Search for inelastic scattering of WIMP dark matter in XENON1T

E. Aprile; J. Aalbers; F. Agostini; M. Alfonsi; L. Althueser; F. D. Amaro; S. Andaloro; E. Angelino; J. R. Angevaare; V. C. Antochi; F. Arneodo; L. Baudis; B. Bauermeister; L. Bellagamba; M. L. Benabderrahmane; A. Brown; E. Brown; S. Bruenner; G. Bruno; R. Budnik; C. Capelli; J. M.R. Cardoso; D. Cichon; B. Cimmino; M. Clark; D. Coderre; A. P. Colijn; J. Conrad; J. Cuenca; J. P. Cussonneau; M. P. Decowski; A. Depoian; P. Di Gangi; A. Di Giovanni; R. Di Stefano; S. Diglio; A. Elykov; A. D. Ferella; W. Fulgione; P. Gaemers; R. Gaior; M. Galloway; F. Gao; L. Grandi; C. Hils; K. Hiraide; L. Hoetzsch; J. Howlett; M. Iacovacci; Y. Itow; F. Joerg; N. Kato; S. Kazama; M. Kobayashi; G. Koltman; A. Kopec; H. Landsman; R. F. Lang; L. Levinson; S. Liang; Q. Lin; S. Lindemann; M. Lindner; F. Lombardi; J. Long; J. A.M. Lopes; Y. Ma; C. Macolino; J. Mahlstedt; A. Mancuso; L. Manenti; A. Manfredini; F. Marignetti; T. Marrodan Undagoitia; K. Martens; J. Masbou; D. Masson; S. Mastroianni; M. Messina; K. Miuchi; K. Mizukoshi; A. Molinario; K. Morå; S. Moriyama; Y. Mosbacher; M. Murra; J. Naganoma; K. Ni; U. Oberlack; K. Odgers; J. Palacio; B. Pelssers; R. Peres; J. Pienaar; M. Pierre; V. Pizzella; G. Plante; J. Qi; J. Qin; D. Ramírez Garciá; S. Reichard; A. Rocchetti; N. Rupp; J. M.F. Dos Santos; G. Sartorelli; N. Sarcević; M. Scheibelhut; J. Schreiner; D. Schulte; H. Schulze Eißing; M. Schumann; L. Scotto Lavina; M. Selvi; F. Semeria; P. Shagin; E. Shockley; M. Silva; H. Simgen; A. Takeda; C. Therreau; D. Thers; F. Toschi; G. Trinchero; C. Tunnell; K. Valerius; M. Vargas; G. Volta; Y. Wei; C. Weinheimer; M. Weiss; D. Wenz; C. Wittweg; T. Wolf; Z. Xu; M. Yamashita; J. Ye; G. Zavattini; Y. Zhang; T. Zhu; J. P. Zopounidis

doi:10.1103/PhysRevD.103.063028

Search for inelastic scattering of WIMP dark matter in XENON1T

E. Aprile, J. Aalbers, F. Agostini, M. Alfonsi, L. Althueser, F. D. Amaro, S. Andaloro, E. Angelino, J. R. Angevaare, V. C. Antochi, F. Arneodo, L. Baudis, B. Bauermeister, L. Bellagamba, M. L. Benabderrahmane, A. Brown, E. Brown, S. Bruenner, G. Bruno, R. BudnikC. Capelli, J. M.R. Cardoso, D. Cichon, B. Cimmino, M. Clark, D. Coderre, A. P. Colijn, J. Conrad, J. Cuenca, J. P. Cussonneau, M. P. Decowski, A. Depoian, P. Di Gangi, A. Di Giovanni, R. Di Stefano, S. Diglio, A. Elykov, A. D. Ferella, W. Fulgione, P. Gaemers, R. Gaior, M. Galloway, F. Gao, L. Grandi, C. Hils, K. Hiraide, L. Hoetzsch, J. Howlett, M. Iacovacci, Y. Itow, F. Joerg, N. Kato, S. Kazama, M. Kobayashi, G. Koltman, A. Kopec, H. Landsman, R. F. Lang, L. Levinson, S. Liang, Q. Lin, S. Lindemann, M. Lindner, F. Lombardi, J. Long, J. A.M. Lopes, Y. Ma, C. Macolino, J. Mahlstedt, A. Mancuso, L. Manenti, A. Manfredini, F. Marignetti, T. Marrodan Undagoitia, K. Martens, J. Masbou, D. Masson, S. Mastroianni, M. Messina, K. Miuchi, K. Mizukoshi, A. Molinario, K. Morå, S. Moriyama, Y. Mosbacher, M. Murra, J. Naganoma, K. Ni, U. Oberlack, K. Odgers, J. Palacio, B. Pelssers, R. Peres, J. Pienaar, M. Pierre, V. Pizzella, G. Plante, J. Qi, J. Qin, D. Ramírez Garciá, S. Reichard, A. Rocchetti, N. Rupp, J. M.F. Dos Santos, G. Sartorelli, N. Sarcević, M. Scheibelhut, J. Schreiner, D. Schulte, H. Schulze Eißing, M. Schumann, L. Scotto Lavina, M. Selvi, F. Semeria, P. Shagin, E. Shockley, M. Silva, H. Simgen, A. Takeda, C. Therreau, D. Thers, F. Toschi, G. Trinchero, C. Tunnell, K. Valerius, M. Vargas, G. Volta, Y. Wei, C. Weinheimer, M. Weiss, D. Wenz, C. Wittweg, T. Wolf, Z. Xu, M. Yamashita, J. Ye, G. Zavattini, Y. Zhang, T. Zhu, J. P. Zopounidis

