, Phenomenological |
Abstract
As no evidence for classic WIMP-based signatures of dark matter have been found at the LHC, several phenomenological studies have raised the possibility of accessing a strongly-interacting dark sector through new collider-event topologies. If dark mesons exist, their evolution and hadronization procedure are currently little constrained. They could decay promptly and result in QCD-like jet structures, even though the original decaying particles are dark sector ones; they could behave as semi-visible jets; or they could behave as completely detector-stable hadrons, in which case the final state is just the missing transverse momentum. In this contribution we will introduce a study performed to explore use of jet substructure methods to distinguish dark-sector from QCD jets in the first two scenarios, using observables in a IRC-safe linear basis, and discuss ways forward for this approach to dark-matter at the LHC.
Published as SciPost Phys. Proc. 15, 006 (2024)
Reports on this Submission
Report #1 by Anonymous (Referee 1) on 2023-1-17 (Contributed Report)
- Cite as: Anonymous, Report on arXiv:2209.14964v2, delivered 2023-01-17, doi: 10.21468/SciPost.Report.6543