Dark Matter Results from 225 Live Days of XENON100 Data

E. Aprile; M. Alfonsi; K. Arisaka; F. Arneodo; C. Balan; L. Baudis; B. Bauermeister; A. Behrens; P. Beltrame; K. Bokeloh; E. Brown; G. Bruno; R. Budnik; J. M. R. Cardoso; W.-t. Chen; B. Choi; D. Cline; A. P. Colijn; H. Contreras; J. P. Cussonneau; M. P. Decowski; E. Duchovni; S. Fattori; A. D. Ferella; W. Fulgione; F. Gao; M. Garbini; C. Ghag; K.-l. Giboni; L. W. Goetzke; C. Grignon; E. Gross; W. Hampel; F. Kaether; A. Kish; J. Lamblin; H. Landsman; R. F. Lang; M. Le Calloch; C. Levy; K. E. Lim; Q. Lin; S. Lindemann; M. Lindner; J. A. M. Lopes; K. Lung; T. Marrod??n Undagoitia; F. V. Massoli; A. J. Melgarejo Fernandez; Y. Meng; A. Molinario; E. Nativ; K. Ni; U. Oberlack; S. E. A. Orrigo; E. Pantic; R. Persiani; G. Plante; N. Priel; A. Rizzo; S. Rosendahl; J. M. F. Dos Santos; G. Sartorelli; J. Schreiner; M. Schumann; L. Scotto Lavina; P. R. Scovell; M. Selvi; P. Shagin; H. Simgen; A. Teymourian; D. Thers; O. Vitells; H. Wang; M. Weber; C. Weinheimer

doi:10.1103/PhysRevLett.109.181301

Dark Matter Results from 225 Live Days of XENON100 Data

E. Aprile, M. Alfonsi, K. Arisaka, F. Arneodo, C. Balan, L. Baudis, B. Bauermeister, A. Behrens, P. Beltrame, K. Bokeloh, E. Brown, G. Bruno, R. Budnik, J. M. R. Cardoso, W.-t. Chen, B. Choi, D. Cline, A. P. Colijn, H. Contreras, J. P. CussonneauM. P. Decowski, E. Duchovni, S. Fattori, A. D. Ferella, W. Fulgione, F. Gao, M. Garbini, C. Ghag, K.-l. Giboni, L. W. Goetzke, C. Grignon, E. Gross, W. Hampel, F. Kaether, A. Kish, J. Lamblin, H. Landsman, R. F. Lang, M. Le Calloch, C. Levy, K. E. Lim, Q. Lin, S. Lindemann, M. Lindner, J. A. M. Lopes, K. Lung, T. Marrod??n Undagoitia, F. V. Massoli, A. J. Melgarejo Fernandez, Y. Meng, A. Molinario, E. Nativ, K. Ni, U. Oberlack, S. E. A. Orrigo, E. Pantic, R. Persiani, G. Plante, N. Priel, A. Rizzo, S. Rosendahl, J. M. F. Dos Santos, G. Sartorelli, J. Schreiner, M. Schumann, L. Scotto Lavina, P. R. Scovell, M. Selvi, P. Shagin, H. Simgen, A. Teymourian, D. Thers, O. Vitells, H. Wang, M. Weber, C. Weinheimer

School of Physics and Astronomy

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Abstract / Description of output

We report on a search for particle dark matter with the XENON100 experiment, operated at the Laboratori Nazionali del Gran Sasso for 13 months during 2011 and 2012. XENON100 features an ultralow electromagnetic background of (5.3±0.6)×10-3 events/(keVee×kg×day) in the energy region of interest. A blind analysis of 224.6 live days×34 kg exposure has yielded no evidence for dark matter interactions. The two candidate events observed in the predefined nuclear recoil energy range of 6.6–30.5 keVnr are consistent with the background expectation of (1.0±0.2) events. A profile likelihood analysis using a 6.6–43.3 keVnr energy range sets the most stringent limit on the spin-independent elastic weakly interacting massive particle–nucleon scattering cross section for weakly interacting massive particle masses above 8 GeV/c2, with a minimum of 2×10-45 cm2 at 55 GeV/c2 and 90% confidence level.