Physics

Research output: Contribution to journal › Article › peer-review

Abstract

We report the results of a search for the inelastic scattering of weakly interacting massive particles (WIMPs) in the XENON1T dark matter experiment. Scattering off Xe129 is the most sensitive probe of inelastic WIMP interactions, with a signature of a 39.6 keV deexcitation photon detected simultaneously with the nuclear recoil. Using an exposure of 0.83 tonne-years, we find no evidence of inelastic WIMP scattering with a significance of more than 2σ. A profile-likelihood ratio analysis is used to set upper limits on the cross section of WIMP-nucleus interactions. We exclude new parameter space for WIMPs heavier than 100 GeV/c2, with the strongest upper limit of 3.3×10-39 cm2 for 130 GeV/c2 WIMPs at 90% confidence level.

Original language	English (US)
Article number	063028
Journal	Physical Review D
Volume	103
Issue number	6
DOIs	https://doi.org/10.1103/PhysRevD.103.063028
State	Published - Mar 19 2021

ASJC Scopus subject areas

Nuclear and High Energy Physics

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10.1103/PhysRevD.103.063028

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Aprile, E., Aalbers, J., Agostini, F., Alfonsi, M., Althueser, L., Amaro, F. D., Andaloro, S., Angelino, E., Angevaare, J. R., Antochi, V. C., Arneodo, F., Baudis, L., Bauermeister, B., Bellagamba, L., Benabderrahmane, M. L., Brown, A., Brown, E., Bruenner, S., Bruno, G., ... Zopounidis, J. P. (2021). Search for inelastic scattering of WIMP dark matter in XENON1T. Physical Review D, 103(6), Article 063028. https://doi.org/10.1103/PhysRevD.103.063028

Aprile, E, Aalbers, J, Agostini, F, Alfonsi, M, Althueser, L, Amaro, FD, Andaloro, S, Angelino, E, Angevaare, JR, Antochi, VC, Arneodo, F, Baudis, L, Bauermeister, B, Bellagamba, L, Benabderrahmane, ML, Brown, A, Brown, E, Bruenner, S, Bruno, G, Budnik, R, Capelli, C, Cardoso, JMR, Cichon, D, Cimmino, B, Clark, M, Coderre, D, Colijn, AP, Conrad, J, Cuenca, J, Cussonneau, JP, Decowski, MP, Depoian, A, Di Gangi, P, Di Giovanni, A, Di Stefano, R, Diglio, S, Elykov, A, Ferella, AD, Fulgione, W, Gaemers, P, Gaior, R, Galloway, M, Gao, F, Grandi, L, Hils, C, Hiraide, K, Hoetzsch, L, Howlett, J, Iacovacci, M, Itow, Y, Joerg, F, Kato, N, Kazama, S, Kobayashi, M, Koltman, G, Kopec, A, Landsman, H, Lang, RF, Levinson, L, Liang, S, Lin, Q, Lindemann, S, Lindner, M, Lombardi, F, Long, J, Lopes, JAM, Ma, Y, Macolino, C, Mahlstedt, J, Mancuso, A, Manenti, L, Manfredini, A, Marignetti, F, Marrodan Undagoitia, T, Martens, K, Masbou, J, Masson, D, Mastroianni, S, Messina, M, Miuchi, K, Mizukoshi, K, Molinario, A, Morå, K, Moriyama, S, Mosbacher, Y, Murra, M, Naganoma, J, Ni, K, Oberlack, U, Odgers, K, Palacio, J, Pelssers, B, Peres, R, Pienaar, J, Pierre, M, Pizzella, V, Plante, G, Qi, J, Qin, J, Ramírez Garciá, D, Reichard, S, Rocchetti, A, Rupp, N, Dos Santos, JMF, Sartorelli, G, Sarcević, N, Scheibelhut, M, Schreiner, J, Schulte, D, Schulze Eißing, H, Schumann, M, Scotto Lavina, L, Selvi, M, Semeria, F, Shagin, P, Shockley, E, Silva, M, Simgen, H, Takeda, A, Therreau, C, Thers, D, Toschi, F, Trinchero, G, Tunnell, C, Valerius, K, Vargas, M, Volta, G, Wei, Y, Weinheimer, C, Weiss, M, Wenz, D, Wittweg, C, Wolf, T, Xu, Z, Yamashita, M, Ye, J, Zavattini, G, Zhang, Y, Zhu, T & Zopounidis, JP 2021, 'Search for inelastic scattering of WIMP dark matter in XENON1T', Physical Review D, vol. 103, no. 6, 063028. https://doi.org/10.1103/PhysRevD.103.063028

