8–11 Oct 2024
Tsung-Dao Lee Institute
Asia/Shanghai timezone

Light neutrinophilic WIMP in the U(1)B−L model

8 Oct 2024, 14:30
30m
Tsung-Dao Lee Institute/N4F-N400 - meeting room (Tsung-Dao Lee Institute)

Tsung-Dao Lee Institute/N4F-N400 - meeting room

Tsung-Dao Lee Institute

70

Speaker

Yu Watanabe (IPMU)

Description

In light of the negative results from WIMP search experiments, attention has shifted toward light thermal DM. Moreover, light DM has the potential to address the core-cusp problem with its large self-scattering rate. However, such models may also predict a high annihilation rate, which could be constrained severely by gamma-ray telescopes. In our study, we explored the possibility of neutrinophilic DM within the U(1)B-L extension of the Standard Model. We conducted a phenomenological analysis of this model to identify viable parameter sets that explain the relic abundance via the freeze-out mechanism, resolve the core-cusp problem, and remain consistent with current observational constraints.

Primary author

Presentation materials