Original language	English
Article number	181301
Number of pages	6
Journal	Physical Review Letters
Volume	109
Issue number	18
DOIs	https://doi.org/10.1103/PhysRevLett.109.181301
Publication status	Published - 2 Nov 2012

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10.1103/PhysRevLett.109.181301

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Aprile, E., Alfonsi, M., Arisaka, K., Arneodo, F., Balan, C., Baudis, L., Bauermeister, B., Behrens, A., Beltrame, P., Bokeloh, K., Brown, E., Bruno, G., Budnik, R., Cardoso, J. M. R., Chen, W., Choi, B., Cline, D., Colijn, A. P., Contreras, H., ... Weinheimer, C. (2012). Dark Matter Results from 225 Live Days of XENON100 Data. Physical Review Letters, 109(18), Article 181301. https://doi.org/10.1103/PhysRevLett.109.181301

@article{d1f82b001ccc465b8a4381c5ebfe8746,

title = "Dark Matter Results from 225 Live Days of XENON100 Data",

abstract = "We report on a search for particle dark matter with the XENON100 experiment, operated at the Laboratori Nazionali del Gran Sasso for 13 months during 2011 and 2012. XENON100 features an ultralow electromagnetic background of (5.3±0.6)×10-3 events/(keVee×kg×day) in the energy region of interest. A blind analysis of 224.6 live days×34 kg exposure has yielded no evidence for dark matter interactions. The two candidate events observed in the predefined nuclear recoil energy range of 6.6–30.5 keVnr are consistent with the background expectation of (1.0±0.2) events. A profile likelihood analysis using a 6.6–43.3 keVnr energy range sets the most stringent limit on the spin-independent elastic weakly interacting massive particle–nucleon scattering cross section for weakly interacting massive particle masses above 8 GeV/c2, with a minimum of 2×10-45 cm2 at 55 GeV/c2 and 90% confidence level.",

author = "E. Aprile and M. Alfonsi and K. Arisaka and F. Arneodo and C. Balan and L. Baudis and B. Bauermeister and A. Behrens and P. Beltrame and K. Bokeloh and E. Brown and G. Bruno and R. Budnik and Cardoso, {J. M. R.} and W.-t. Chen and B. Choi and D. Cline and Colijn, {A. P.} and H. Contreras and Cussonneau, {J. P.} and Decowski, {M. P.} and E. Duchovni and S. Fattori and Ferella, {A. D.} and W. Fulgione and F. Gao and M. Garbini and C. Ghag and K.-l. Giboni and Goetzke, {L. W.} and C. Grignon and E. Gross and W. Hampel and F. Kaether and A. Kish and J. Lamblin and H. Landsman and Lang, {R. F.} and {Le Calloch}, M. and C. Levy and Lim, {K. E.} and Q. Lin and S. Lindemann and M. Lindner and Lopes, {J. A. M.} and K. Lung and {Marrod??n Undagoitia}, T. and Massoli, {F. V.} and {Melgarejo Fernandez}, {A. J.} and Y. Meng and A. Molinario and E. Nativ and K. Ni and U. Oberlack and Orrigo, {S. E. A.} and E. Pantic and R. Persiani and G. Plante and N. Priel and A. Rizzo and S. Rosendahl and {Dos Santos}, {J. M. F.} and G. Sartorelli and J. Schreiner and M. Schumann and {Scotto Lavina}, L. and Scovell, {P. R.} and M. Selvi and P. Shagin and H. Simgen and A. Teymourian and D. Thers and O. Vitells and H. Wang and M. Weber and C. Weinheimer",

year = "2012",

month = nov,

day = "2",

doi = "10.1103/PhysRevLett.109.181301",

language = "English",

volume = "109",

journal = "Physical Review Letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "18",

}

Aprile, E, Alfonsi, M, Arisaka, K, Arneodo, F, Balan, C, Baudis, L, Bauermeister, B, Behrens, A, Beltrame, P, Bokeloh, K, Brown, E, Bruno, G, Budnik, R, Cardoso, JMR, Chen, W, Choi, B, Cline, D, Colijn, AP, Contreras, H, Cussonneau, JP, Decowski, MP, Duchovni, E, Fattori, S, Ferella, AD, Fulgione, W, Gao, F, Garbini, M, Ghag, C, Giboni, K, Goetzke, LW, Grignon, C, Gross, E, Hampel, W, Kaether, F, Kish, A, Lamblin, J, Landsman, H, Lang, RF, Le Calloch, M, Levy, C, Lim, KE, Lin, Q, Lindemann, S, Lindner, M, Lopes, JAM, Lung, K, Marrod??n Undagoitia, T, Massoli, FV, Melgarejo Fernandez, AJ, Meng, Y, Molinario, A, Nativ, E, Ni, K, Oberlack, U, Orrigo, SEA, Pantic, E, Persiani, R, Plante, G, Priel, N, Rizzo, A, Rosendahl, S, Dos Santos, JMF, Sartorelli, G, Schreiner, J, Schumann, M, Scotto Lavina, L, Scovell, PR, Selvi, M, Shagin, P, Simgen, H, Teymourian, A, Thers, D, Vitells, O, Wang, H, Weber, M & Weinheimer, C 2012, 'Dark Matter Results from 225 Live Days of XENON100 Data', Physical Review Letters, vol. 109, no. 18, 181301. https://doi.org/10.1103/PhysRevLett.109.181301

TY - JOUR

T1 - Dark Matter Results from 225 Live Days of XENON100 Data

AU - Aprile, E.