@article{47bb8eee3a694104996e7a8487d6e683,

title = "Search for inelastic scattering of WIMP dark matter in XENON1T",

abstract = "We report the results of a search for the inelastic scattering of weakly interacting massive particles (WIMPs) in the XENON1T dark matter experiment. Scattering off Xe129 is the most sensitive probe of inelastic WIMP interactions, with a signature of a 39.6 keV deexcitation photon detected simultaneously with the nuclear recoil. Using an exposure of 0.83 tonne-years, we find no evidence of inelastic WIMP scattering with a significance of more than 2σ. A profile-likelihood ratio analysis is used to set upper limits on the cross section of WIMP-nucleus interactions. We exclude new parameter space for WIMPs heavier than 100 GeV/c2, with the strongest upper limit of 3.3×10-39 cm2 for 130 GeV/c2 WIMPs at 90% confidence level.",

author = "E. Aprile and J. Aalbers and F. Agostini and M. Alfonsi and L. Althueser and Amaro, {F. D.} and S. Andaloro and E. Angelino and Angevaare, {J. R.} and Antochi, {V. C.} and F. Arneodo and L. Baudis and B. Bauermeister and L. Bellagamba and Benabderrahmane, {M. L.} and A. Brown and E. Brown and S. Bruenner and G. Bruno and R. Budnik and C. Capelli and Cardoso, {J. M.R.} and D. Cichon and B. Cimmino and M. Clark and D. Coderre and Colijn, {A. P.} and J. Conrad and J. Cuenca and Cussonneau, {J. P.} and Decowski, {M. P.} and A. Depoian and {Di Gangi}, P. and {Di Giovanni}, A. and {Di Stefano}, R. and S. Diglio and A. Elykov and Ferella, {A. D.} and W. Fulgione and P. Gaemers and R. Gaior and M. Galloway and F. Gao and L. Grandi and C. Hils and K. Hiraide and L. Hoetzsch and J. Howlett and M. Iacovacci and Y. Itow and F. Joerg and N. Kato and S. Kazama and M. Kobayashi and G. Koltman and A. Kopec and H. Landsman and Lang, {R. F.} and L. Levinson and S. Liang and Q. Lin and S. Lindemann and M. Lindner and F. Lombardi and J. Long and Lopes, {J. A.M.} and Y. Ma and C. Macolino and J. Mahlstedt and A. Mancuso and L. Manenti and A. Manfredini and F. Marignetti and {Marrodan Undagoitia}, T. and K. Martens and J. Masbou and D. Masson and S. Mastroianni and M. Messina and K. Miuchi and K. Mizukoshi and A. Molinario and K. Mor{\aa} and S. Moriyama and Y. Mosbacher and M. Murra and J. Naganoma and K. Ni and U. Oberlack and K. Odgers and J. Palacio and B. Pelssers and R. Peres and J. Pienaar and M. Pierre and V. Pizzella and G. Plante and J. Qi and J. Qin and {Ram{\'i}rez Garci{\'a}}, D. and S. Reichard and A. Rocchetti and N. Rupp and {Dos Santos}, {J. M.F.} and G. Sartorelli and N. Sarcevi{\'c} and M. Scheibelhut and J. Schreiner and D. Schulte and {Schulze Ei{\ss}ing}, H. and M. Schumann and {Scotto Lavina}, L. and M. Selvi and F. Semeria and P. Shagin and E. Shockley and M. Silva and H. Simgen and A. Takeda and C. Therreau and D. Thers and F. Toschi and G. Trinchero and C. Tunnell and K. Valerius and M. Vargas and G. Volta and Y. Wei and C. Weinheimer and M. Weiss and D. Wenz and C. Wittweg and T. Wolf and Z. Xu and M. Yamashita and J. Ye and G. Zavattini and Y. Zhang and T. Zhu and Zopounidis, {J. P.}",

