Astrophysical neutrinos in Hyper-Kamiokande

被引：0
|
作者：
Bravo-Berguno, D. [1 ]
机构：
[1] Univ Autonoma Madrid UAM, Madrid, Spain
来源：
EUROPEAN PHYSICAL SOCIETY CONFERENCE ON HIGH ENERGY PHYSICS, EPS-HEP2019 | 2020年
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D O I：
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中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
Hyper-Kamiokande is a proposed next-generation underground large water-Cherenkov detector with a 187kton target volume of water and 40% photo coverage.With about 10 times larger fiducial volume than Super-Kamiokande, the sensitivities for astrophysical neutrinos, like solar or supernova neutrinos, but also contributions to multimessenger astronomy and dark matter searches, will be greatly improved in HyperK. The physics potential of HyperK on astrophysical neutrinos and its expected performance will be discussed.
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页数：7
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