Loosely bound composite dark matter
Abstract We investigate loosely bound composite states made of dark matter, where the binding energy for constituent particles is considerably less than the constituent mass. We focus on models of nuclear and molecular dark matter, where constituents are separated by length scales larger than the inverse constituent mass, just like nuclei and atoms in the Standard Model. The cosmology, structure, and interactions at underground experiments are described. We find that loosely bound composites can have a very large cross section for scattering with nuclei that scales with nucleon number like ∼ A 4 . For some couplings, these composites produce extremely soft (≪ keV) individual atomic recoils while depositing a large amount of total recoil energy (≫ keV) in a single passage through a detector, implying an interesting new class of signatures for low threshold direct detection.
Authors
- Christopher V. Cappiello (ORCID: https://orcid.org/0000-0002-7466-9634)
- Javier F. Acevedo (ORCID: https://orcid.org/0000-0003-3666-0951)
- Gopolang Mohlabeng (ORCID: https://orcid.org/0000-0002-7482-2643)
- Joseph Bramante (ORCID: https://orcid.org/0000-0001-8905-1960)
- Yilda Boukhtouchen
- Narayani Tyagi (ORCID: https://orcid.org/0000-0003-3638-8046)
Institutions
- Simon Fraser University (CA)
- Perimeter Institute (CA)
- University of California, Irvine (US)
- Washington University in St. Louis (US)
- SLAC National Accelerator Laboratory (US)
- Arthur B. McDonald-Canadian Astroparticle Physics Research Institute (CA)
Publication Details
- Journal
- Journal of Cosmology and Astroparticle Physics
- Published
- 2025-03-01
- DOI
- https://doi.org/10.1088/1475-7516/2025/03/013
- Citations
- 2
- Primary Topic
- Dark Matter and Cosmic Phenomena
- Type
- article
- Field-Weighted Citation Impact
- 3.74