28 August 2023 to 1 September 2023
University of Vienna
Europe/Vienna timezone

A New Method for Detecting Charged-Current Neutrino Interactions on 136Xe in KamLAND-Zen: Implications for Solar Neutrino Measurements and Fermionic Dark Matter Searches

30 Aug 2023, 15:30
1h
University of Vienna

University of Vienna

Universitätsring 1 A-1010 Vienna, Austria
Poster Neutrino physics and astrophysics Poster session

Speaker

Mr Koga Tachibana (RCNS, Tohoku University)

Description

136Xe nuclei capture electron neutrinos through charged-current (CC) interactions, leading to the excited states of 136Cs: (ν_e + 136Xe → e^- + 136Cs*). This process can be used for solar neutrino measurements and fermionic dark matter searches.

The recent observation of low-lying isomeric states in 136Cs* with lifetimes on the order of 100 ns [1] implies that the CC interaction can be identified by a delayed coincidence measurement. This technique involves detecting a prompt signal consisting of the electron and most of the de-excitation gamma rays, followed by a delayed signal consisting of the remaining de-excitation gamma rays with energies below 140 keV.

KamLAND-Zen is an experiment designed to search for the neutrinoless double beta decay of 136Xe, using an organic liquid scintillator that dissolves 750 kg of xenon gas (91% enriched in 136Xe). This presentation will discuss the feasibility of identifying the CC interaction in KamLAND-Zen.

References
[1] S.J. Haselschwardt et. al, arXiv:2301.11893 (2023).

Submitted on behalf of a Collaboration? No

Authors

Mr Koga Tachibana (RCNS, Tohoku University) Dr Takahiko Hachiya (Research Center for Neutrino Science (RCNS), Tohoku university)

Co-author

KamLAND-Zen collaboration

Presentation materials