note = "Funding Information: We gratefully acknowledge support from the National Science Foundation, Swiss National Science Foundation, German Ministry for Education and Research, Max Planck Gesellschaft, Deutsche Forschungsgemeinschaft, Helmholtz Association, Netherlands Organisation for Scientific Research (NWO), Weizmann Institute of Science, ISF, Fundacao para a Ciencia e a Tecnologia, R{\'e}gion des Pays de la Loire, Knut and Alice Wallenberg Foundation, Kavli Foundation, JSPS Kakenhi in Japan, and Istituto Nazionale di Fisica Nucleare. This project received funding or support from the European Unions Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie Grants No. 690575 and No. 674896, respectively. Data processing was performed using infrastructures from the Open Science Grid, the European Grid Initiative and the Dutch national e-infrastructure with the support of SURF Cooperative. We are grateful to Laboratori Nazionali del Gran Sasso for hosting and supporting the XENON project. Publisher Copyright: {\textcopyright} 2021 authors. Published by the American Physical Society.",

year = "2021",

month = mar,

day = "19",

doi = "10.1103/PhysRevD.103.063028",

language = "English (US)",

volume = "103",

journal = "Physical Review D",

issn = "2470-0010",

publisher = "American Physical Society",

number = "6",

}

TY - JOUR

T1 - Search for inelastic scattering of WIMP dark matter in XENON1T

AU - Aprile, E.

AU - Aalbers, J.

AU - Agostini, F.

AU - Alfonsi, M.

AU - Althueser, L.

AU - Amaro, F. D.

AU - Andaloro, S.

AU - Angelino, E.

AU - Angevaare, J. R.

AU - Antochi, V. C.

AU - Arneodo, F.

AU - Baudis, L.

AU - Bauermeister, B.

AU - Bellagamba, L.

AU - Benabderrahmane, M. L.

AU - Brown, A.

AU - Brown, E.

AU - Bruenner, S.

AU - Bruno, G.

AU - Budnik, R.

AU - Capelli, C.

AU - Cardoso, J. M.R.

AU - Cichon, D.

AU - Cimmino, B.

AU - Clark, M.

AU - Coderre, D.

AU - Colijn, A. P.

AU - Conrad, J.

AU - Cuenca, J.

AU - Cussonneau, J. P.

AU - Decowski, M. P.

AU - Depoian, A.

AU - Di Gangi, P.

AU - Di Giovanni, A.

AU - Di Stefano, R.

AU - Diglio, S.

AU - Elykov, A.

AU - Ferella, A. D.

AU - Fulgione, W.

AU - Gaemers, P.

AU - Gaior, R.

AU - Galloway, M.

AU - Gao, F.

AU - Grandi, L.

AU - Hils, C.

AU - Hiraide, K.

AU - Hoetzsch, L.

AU - Howlett, J.

AU - Iacovacci, M.

AU - Itow, Y.

AU - Joerg, F.

AU - Kato, N.

AU - Kazama, S.

AU - Kobayashi, M.

AU - Koltman, G.

AU - Kopec, A.

AU - Landsman, H.

AU - Lang, R. F.

AU - Levinson, L.

AU - Liang, S.

AU - Lin, Q.

AU - Lindemann, S.

AU - Lindner, M.

AU - Lombardi, F.

AU - Long, J.

AU - Lopes, J. A.M.

AU - Ma, Y.

AU - Macolino, C.

AU - Mahlstedt, J.

AU - Mancuso, A.

AU - Manenti, L.

AU - Manfredini, A.

AU - Marignetti, F.

AU - Marrodan Undagoitia, T.

AU - Martens, K.

AU - Masbou, J.

AU - Masson, D.

AU - Mastroianni, S.

AU - Messina, M.

AU - Miuchi, K.

AU - Mizukoshi, K.

AU - Molinario, A.

AU - Morå, K.

AU - Moriyama, S.

AU - Mosbacher, Y.

AU - Murra, M.

AU - Naganoma, J.

