7–13 Sept 2025
Hermitage Hotel, Isola D'Elba
Europe/Rome timezone

Probing GeV-Scale Dark Matter Annihilation with the JUNO Experiment

12 Sept 2025, 18:00
30m
Hermitage Hotel, Isola D'Elba

Hermitage Hotel, Isola D'Elba

57037 Portoferraio Isola d’Elba (Li) Italy
Talk Dark Matter (Its nature: Theory, Observations, Detection, Production at accelerators) Afternoon session

Speaker

Utane Sawangwit (National Astronomical Research Institute of Thailand (NARIT))

Description

The Jiangmen Underground Neutrino Observatory (JUNO) is poised to make significant contributions to neutrino physics, including the indirect search for dark matter from the annihilation of WIMPs with masses in the GeV range, which can become gravitationally trapped within the solar core. While Pulse Shape Discrimination (PSD) is a standard technique for classifying events in JUNO , this work demonstrates that a substantial improvement in sensitivity can be achieved by applying dedicated machine learning (ML) and deep learning (DL) algorithms. This enhanced signal-to-background discrimination JUNO can become a leading instrument in the search for solar WIMPs, with a projected sensitivity that is comparable to current limits from major facilities like the IceCube Neutrino Observatory, particularly in the challenging low-mass WIMP range (3-20 GeV). This work highlights JUNO's strong potential to probe the existence of dark matter and its important role in the global multi-messenger effort.

References https://doi.org/10.1016/j.ppnp.2021.103927 , Angel Abusleme et al JCAP09 (2023) 001, J Siripak et al 2023 J. Phys.: Conf. Ser. 2431 012094

Author

Utane Sawangwit (National Astronomical Research Institute of Thailand (NARIT))

Co-authors

JUNO Collaboration Ms Jaruchit Siripak (Suranaree University of Technology, Thailand)

Presentation materials