Positronium Decays with Dark and Fermionic Dark Matter
arXiv:2111.10949 · doi:10.1103/PhysRevD.105.095023
Abstract
We investigate the invisible decay of positronium to probe the fermionic light dark matter mediated by the dark boson. Too tiny is the invisible decay rate of positronium through weak interaction in the standard model to be detected in the experiment. We show that it can be enhanced to be observed in the future if the dark matter is lighter than the electron in the dark model. We also compute the relic abundance of such light dark matter and discuss the Big Bang Nucleosynthesis constraint with an alternative thermal history scenario.
8 pages, 4 figures
References in corpus (8)
- Constraints on the Self-Interaction Cross-Section of Dark Matter from Numerical Simulations of the Merging Galaxy Cluster 1E 0657-5
- Search for dark matter annihilations towards the inner Galactic halo from 10 years of observations with H.E.S.S
- Refined Bounds on MeV-scale Thermal Dark Sectors from BBN and the CMB
- An Improved Limit on Invisible Decays of Positronium
- Singlet fermionic dark matter
- The minimal model of fermionic dark matter
- Two-loop corrections to the parameter in Two-Higgs-Doublet Models
- Confronting Dirac Fermionic Dark Matter with Recent Data