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16–19 Nov 2026
Asia/Shanghai timezone

From a Dark Matter Detector to a Neutrino Observatory: Latest Results from XENONnT

17 Nov 2026, 17:45
20m

Speaker

可欣 刘(Tsinghua University)

Description

Large liquid xenon detectors developed for dark matter searches combine substantial target masses with excellent background control, offering a versatile platform for rare event physics. XENONnT’s exceptionally low background and low energy threshold have enabled its emergence as an observatory for solar neutrinos. I will present recent measurements of elastic scattering of neutrinos on electrons and coherent elastic scattering of neutrinos on nuclei, probing solar pp and $^8B$ neutrinos through complementary electronic and nuclear recoil channels. These results open new opportunities for precision electroweak and neutrino physics, while informing the development of future geoneutrino detection strategies.

Primary author

可欣 刘(Tsinghua University)

Presentation materials

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