Analysis of the XENON100 dark matter search data

E Aprile; M Alfonsi; K Arisaka; F Arneodo; C Balan; L Baudis; A Behrens; Paolo Beltrame; K Bokeloh; E Brown; G Bruno; Ran Budnik; JMR Cardoso; WT Chen; B Choi; DB Cline; H Contreras; JP Cussonneau; MP Decowski; Ehud Duchovni; S Fattorii; AD Ferella; W Fulgione; F Gao; M Garbini; KL Giboni; LW Goetzke; C Grignon; Eilam Gross; W Hampel; A Kish; J Lamblin; Hagar Landsman; RF Lang; Calloch, M Le Calloch; Camilla Levy; KE Lim; Q Lin; S Lindemann; M Lindner; JAM Lopes; K Lung; TM Undagoitia; FV Massoli; Y Mei; AJM Fernandez; Y Meng; A Molinario; Etai Nativ; K Ni; U Oberlack; SEA Orrigo; E Pantic; R Persiani; G Plante; Nadav Priel; A Rizzo; S Rosendahl; Santos, JMF dos Santos; G Sartorelli; J Schreiner; M Schumann; LS Lavina; PR Scovell; M Selvi; P Shagin; H Simgen; A Teymourian; D Thers; Ofer Vitells; H Wang; M Weber; C Weinheimer

doi:https://doi.org/10.1016/j.astropartphys.2013.10.002

Analysis of the XENON100 dark matter search data

E Aprile, M Alfonsi, K Arisaka, F Arneodo, C Balan, L Baudis, A Behrens, Paolo Beltrame, K Bokeloh, E Brown, G Bruno, Ran Budnik, JMR Cardoso, WT Chen, B Choi, DB Cline, H Contreras, JP Cussonneau, MP Decowski, Ehud DuchovniS Fattorii, AD Ferella, W Fulgione, F Gao, M Garbini, KL Giboni, LW Goetzke, C Grignon, Eilam Gross, W Hampel, A Kish, J Lamblin, Hagar Landsman, RF Lang, Calloch, M Le Calloch, Camilla Levy, KE Lim, Q Lin, S Lindemann, M Lindner, JAM Lopes, K Lung, TM Undagoitia, FV Massoli, Y Mei, AJM Fernandez, Y Meng, A Molinario, Etai Nativ, K Ni, U Oberlack, SEA Orrigo, E Pantic, R Persiani, G Plante, Nadav Priel, A Rizzo, S Rosendahl, Santos, JMF dos Santos, G Sartorelli, J Schreiner, M Schumann, LS Lavina, PR Scovell, M Selvi, P Shagin, H Simgen, A Teymourian, D Thers, Ofer Vitells, H Wang, M Weber, C Weinheimer

Department of Particle Physics and Astrophysics

Weizmann Institute Of Science

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

Abstract

The XENON100 experiment, situated in the Laboratori Nazionali del Gran Sasso, aims at the direct detection of dark matter in the form of weakly interacting massive particles (WIMPs), based on their interactions with xenon nuclei in an ultra low background dual-phase time projection chamber. This paper describes the general methods developed for the analysis of the XENON 100 data. These methods have been used in the 100.9 and 224.6 live days science runs from which results on spin-independent elastic, spin-dependent elastic and inelastic WIMP-nucleon cross-sections have already been reported. (C) 2013 Elsevier B.V. All rights reserved.

Original language	English
Pages (from-to)	11-24
Number of pages	14
Journal	Astroparticle Physics
Volume	54
DOIs	https://doi.org/10.1016/j.astropartphys.2013.10.002
State	Published - Feb 2014

Access to Document

https://doi.org/10.1016/j.astropartphys.2013.10.002

https://ezproxy.weizmann.ac.il/login?url=http://dx.doi.org/10.1016/j.astropartphys.2013.10.002

Cite this

Aprile, E., Alfonsi, M., Arisaka, K., Arneodo, F., Balan, C., Baudis, L., Behrens, A., Beltrame, P., Bokeloh, K., Brown, E., Bruno, G., Budnik, R., Cardoso, JMR., Chen, WT., Choi, B., Cline, DB., Contreras, H., Cussonneau, JP., Decowski, MP., ... Weinheimer, C. (2014). Analysis of the XENON100 dark matter search data. Astroparticle Physics, 54, 11-24. https://doi.org/10.1016/j.astropartphys.2013.10.002

