Stable bi-frequency spinor modes as Dark Matter candidates
arXiv:2501.04027 · doi:10.1007/JHEP10(2025)082
Abstract
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.
14 pages
References in corpus (9)
- Nonlinear topological photonics
- Sterile Neutrinos
- Neutron -- Mirror Neutron Oscillation: How Fast Might It Be?
- A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics
- Dark Matter: The Leptonic Connection
- More about neutron - mirror neutron oscillation
- Exotic Dark Spinor Fields
- Experimental Search for Neutron to Mirror Neutron Oscillations as an Explanation of the Neutron Lifetime Anomaly
- Neutron-Mirror-Neutron Oscillation and Neutron Star Cooling