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| 001 | 627807 | ||
| 005 | 20250715151508.0 | ||
| 024 | 7 | _ | |a 10.1103/PhysRevLett.134.181802 |2 doi |
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| 024 | 7 | _ | |a arXiv:2405.08858 |2 arXiv |
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| 088 | _ | _ | |a DESY-24-069 |2 DESY |
| 088 | _ | _ | |a arXiv:2405.08858 |2 arXiv |
| 088 | _ | _ | |a APS/123-QED |2 Other |
| 100 | 1 | _ | |a Capdevilla, Rodolfo |0 0000-0002-0122-7704 |b 0 |
| 245 | _ | _ | |a Discovering Electroweak Interacting Dark Matter at Muon Colliders Using Soft Tracks |
| 260 | _ | _ | |a College Park, Md. |c 2025 |b APS |
| 336 | 7 | _ | |a article |2 DRIVER |
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| 336 | 7 | _ | |a ARTICLE |2 BibTeX |
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| 336 | 7 | _ | |a Journal Article |0 0 |2 EndNote |
| 500 | _ | _ | |a 4 pages, 1 Table, 5 Figures |
| 520 | _ | _ | |a Minimal Dark Matter models feature one neutral particle that serves as a thermal relic dark matter candidate, as well as quasi-degenerate charged states with TeV masses. When the charged states are produced at colliders, they can decay into dark matter and a low-momentum (soft) charged particle, which is challenging to reconstruct at hadron colliders. We demonstrate that a 3 TeV Muon Collider is capable of detecting these soft tracks, enabling the discovery of thermal Higgsinos and similar dark matter candidates which constitute highly motivated scenarios for future collider searches. |
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| 693 | _ | _ | |1 EXP:(DE-H253)MUON-20220801 |0 EXP:(DE-H253)MUON-20220801 |a Planned International Muon Collider Facility |x 0 |
| 700 | 1 | _ | |a Meloni, Federico |0 P:(DE-H253)PIP1083387 |b 1 |e Corresponding author |
| 700 | 1 | _ | |a Zurita, Jose |0 0000-0001-5710-3965 |b 2 |
| 773 | _ | _ | |a 10.1103/PhysRevLett.134.181802 |g Vol. 134, no. 18, p. 181802 |0 PERI:(DE-600)1472655-5 |n 18 |p 181802 |t Physical review letters |v 134 |y 2025 |x 0031-9007 |
| 787 | 0 | _ | |a Capdevilla, Rodolfo et.al. |d 2024 |i IsParent |0 PUBDB-2024-01706 |r FERMILAB-PUB-23-0832-T ; DESY-24-069 ; arXiv:2405.08858 ; APS/123-QED |t Discovering Electroweak Interacting Dark Matter at Muon Colliders using Soft Tracks |
| 856 | 4 | _ | |y OpenAccess |u https://bib-pubdb1.desy.de/record/627807/files/PhysRevLett.134.181802.pdf |
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