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PandaX-xT—A deep underground multi-ten-tonne liquid xenon observatory

  • PandaX Collaboration
  • School of Physics and Astronomy
  • Shanghai Jiao Tong University
  • Sun Yat-Sen University
  • Yantai University
  • Fudan University
  • Chinesen Academy of Sciences
  • Beihang University
  • Yalong River Hydropower Development Company, Ltd.
  • University of Maryland, College Park
  • University of Science and Technology of China
  • University of Science and Technology of China
  • Shandong University
  • Peking University
  • Nankai University
  • Shanghai Jiao Tong University

Research output: Contribution to journalArticlepeer-review

Abstract

We propose a major upgrade to the existing PandaX-4T experiment at the China Jinping Underground Laboratory. The new experiment, PandaX-xT, will be a multi-ten-tonne liquid xenon, ultra-low background, and general-purpose observatory. The full-scaled PandaX-xT contains a 43-t liquid xenon active target. Such an experiment will significantly advance our fundamental understanding of particle physics and astrophysics. The sensitivity of dark matter direct detection will be improved by nearly two orders of magnitude compared to the current best limits, approaching the so-called “neutrino floor” for a dark matter mass above 10 GeV/c2, providing a key test to the Weakly Interacting Massive Particle paradigm. By searching for the neutrinoless double beta decay of 136Xe isotope in the detector, the effective Majorana neutrino mass can be measured to a 10–41 meV/c2 sensitivity, providing a key test to the Dirac/Majorana nature of neutrinos. Astrophysical neutrinos and other ultra-rare interactions can also be measured and searched for with an unprecedented background level, opening up new windows of discovery. Depending on the findings, PandaX-xT will seek the next stage upgrade utilizing isotopic separation of natural xenon.

Original languageEnglish
Article number221011
JournalScience China: Physics, Mechanics and Astronomy
Volume68
Issue number2
DOIs
StatePublished - Feb 2025

Keywords

  • astrophysical neutrinos
  • dark matter
  • liquid xenon
  • neutrino less double beta decay

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