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Mongillo M, Abdullahi A, Banto Oberhauser B, Crivelli P, Hostert M, Massaro D, Molina Bueno L, Pascoli S. Constraining light thermal inelastic dark matter with NA64. THE EUROPEAN PHYSICAL JOURNAL. C, PARTICLES AND FIELDS 2023; 83:391. [PMID: 37180830 PMCID: PMC10172231 DOI: 10.1140/epjc/s10052-023-11536-5] [Citation(s) in RCA: 1] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Grants] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 03/09/2023] [Accepted: 04/18/2023] [Indexed: 05/16/2023]
Abstract
A vector portal between the Standard Model and the dark sector is a predictive and compelling framework for thermal dark matter. Through co-annihilations, models of inelastic dark matter (iDM) and inelastic Dirac dark matter (i2DM) can reproduce the observed relic density in the MeV to GeV mass range without violating cosmological limits. In these scenarios, the vector mediator behaves like a semi-visible particle, evading traditional bounds on visible or invisible resonances, and uncovering new parameter space to explain the muon ( g - 2 ) anomaly. By means of a more inclusive signal definition at the NA64 experiment, we place new constraints on iDM and i2DM using a missing energy technique. With a recast-based analysis, we contextualize the NA64 exclusion limits in parameter space and estimate the reach of the newly collected and expected future NA64 data. Our results motivate the development of an optimized search program for semi-visible particles, in which fixed-target experiments like NA64 provide a powerful probe in the sub-GeV mass range.
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Affiliation(s)
- Martina Mongillo
- Institute for Particle Physics and Astrophysics, ETH Zürich, 8093 Zurich, Switzerland
| | - Asli Abdullahi
- Theoretical Physics Department, Fermi National Accelerator Laboratory, Batavia, IL 60510 USA
- Department of Physics, Institute for Particle Physics Phenomenology, Durham University, South Road, Durham, DH1 3LE UK
| | | | - Paolo Crivelli
- Institute for Particle Physics and Astrophysics, ETH Zürich, 8093 Zurich, Switzerland
| | - Matheus Hostert
- Perimeter Institute for Theoretical Physics, Waterloo, ON, N2J 2W9 Canada
- School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455 USA
- William I. Fine Theoretical Physics Institute, School of Physics and Astronomy, University of Minnesota, Minneapolis, MN, 55455 USA
| | - Daniele Massaro
- Dipartimento di Fisica e Astronomia, Università di Bologna, Via Irnerio 46, 40126 Bologna, Italy
- INFN, Sezione di Bologna, viale Berti Pichat 6/2, 40127 Bologna, Italy
- Centre for Cosmology, Particle Physics and Phenomenology (CP3), Université Catholique de Louvain, 1348 Louvain-la-Neuve, Belgium
| | - Laura Molina Bueno
- Instituto de Fisica Corpuscular (CSIC/UV), Carrer del Catedrátic José Beltrán Martinez 2, 46980 Paterna, Valencia Spain
| | - Silvia Pascoli
- Dipartimento di Fisica e Astronomia, Università di Bologna, Via Irnerio 46, 40126 Bologna, Italy
- INFN, Sezione di Bologna, viale Berti Pichat 6/2, 40127 Bologna, Italy
- Theoretical Physics Department, CERN, Geneva, Switzerland
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Tsai YD, McGehee R, Murayama H. Resonant Self-Interacting Dark Matter from Dark QCD. PHYSICAL REVIEW LETTERS 2022; 128:172001. [PMID: 35570435 DOI: 10.1103/physrevlett.128.172001] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/02/2021] [Revised: 01/07/2022] [Accepted: 03/10/2022] [Indexed: 06/15/2023]
Abstract
We present new models utilizing QCD-like dark sectors to resolve small-scale structure problems. These models of resonant self-interacting dark matter in a dark sector with QCD are based on analogies to the meson spectra in standard model QCD. We introduce a simple model that realizes resonant self-interaction (analogous to the ϕ-K-K system) and thermal freeze-out, in which dark mesons are made of two light quarks. We also consider asymmetric dark matter composed of heavy and light dark quarks to realize a resonant self-interaction (analogous to the ϒ(4S)-B-B system) and discuss the experimental probes of both setups. Finally, we comment on the possible resonant self-interactions already built into SIMP and ELDER mechanisms while using lattice results to determine feasibility.
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Affiliation(s)
- Yu-Dai Tsai
- Department of Physics and Astronomy, University of California, Irvine, California 92697-4575, USA
- Fermilab, Fermi National Accelerator Laboratory, Batavia, Illinois 60510, USA
- University of Chicago, Kavli Institute for Cosmological Physics, Chicago, Illinois 60637, USA
| | - Robert McGehee
- Department of Physics, University of California, Berkeley, California 94720, USA
- Ernest Orlando Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
| | - Hitoshi Murayama
- Department of Physics, University of California, Berkeley, California 94720, USA
- Ernest Orlando Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
- Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa 277-8583, Japan
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