Stable bi-frequency spinor modes as Dark Matter candidates
A bstract We show that spinor systems with scalar self-interaction, such as the Dirac-Klein-Gordon system with Yukawa coupling or the Soler model, generically have bi-frequency solitary wave solutions. We develop the approach to stability properties of such waves and use the radial reduction to show that indeed the (linear) stability is available for a wide range of parameters. We show that only bi-frequency modes can be dynamically stable and suggest that stable bi-frequency modes can serve as storages of the Dark Matter. The approach is based on linear stability results of one-frequency solitary waves in (3+1)D Soler model, which we obtain as a by-product.
Authors
- N. R. Kulkarni (ORCID: https://orcid.org/0000-0001-7913-7074)
- Jesús Cuevas–Maraver (ORCID: https://orcid.org/0000-0002-7162-5759)
- Andrew Comech (ORCID: https://orcid.org/0000-0003-2112-9359)
- Nabile Boussaïd (ORCID: https://orcid.org/0000-0003-2858-2084)
Institutions
- Mitchell Institute (US)
- Institut UTINAM (FR)
- Université Marie et Louis Pasteur (FR)
- Universidad de Sevilla (ES)
- Texas A&M University (US)
Publication Details
- Journal
- Journal of High Energy Physics
- Published
- 2025-10-10
- DOI
- https://doi.org/10.1007/jhep10(2025)082
- Citations
- 1
- Primary Topic
- Advanced Mathematical Physics Problems
- Type
- article
- Field-Weighted Citation Impact
- 3.69
Funders
- Agence Nationale de la Recherche
- Agencia Estatal de Investigación