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PreprintCC BY 4.0arXiv

Semi-visible Jets from Sneaky Dark Matter

  • Deepak Kar
  • Christiane Scherb
  • Pedro Schwaller
  • Sukanya Sinha
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Abstract

In this paper, we compare two different ways of generating semi-visible jet signature in non-resonant production mode, and flag the potential advantages of the new generation approach we propose. In addition, we suggest a more efficient matrix element to parton shower matching configuration for this hadronic final state signature. Finally, we perform a reinterpretation study of the ATLAS search for t-channel semi-visible jet production and obtain collider limits on the sneaky DM scenario.

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Cite

BibTeXRIS
BibTeX
@misc{kar2026semivisible,
  title = {{Semi-visible Jets from Sneaky Dark Matter}},
  author = {Deepak Kar and Christiane Scherb and Pedro Schwaller and Sukanya Sinha},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2609.13438},
  eprint = {2609.13438},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.13438},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Semi-visible Jets from Sneaky Dark Matter
AU  - Deepak Kar
AU  - Christiane Scherb
AU  - Pedro Schwaller
AU  - Sukanya Sinha
PY  - 2026
DA  - 2026/10/21
PB  - arXiv
DO  - 10.48550/arxiv.2609.13438
UR  - https://arxiv.org/abs/2609.13438
AB  - In this paper, we compare two different ways of generating semi-visible jet signature in non-resonant production mode, and flag the potential advantages of the new generation approach we propose. In addition, we suggest a more efficient matrix element to parton shower matching configuration for this hadronic final state signature. Finally, we perform a reinterpretation study of the ATLAS search for t-channel semi-visible jet production and obtain collider limits on the sneaky DM scenario.
ER  -