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- W3206774105 abstract "The current phase of the XENON Dark Matter Project, namedXENONnT, will be operative in 2020 in the underground Laboratori Nazionali delGran Sasso (LNGS). It is a multi-ton detector for direct search of Dark Matter,consisting of a double phase liquid-gas xenon Time Projection Chamber (TPC)which contains 5.9 tons of liquid xenon target mass, inserted in a cryostat surroundedby a tank containing 700 tons of water doped with Gd sulphate. Its aim, as that of itsprecursor XENON1T, is to detect elastic scattering of Weakly Interacting MassiveParticles (WIMPs) off xenon nuclei. The presence of two Veto sub-systems, themuon Veto instrumented with 84 photomultiplier tubes (PMTs) and the neutronVeto with other 120 PMTs, allows to reduce the background for WIMPs searchthrough muon and neutron tagging, while the presence of Gd sulphate increasesthe neutron capture cross section. Thanks to the large xenon target used and thepresence of the two Vetoes, XENONnT will be able also to detect all flavours ofSupernova neutrinos. Here the results from Monte Carlo simulations of XENONnTdetection efficiency are presented for Supernova neutrinos through their inverse betadecay interactions in water of the two Veto sub-systems." @default.
- W3206774105 created "2021-10-25" @default.
- W3206774105 creator A5081041375 @default.
- W3206774105 date "2020-01-01" @default.
- W3206774105 modified "2023-09-27" @default.
- W3206774105 title "Supernova neutrino detection in XENONnT neutron and muon Vetoes" @default.
- W3206774105 doi "https://doi.org/10.1393/ncc/i2020-20119-y" @default.
- W3206774105 hasPublicationYear "2020" @default.
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