AU - Ni, K.

AU - Oberlack, U.

AU - Odgers, K.

AU - Palacio, J.

AU - Pelssers, B.

AU - Peres, R.

AU - Pienaar, J.

AU - Pierre, M.

AU - Pizzella, V.

AU - Plante, G.

AU - Qi, J.

AU - Qin, J.

AU - Ramírez Garciá, D.

AU - Reichard, S.

AU - Rocchetti, A.

AU - Rupp, N.

AU - Dos Santos, J. M.F.

AU - Sartorelli, G.

AU - Sarcević, N.

AU - Scheibelhut, M.

AU - Schreiner, J.

AU - Schulte, D.

AU - Schulze Eißing, H.

AU - Schumann, M.

AU - Scotto Lavina, L.

AU - Selvi, M.

AU - Semeria, F.

AU - Shagin, P.

AU - Shockley, E.

AU - Silva, M.

AU - Simgen, H.

AU - Takeda, A.

AU - Therreau, C.

AU - Thers, D.

AU - Toschi, F.

AU - Trinchero, G.

AU - Tunnell, C.

AU - Valerius, K.

AU - Vargas, M.

AU - Volta, G.

AU - Wei, Y.

AU - Weinheimer, C.

AU - Weiss, M.

AU - Wenz, D.

AU - Wittweg, C.

AU - Wolf, T.

AU - Xu, Z.

AU - Yamashita, M.

AU - Ye, J.

AU - Zavattini, G.

AU - Zhang, Y.

AU - Zhu, T.

AU - Zopounidis, J. P.

N1 - Funding Information: We gratefully acknowledge support from the National Science Foundation, Swiss National Science Foundation, German Ministry for Education and Research, Max Planck Gesellschaft, Deutsche Forschungsgemeinschaft, Helmholtz Association, Netherlands Organisation for Scientific Research (NWO), Weizmann Institute of Science, ISF, Fundacao para a Ciencia e a Tecnologia, Région des Pays de la Loire, Knut and Alice Wallenberg Foundation, Kavli Foundation, JSPS Kakenhi in Japan, and Istituto Nazionale di Fisica Nucleare. This project received funding or support from the European Unions Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie Grants No. 690575 and No. 674896, respectively. Data processing was performed using infrastructures from the Open Science Grid, the European Grid Initiative and the Dutch national e-infrastructure with the support of SURF Cooperative. We are grateful to Laboratori Nazionali del Gran Sasso for hosting and supporting the XENON project. Publisher Copyright: © 2021 authors. Published by the American Physical Society.

PY - 2021/3/19

Y1 - 2021/3/19

N2 - We report the results of a search for the inelastic scattering of weakly interacting massive particles (WIMPs) in the XENON1T dark matter experiment. Scattering off Xe129 is the most sensitive probe of inelastic WIMP interactions, with a signature of a 39.6 keV deexcitation photon detected simultaneously with the nuclear recoil. Using an exposure of 0.83 tonne-years, we find no evidence of inelastic WIMP scattering with a significance of more than 2σ. A profile-likelihood ratio analysis is used to set upper limits on the cross section of WIMP-nucleus interactions. We exclude new parameter space for WIMPs heavier than 100 GeV/c2, with the strongest upper limit of 3.3×10-39 cm2 for 130 GeV/c2 WIMPs at 90% confidence level.

AB - We report the results of a search for the inelastic scattering of weakly interacting massive particles (WIMPs) in the XENON1T dark matter experiment. Scattering off Xe129 is the most sensitive probe of inelastic WIMP interactions, with a signature of a 39.6 keV deexcitation photon detected simultaneously with the nuclear recoil. Using an exposure of 0.83 tonne-years, we find no evidence of inelastic WIMP scattering with a significance of more than 2σ. A profile-likelihood ratio analysis is used to set upper limits on the cross section of WIMP-nucleus interactions. We exclude new parameter space for WIMPs heavier than 100 GeV/c2, with the strongest upper limit of 3.3×10-39 cm2 for 130 GeV/c2 WIMPs at 90% confidence level.

UR - http://www.scopus.com/inward/record.url?scp=85103081181&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85103081181&partnerID=8YFLogxK

U2 - 10.1103/PhysRevD.103.063028

DO - 10.1103/PhysRevD.103.063028

M3 - Article

AN - SCOPUS:85103081181

SN - 2470-0010

VL - 103

JO - Physical Review D

JF - Physical Review D

IS - 6

M1 - 063028

ER -

Search for inelastic scattering of WIMP dark matter in XENON1T

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