Projected WIMP sensitivity of the XENONnT dark matter experiment
XENONnT is a dark matter direct detection experiment, utilizing 5.9 t of instrumented liquid xenon, located at the INFN Laboratori Nazionali del Gran Sasso. In this work, we predict the experimental background and project the sensitivity of XENONnT to the detection of weakly interacting massive part...
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| Published in | Journal of cosmology and astroparticle physics Vol. 2020; no. 11; p. 31 |
|---|---|
| Main Authors | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
| Format | Journal Article |
| Language | English |
| Published |
Bristol
IOP Publishing
01.11.2020
Institute of Physics (IOP) |
| Subjects | |
| Online Access | Get full text |
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| Abstract | XENONnT is a dark matter direct detection experiment, utilizing 5.9 t of instrumented liquid xenon, located at the INFN Laboratori Nazionali del Gran Sasso. In this work, we predict the experimental background and project the sensitivity of XENONnT to the detection of weakly interacting massive particles (WIMPs). The expected average differential background rate in the energy region of interest, corresponding to (1, 13) keV and (4, 50) keV for electronic and nuclear recoils, amounts to 12.3 ± 0.6 (keV t y)
-1
and (2.2± 0.5)× 10
−3
(keV t y)
-1
, respectively, in a 4 t fiducial mass. We compute unified confidence intervals using the profile construction method, in order to ensure proper coverage. With the exposure goal of 20 t y, the expected sensitivity to spin-independent WIMP-nucleon interactions reaches a cross-section of 1.4×10
−48
cm
2
for a 50 GeV/c
2
mass WIMP at 90% confidence level, more than one order of magnitude beyond the current best limit, set by XENON1T . In addition, we show that for a 50 GeV/c
2
WIMP with cross-sections above 2.6×10
−48
cm
2
(5.0×10
−48
cm
2
) the median XENONnT discovery significance exceeds 3σ (5σ). The expected sensitivity to the spin-dependent WIMP coupling to neutrons (protons) reaches 2.2×10
−43
cm
2
(6.0×10
−42
cm
2
). |
|---|---|
| AbstractList | XENONnT is a dark matter direct detection experiment, utilizing 5.9 t of instrumented liquid xenon, located at the INFN Laboratori Nazionali del Gran Sasso. In this work, we predict the experimental background and project the sensitivity of XENONnT to the detection of weakly interacting massive particles (WIMPs). The expected average differential background rate in the energy region of interest, corresponding to (1, 13) keV and (4, 50) keV for electronic and nuclear recoils, amounts to 12.3 +/- 0.6 (keV t y)(-1) and (2.2 +/- 0.5) x 10(-3 )(keV t y)(-1), respectively, in a 4t fiducial mass. We compute unified confidence intervals using the profile construction method, in order to ensure proper coverage. With the exposure goal of 20 t y, the expected sensitivity to spin-independent WIMP-nucleon interactions reaches a cross-section of 1.4 x 10(-48) cm(2) for a 50 GeV/c(2) mass WIMP at 90% confidence level, more than one order of magnitude beyond the current best limit, set by XENON1T. In addition, we show that for a 50 GeV/c(2) WIMP with cross-sections above 2.6 x 10(-48) cm(2) (5.0 x 10(-48) cm(2)) the median XENONnT discovery significance exceeds 3 sigma (5 sigma). The expected sensitivity to the spin-dependent WIMP coupling to neutrons (protons) reaches 2.2 x 10(-43) cm(2) (6.0 x 10(-42) cm(2)). XENONnT is a dark matter direct detection experiment, utilizing 5.9 t of instrumented liquid xenon, located at the INFN Laboratori Nazionali del Gran Sasso. In this work, we predict the experimental background and project the sensitivity of XENONnT to the detection of weakly interacting massive particles (WIMPs). The expected average differential background rate in the energy region of interest, corresponding to (1, 13) keV and (4, 50) keV for electronic and nuclear recoils, amounts to 12.3±0.6 (keV t y)-1 and (2.2±0.5)×10−3 (keV t y)-1, respectively, in a 4 t fiducial mass. We compute unified confidence intervals using the profile construction method, in order to ensure proper coverage. With the exposure goal of 20 t y, the expected sensitivity to spin-independent WIMP-nucleon interactions reaches a cross-section of 1.4×10−48cm2 for a 50 GeV/c2 mass WIMP at 90% confidence level, more than one order of magnitude beyond the current best limit, set by XENON1T . In addition, we show that for a 50 GeV/c2 WIMP with cross-sections above 2.6×10−48cm2 (5.0×10−48cm2) the median XENONnT discovery significance exceeds 3σ (5σ). The expected sensitivity to the spin-dependent WIMP