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Energy resolution and linearity of XENON1T in the MeV energy range

AbstractXenon dual-phase time projection chambers designed to search for weakly interacting massive particles have so far shown a relative energy resolution which degrades with energy above $$\sim $$∼ 200 keV due to the saturation effects. This has limited their sensitivity in the search for rare events like the neutrinoless double-beta decay of $$^{136} \hbox {Xe}$$136Xe at its Q value, $$Q_{\beta \beta }\simeq 2.46\,\hbox {MeV}$$Qββ≃2.46MeV. For the XENON1T dual-phase time projection chamber, we demonstrate that the relative energy resolution at $$1\,\sigma /\mu $$1σ/μ is as low as ($$0.80 \pm 0.02$$0.80±0.02) % in its one-ton fiducial mass, and for single-site interactions at $$Q_{\beta \beta }$$Qββ. We also present a new signal correction method to rectify the saturation effects of the signal readout system, resulting in more accurate position reconstruction and indirectly improving the energy resolution. The very good result achieved in XENON1T opens up new windows for the xenon dual-phase dark matter detectors to simultaneously search for other rare events.
- Sorbonne Paris Cité France
- UNIVERSITE PARIS DESCARTES France
- Kavli Institute for the Physics and Mathematics of the Universe Japan
- University of Zurich Switzerland
- Purdue University West Lafayette United States
Physics - Instrumentation and Detectors, [PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex], measurement methods, energy resolution, 115, FOS: Physical sciences, QC770-798, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], Astrophysics, 530, energy dependence, High Energy Physics - Experiment, XENON, High Energy Physics - Experiment (hep-ex), Dark Matter, Direct Detection, Xenon, double-beta decay: (0neutrino), Nuclear and particle physics. Atomic energy. Radioactivity, 539, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear Experiment (nucl-ex), Nuclear Experiment, Instrumentation and Methods for Astrophysics (astro-ph.IM), wimp, dark matter, liquid xenon, time projection chamber, direct detection, Instrumentation and Detectors (physics.ins-det), sensitivity, QB460-466, [PHYS.PHYS.PHYS-INS-DET] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], time projection chamber: xenon, Astrophysics - Instrumentation and Methods for Astrophysics, time projection chamber, weakly interacting massive particles, XENON1T
Physics - Instrumentation and Detectors, [PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex], measurement methods, energy resolution, 115, FOS: Physical sciences, QC770-798, [PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex], Astrophysics, 530, energy dependence, High Energy Physics - Experiment, XENON, High Energy Physics - Experiment (hep-ex), Dark Matter, Direct Detection, Xenon, double-beta decay: (0neutrino), Nuclear and particle physics. Atomic energy. Radioactivity, 539, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear Experiment (nucl-ex), Nuclear Experiment, Instrumentation and Methods for Astrophysics (astro-ph.IM), wimp, dark matter, liquid xenon, time projection chamber, direct detection, Instrumentation and Detectors (physics.ins-det), sensitivity, QB460-466, [PHYS.PHYS.PHYS-INS-DET] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], time projection chamber: xenon, Astrophysics - Instrumentation and Methods for Astrophysics, time projection chamber, weakly interacting massive particles, XENON1T
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