@article{67fe41176e2b49e6ad191349d785a21c,

title = "Analysis of the XENON100 dark matter search data",

abstract = "The XENON100 experiment, situated in the Laboratori Nazionali del Gran Sasso, aims at the direct detection of dark matter in the form of weakly interacting massive particles (WIMPs), based on their interactions with xenon nuclei in an ultra low background dual-phase time projection chamber. This paper describes the general methods developed for the analysis of the XENON 100 data. These methods have been used in the 100.9 and 224.6 live days science runs from which results on spin-independent elastic, spin-dependent elastic and inelastic WIMP-nucleon cross-sections have already been reported. (C) 2013 Elsevier B.V. All rights reserved.",

author = "E Aprile and M Alfonsi and K Arisaka and F Arneodo and C Balan and L Baudis and A Behrens and Paolo Beltrame and K Bokeloh and E Brown and G Bruno and Ran Budnik and JMR Cardoso and WT Chen and B Choi and DB Cline and H Contreras and JP Cussonneau and MP Decowski and Ehud Duchovni and S Fattorii and AD Ferella and W Fulgione and F Gao and M Garbini and KL Giboni and LW Goetzke and C Grignon and Eilam Gross and W Hampel and A Kish and J Lamblin and Hagar Landsman and RF Lang and {Le Calloch}, {Calloch, M} and Camilla Levy and KE Lim and Q Lin and S Lindemann and M Lindner and JAM Lopes and K Lung and TM Undagoitia and FV Massoli and Y Mei and AJM Fernandez and Y Meng and A Molinario and Etai Nativ and K Ni and U Oberlack and SEA Orrigo and E Pantic and R Persiani and G Plante and Nadav Priel and A Rizzo and S Rosendahl and {dos Santos}, {Santos, JMF} and G Sartorelli and J Schreiner and M Schumann and LS Lavina and PR Scovell and M Selvi and P Shagin and H Simgen and A Teymourian and D Thers and Ofer Vitells and H Wang and M Weber and C Weinheimer",

note = "NSF; DOE; SNF; Volkswagen Foundation; FCT; Region des Pays de la Loire; STCSM; NSFC; DFG; MPG; Stichting voor Fundamenteel Onderzoek der Materie (FOM); Weizmann Institute of Science; EMG research center; INFN; Alexander von Humboldt Foundation We gratefully acknowledge support from NSF, DOE, SNF, Volkswagen Foundation, FCT, Region des Pays de la Loire, STCSM, NSFC, DFG, MPG, Stichting voor Fundamenteel Onderzoek der Materie (FOM), the Weizmann Institute of Science, the EMG research center and INFN. T.M.U. acknowledges the Alexander von Humboldt Foundation for support through a Feodor Lynen scholarship. We are grateful to LNGS for hosting and supporting XENON100.",

year = "2014",

month = feb,

doi = "https://doi.org/10.1016/j.astropartphys.2013.10.002",

language = "الإنجليزيّة",

volume = "54",

pages = "11--24",

journal = "Astroparticle Physics",

issn = "0927-6505",

publisher = "Elsevier",

}

Aprile, E, Alfonsi, M, Arisaka, K, Arneodo, F, Balan, C, Baudis, L, Behrens, A, Beltrame, P, Bokeloh, K, Brown, E, Bruno, G, Budnik, R, Cardoso, JMR, Chen, WT, Choi, B, Cline, DB, Contreras, H, Cussonneau, JP, Decowski, MP, Duchovni, E, Fattorii, S, Ferella, AD, Fulgione, W, Gao, F, Garbini, M, Giboni, KL, Goetzke, LW, Grignon, C, Gross, E, Hampel, W, Kish, A, Lamblin, J, Landsman, H, Lang, RF, Le Calloch, CM, Levy, C, Lim, KE, Lin, Q, Lindemann, S, Lindner, M, Lopes, JAM, Lung, K, Undagoitia, TM, Massoli, FV, Mei, Y, Fernandez, AJM, 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, SJMF, Sartorelli, G, Schreiner, J, Schumann, M, Lavina, LS, Scovell, PR, Selvi, M, Shagin, P, Simgen, H, Teymourian, A, Thers, D, Vitells, O, Wang, H, Weber, M & Weinheimer, C 2014, 'Analysis of the XENON100 dark matter search data', Astroparticle Physics, vol. 54, pp. 11-24. https://doi.org/10.1016/j.astropartphys.2013.10.002