AU - Alfonsi, M.

AU - Arisaka, K.

AU - Arneodo, F.

AU - Balan, C.

AU - Baudis, L.

AU - Bauermeister, B.

AU - Behrens, A.

AU - Beltrame, P.

AU - Bokeloh, K.

AU - Brown, E.

AU - Bruno, G.

AU - Budnik, R.

AU - Cardoso, J. M. R.

AU - Chen, W.-t.

AU - Choi, B.

AU - Cline, D.

AU - Colijn, A. P.

AU - Contreras, H.

AU - Cussonneau, J. P.

AU - Decowski, M. P.

AU - Duchovni, E.

AU - Fattori, S.

AU - Ferella, A. D.

AU - Fulgione, W.

AU - Gao, F.

AU - Garbini, M.

AU - Ghag, C.

AU - Giboni, K.-l.

AU - Goetzke, L. W.

AU - Grignon, C.

AU - Gross, E.

AU - Hampel, W.

AU - Kaether, F.

AU - Kish, A.

AU - Lamblin, J.

AU - Landsman, H.

AU - Lang, R. F.

AU - Le Calloch, M.

AU - Levy, C.

AU - Lim, K. E.

AU - Lin, Q.

AU - Lindemann, S.

AU - Lindner, M.

AU - Lopes, J. A. M.

AU - Lung, K.

AU - Marrod??n Undagoitia, T.

AU - Massoli, F. V.

AU - Melgarejo Fernandez, A. J.

AU - Meng, Y.

AU - Molinario, A.

AU - Nativ, E.

AU - Ni, K.

AU - Oberlack, U.

AU - Orrigo, S. E. A.

AU - Pantic, E.

AU - Persiani, R.

AU - Plante, G.

AU - Priel, N.

AU - Rizzo, A.

AU - Rosendahl, S.

AU - Dos Santos, J. M. F.

AU - Sartorelli, G.

AU - Schreiner, J.

AU - Schumann, M.

AU - Scotto Lavina, L.

AU - Scovell, P. R.

AU - Selvi, M.

AU - Shagin, P.

AU - Simgen, H.

AU - Teymourian, A.

AU - Thers, D.

AU - Vitells, O.

AU - Wang, H.

AU - Weber, M.

AU - Weinheimer, C.

PY - 2012/11/2

Y1 - 2012/11/2

N2 - We report on a search for particle dark matter with the XENON100 experiment, operated at the Laboratori Nazionali del Gran Sasso for 13 months during 2011 and 2012. XENON100 features an ultralow electromagnetic background of (5.3±0.6)×10-3 events/(keVee×kg×day) in the energy region of interest. A blind analysis of 224.6 live days×34 kg exposure has yielded no evidence for dark matter interactions. The two candidate events observed in the predefined nuclear recoil energy range of 6.6–30.5 keVnr are consistent with the background expectation of (1.0±0.2) events. A profile likelihood analysis using a 6.6–43.3 keVnr energy range sets the most stringent limit on the spin-independent elastic weakly interacting massive particle–nucleon scattering cross section for weakly interacting massive particle masses above 8 GeV/c2, with a minimum of 2×10-45 cm2 at 55 GeV/c2 and 90% confidence level.

AB - We report on a search for particle dark matter with the XENON100 experiment, operated at the Laboratori Nazionali del Gran Sasso for 13 months during 2011 and 2012. XENON100 features an ultralow electromagnetic background of (5.3±0.6)×10-3 events/(keVee×kg×day) in the energy region of interest. A blind analysis of 224.6 live days×34 kg exposure has yielded no evidence for dark matter interactions. The two candidate events observed in the predefined nuclear recoil energy range of 6.6–30.5 keVnr are consistent with the background expectation of (1.0±0.2) events. A profile likelihood analysis using a 6.6–43.3 keVnr energy range sets the most stringent limit on the spin-independent elastic weakly interacting massive particle–nucleon scattering cross section for weakly interacting massive particle masses above 8 GeV/c2, with a minimum of 2×10-45 cm2 at 55 GeV/c2 and 90% confidence level.

U2 - 10.1103/PhysRevLett.109.181301

DO - 10.1103/PhysRevLett.109.181301

M3 - Article

SN - 0031-9007

VL - 109

JO - Physical Review Letters

JF - Physical Review Letters

IS - 18

M1 - 181301

ER -

Dark Matter Results from 225 Live Days of XENON100 Data

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