Atomki anomaly and the Secluded Dark Sector
arXiv:1708.09756 · doi:10.1051/epjconf/201816806007
Abstract
The Atomiki anomaly can be interpreted as a new light vector boson. If such a new particle exists, it could be a mediator between the Standard Model sector and the dark sector including the dark matter. We discussed some simple effective models with these particles. In the models, the secluded dark matter models are good candidates to satisfy the thermal relic abundance. In particular, we found that the dark matter self-interaction can be large enough to solve the small scale structure puzzles if the dark matter is a fermion.
5 pages, 4 figures, etc.; contribution to the proceedings of Joint Conference of ICGAC-XIII and IK15, Seoul, 3-7 July 2017; based on 1609.01605
References in corpus (8)
- Results from a search for dark matter in the complete LUX exposure
- Secluded WIMP Dark Matter
- Beyond Collisionless Dark Matter: Particle Physics Dynamics for Dark Matter Halo Structure
- Observation of Anomalous Internal Pair Creation in Be: A Possible Signature of a Light, Neutral Boson
- Protophobic Fifth Force Interpretation of the Observed Anomaly in Be Nuclear Transitions
- Particle Physics Models for the 17 MeV Anomaly in Beryllium Nuclear Decays
- Protophobic Light Vector Boson as a Mediator to the Dark Sector
- The new interaction suggested by the anomalous Be transition sets a rigorous constraint on the mass range of dark matter
Cited by in corpus (5)
- Neutrinos from captured dark matter annihilation in a galactic population of neutron stars
- Solar constraints on captured electrophilic dark matter
- Probing the Dark Matter Capture Rate in a Local Population of Brown Dwarfs with IceCube Gen 2
- Confronting the dark matter capture rate with a continuous gravitational wave probe of local neutron stars
- Can local White Dwarfs constrain Dark Matter interactions?