TY - JOUR

T1 - Analysis of the XENON100 dark matter search data

AU - Aprile, E

AU - Alfonsi, M

AU - Arisaka, K

AU - Arneodo, F

AU - Balan, C

AU - Baudis, L

AU - Behrens, A

AU - Beltrame, Paolo

AU - Bokeloh, K

AU - Brown, E

AU - Bruno, G

AU - Budnik, Ran

AU - Cardoso, JMR

AU - Chen, WT

AU - Choi, B

AU - Cline, DB

AU - Contreras, H

AU - Cussonneau, JP

AU - Decowski, MP

AU - Duchovni, Ehud

AU - Fattorii, S

AU - Ferella, AD

AU - Fulgione, W

AU - Gao, F

AU - Garbini, M

AU - Giboni, KL

AU - Goetzke, LW

AU - Grignon, C

AU - Gross, Eilam

AU - Hampel, W

AU - Kish, A

AU - Lamblin, J

AU - Landsman, Hagar

AU - Lang, RF

AU - Le Calloch, Calloch, M

AU - Levy, Camilla

AU - Lim, KE

AU - Lin, Q

AU - Lindemann, S

AU - Lindner, M

AU - Lopes, JAM

AU - Lung, K

AU - Undagoitia, TM

AU - Massoli, FV

AU - Mei, Y

AU - Fernandez, AJM

AU - Meng, Y

AU - Molinario, A

AU - Nativ, Etai

AU - Ni, K

AU - Oberlack, U

AU - Orrigo, SEA

AU - Pantic, E

AU - Persiani, R

AU - Plante, G

AU - Priel, Nadav

AU - Rizzo, A

AU - Rosendahl, S

AU - dos Santos, Santos, JMF

AU - Sartorelli, G

AU - Schreiner, J

AU - Schumann, M

AU - Lavina, LS

AU - Scovell, PR

AU - Selvi, M

AU - Shagin, P

AU - Simgen, H

AU - Teymourian, A

AU - Thers, D

AU - Vitells, Ofer

AU - Wang, H

AU - Weber, M

AU - Weinheimer, C

N1 - NSF; DOE; SNF; Volkswagen Foundation; FCT; Region des Pays de la Loire; STCSM; NSFC; DFG; MPG; Stichting voor Fundamenteel Onderzoek der Materie (FOM); Weizmann Institute of Science; EMG research center; INFN; Alexander von Humboldt Foundation We gratefully acknowledge support from NSF, DOE, SNF, Volkswagen Foundation, FCT, Region des Pays de la Loire, STCSM, NSFC, DFG, MPG, Stichting voor Fundamenteel Onderzoek der Materie (FOM), the Weizmann Institute of Science, the EMG research center and INFN. T.M.U. acknowledges the Alexander von Humboldt Foundation for support through a Feodor Lynen scholarship. We are grateful to LNGS for hosting and supporting XENON100.

PY - 2014/2

Y1 - 2014/2

N2 - The XENON100 experiment, situated in the Laboratori Nazionali del Gran Sasso, aims at the direct detection of dark matter in the form of weakly interacting massive particles (WIMPs), based on their interactions with xenon nuclei in an ultra low background dual-phase time projection chamber. This paper describes the general methods developed for the analysis of the XENON 100 data. These methods have been used in the 100.9 and 224.6 live days science runs from which results on spin-independent elastic, spin-dependent elastic and inelastic WIMP-nucleon cross-sections have already been reported. (C) 2013 Elsevier B.V. All rights reserved.

AB - The XENON100 experiment, situated in the Laboratori Nazionali del Gran Sasso, aims at the direct detection of dark matter in the form of weakly interacting massive particles (WIMPs), based on their interactions with xenon nuclei in an ultra low background dual-phase time projection chamber. This paper describes the general methods developed for the analysis of the XENON 100 data. These methods have been used in the 100.9 and 224.6 live days science runs from which results on spin-independent elastic, spin-dependent elastic and inelastic WIMP-nucleon cross-sections have already been reported. (C) 2013 Elsevier B.V. All rights reserved.

U2 - https://doi.org/10.1016/j.astropartphys.2013.10.002

DO - https://doi.org/10.1016/j.astropartphys.2013.10.002

M3 - مقالة

SN - 0927-6505

VL - 54

SP - 11

EP - 24

JO - Astroparticle Physics

JF - Astroparticle Physics

ER -

Analysis of the XENON100 dark matter search data

Abstract

Access to Document

Fingerprint

Cite this