coupling to neutrons (protons) reaches 2.2×10−43cm2 (6.0×10−42cm2). XENONnT is a dark matter direct detection experiment, utilizing 5.9 t of instrumented liquid xenon, located at the INFN Laboratori Nazionali del Gran Sasso. In this work, we predict the experimental background and project the sensitivity of XENONnT to the detection of weakly interacting massive particles (WIMPs). The expected average differential background rate in the energy region of interest, corresponding to (1, 13) keV and (4, 50) keV for electronic and nuclear recoils, amounts to 12.3 ± 0.6 (keV t y) -1 and (2.2± 0.5)× 10 −3 (keV t y) -1 , respectively, in a 4 t fiducial mass. We compute unified confidence intervals using the profile construction method, in order to ensure proper coverage. With the exposure goal of 20 t y, the expected sensitivity to spin-independent WIMP-nucleon interactions reaches a cross-section of 1.4×10 −48 cm 2 for a 50 GeV/c 2 mass WIMP at 90% confidence level, more than one order of magnitude beyond the current best limit, set by XENON1T . In addition, we show that for a 50 GeV/c 2 WIMP with cross-sections above 2.6×10 −48 cm 2 (5.0×10 −48 cm 2 ) the median XENONnT discovery significance exceeds 3σ (5σ). The expected sensitivity to the spin-dependent WIMP coupling to neutrons (protons) reaches 2.2×10 −43 cm 2 (6.0×10 −42 cm 2 ). XENONnT is a dark matter direct detection experiment, utilizing 5.9 t of instrumented liquid xenon, located at the INFN Laboratori Nazionali del Gran Sasso. In this work, we predict the experimental background and project the sensitivity of XENONnT to the detection of weakly interacting massive particles (WIMPs). The expected average differential background rate in the energy region of interest, corresponding to (1, 13) keV and (4, 50) keV for electronic and nuclear recoils, amounts to 12.3 ± 0.6 (keV t y)-1 and (2.2± 0.5)× 10−3 (keV t y)-1, respectively, in a 4 t fiducial mass. We compute unified confidence intervals using the profile construction method, in order to ensure proper coverage. With the exposure goal of 20 t y, the expected sensitivity to spin-independent WIMP-nucleon interactions reaches a cross-section of 1.4×10−48 cm2 for a 50 GeV/c2 mass WIMP at 90% confidence level, more than one order of magnitude beyond the current best limit, set by XENON1T . In addition, we show that for a 50 GeV/c2 WIMP with cross-sections above 2.6×10−48 cm2 (5.0×10−48 cm2) the median XENONnT discovery significance exceeds 3σ (5σ). The expected sensitivity to the spin-dependent WIMP coupling to neutrons (protons) reaches 2.2×10−43 cm2 (6.0×10−42 cm2). |
| Author | Antochi, V.C. Clark, M. Aprile, E. Agostini, F. Bruenner, S. Kobayashi, M. Odgers, K. Molinario, A. Budnik, R. Elykov, A. Plante, G. Depoian, A. Long, J. Cichon, D. Mastroianni, S. Gaior, R. Pizzella, V. Lindemann, S. Undagoitia, T. Marrodán Oberlack, U. Coderre, D. Arneodo, F. Benabderrahmane, M.L. Eurin, G. Diglio, S. Aalbers, J. Howlett, J. Murra, M. Palacio, J. Decowski, M.P. Hils, C. Kato, N. Stefano, R. Di Berger, T. Manfredini, A. Naganoma, J. Pienaar, J. Brown, A. Koltman, G. Landsman, H. Capelli, C. Althueser, L. Miuchi, K. Ferella, A.D. Masson, D. Cimmino, B. Manenti, L. Masbou, J. García, D. Ramírez Barge, D. Messina, M. Fulgione, W. Lopes, J.A.M. Qiu, H. Lindner, M. Alfonsi, M. Hasterok, C. Macolino, C. Mizukoshi, K. Hiraide, K. Marignetti, F. Cussonneau, J.P. Mosbacher, Y. Cardoso, J.M.R. Giovanni, A. Di Fune, E. López Moriyama, S. Colijn, A.P. Galloway, M. Lombardi, F. Bauermeister, B. Gaemers, P. Gao, F. Mahlstedt, J. Kopec, A. Conrad, J. Bruno, G. Itow, Y. Kazama, S. Mancuso, A. Grandi, L. Lin, Q. Amaro, F.D. Gangi, P. Di Angelino, E. Lang, R.F. Levinson |
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| Keywords | data analysis method dark matter: direct detection nucleus: recoil background activity report XENON WIMP: dark matter WIMP nucleon: scattering electron: recoil xenon: liquid sensitivity |
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| Snippet | XENONnT is a dark matter direct detection experiment, utilizing 5.9 t of instrumented liquid xenon, located at the INFN Laboratori Nazionali del Gran Sasso. In... |
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| SubjectTerms | Astrophysics Confidence intervals Cross-sections Dark matter dark matter experiments dark matter simulations High Energy Physics - Experiment Instrumentation and Detectors Physics Sensitivity Statistical analysis Weakly interacting massive particles Xenon |
| Title | Projected WIMP sensitivity of the XENONnT dark matter experiment |
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