SciPost Submission Page
Searches for new physics in collision events using a statistical technique for anomaly detection
by S. V. Chekanov
Submission summary
| Authors (as registered SciPost users): | Sergei Chekanov |
| Submission information | |
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| Preprint Link: | https://arxiv.org/abs/2110.06277v1 (pdf) |
| Date accepted: | Feb. 28, 2022 |
| Date submitted: | Oct. 14, 2021, 4:19 p.m. |
| Submitted by: | Sergei Chekanov |
| Submitted to: | SciPost Physics Proceedings |
| Proceedings issue: | 50th International Symposium on Multiparticle Dynamics (ISMD2021) |
| Ontological classification | |
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| Academic field: | Physics |
| Specialties: |
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| Approaches: | Experimental, Phenomenological |
Abstract
This paper discusses a statistical anomaly-detection method for model-independent searches for new physics in collision events produced at the Large Hadron Collider (LHC). The method requires calculations of Z-scores for a large number of Lorenz-invariant variables to identify events that deviate from those expected for the Standard Model (SM).
Published as SciPost Phys. Proc. 10, 015 (2022)
Reports on this Submission
Report #1 by Anonymous (Referee 1) on 2022-1-28 (Invited Report)
- Cite as: Anonymous, Report on arXiv:2110.06277v1, delivered 2022-01-28, doi: 10.21468/SciPost.Report.4264
Strengths
Weaknesses
Report
While not a block for proceedings publication, I note:
0) The RMM is introduced in the author's previous papers, but not really explained here despite not being a widely known concept. But there was a page limit...
1) The effective assumption of Gaussian X_i distributions for RMM seems a bit dangerous, since non-Gaussian tails could masquerade as BSM outliers. I think this can be remedied by a more explicit calculation of full empirical p-value from the found distribution, and conversion to Z, though.
2) The Fig 1 performance plots seem equally normalised across samples with very different cross-sections... this isn't quite clear from the presentation, and a log plot with more realistic cross-sections would illustrate the physics power better, especially re. how the BSM distribution compares to the SM tails.
Requested changes
None needed.