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Response of the XENON100 dark matter detector to nuclear recoils

Authors :
Aprile, E.
Alfonsi, M.
Arisaka, K.
Arneodo, F.
Balan, C.
Baudis, L.
Bauermeister, B.
Behrens, A.
Beltrame, P.
Bokeloh, K.
Brown, A.
Brown, E.
Brünner, S.
Bruno, G.
Budnik, R.
Cardoso, J.
Chen, W.
Choi, B.
Colijn, A.
Contreras, H.
Cussonneau, J.
Decowski, M.
Duchovni, E.
Fattori, S.
Ferella, A.
Fulgione, W.
Gao, F.
Garbini, M.
Geis, C.
Ghag, C.
Giboni, K.
Goetzke, L.
Grignon, C.
Gross, E.
Hampel, W.
Itay, R.
Kaether, F.
Kessler, G.
Kish, A.
Lamblin, J.
Landsman, H.
Lang, R.
Calloch, M.
Levy, C.
Lim, K.
Lin, Q.
Lindemann, S.
Lindner, M.
Lopes, J.
Lung, K.
Marrodan Undagoitia, T.
Undagoitia, T.
Fernandez, A.
Meng, Y.
Messina, M.
Molinario, A.
Ni, K.
Oberlack, U.
Orrigo, S.
Pantic, E.
Persiani, R.
Plante, G.
Priel, N.
Rizzo, A.
Rosendahl, S.
Santos, J.
Sartorelli, G.
Schreiner, J.
Schumann, M.
Lavina, L.
Scovell, P.
Selvi, M.
Shagin, P.
Simgen, H.
Teymourian, A.
Thers, D.
Vitells, O.
Wang, H.
Weber, M.
Weinheimer, C.
Schuhmacher, H.
Wiegel, B.
Astroparticle Physics (IHEF, IoP, FNWI)
Laboratoire SUBATECH Nantes (SUBATECH)
Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes)
XENON100
E. Aprile
M. Alfonsi
K. Arisaka
F. Arneodo
C. Balan
L. Baudi
B. Bauermeister
A. Behren
P. Beltrame
K. Bokeloh
A. Brown
E. Brown
S. Bruenner
G. Bruno
R. Budnik
J. M. R. Cardoso
W.-T. Chen
B. Choi
A. P. Colijn
H. Contrera
J. P. Cussonneau
M. P. Decowski
E. Duchovni
S. Fattori
A. D. Ferella
W. Fulgione
F. Gao
M. Garbini
C. Gei
C. Ghag
K.-L. Giboni
L. W. Goetzke
C. Grignon
E. Gro
W. Hampel
R. Itay
F. Kaether
G. Kessler
A. Kish
H. Landsman
R. F. Lang
M. Le Calloch
C. Levy
K. E. Lim
Q. Lin
S. Lindemann
M. Lindner
J. A. M. Lope
K. Lung
T. Marrodán Undagoitia
F. V. Massoli
A. J. Melgarejo Fernandez
Y. Meng
M. Messina
A. Molinario
K. Ni
U. Oberlack
S. E. A. Orrigo
E. Pantic
R. Persiani
G. Plante
N. Priel
A. Rizzo
S. Rosendahl
J. M. F. dos Santo
G. Sartorelli
J. Schreiner
M. Schumann
L. Scotto Lavina
P. R. Scovell
M. Selvi
P. Shagin
H. Simgen
A. Teymourian
D. Ther
O. Vitell
H. Wang
M. Weber
C. Weinheimer
H. Schuhmacher
B. Wiegel
XENON Collaboration
Source :
Physical Review D. Particles, Fields, Gravitation, and Cosmology, 88(1). American Institute of Physics, Physical Review D, Physical Review D, American Physical Society, 2013, 88, pp.012006. ⟨10.1103/PhysRevD.88.012006⟩, Repositório Científico de Acesso Aberto de Portugal, Repositório Científico de Acesso Aberto de Portugal (RCAAP), instacron:RCAAP
Publication Year :
2013

Abstract

Results from the nuclear recoil calibration of the XENON100 dark matter detector installed underground at the Laboratori Nazionali del Gran Sasso (LNGS), Italy are presented. Data from measurements with an external 241AmBe neutron source are compared with a detailed Monte Carlo simulation which is used to extract the energy dependent charge-yield Qy and relative scintillation efficiency Leff. A very good level of absolute spectral matching is achieved in both observable signal channels - scintillation S1 and ionization S2 - along with agreement in the 2-dimensional particle discrimination space. The results confirm the validity of the derived signal acceptance in earlier reported dark matter searches of the XENON100 experiment.<br />Comment: 10 pages, 10 figures. Matches version accepted by PRD. Contains revised representation of expected WIMP event signature. Conclusions remain unaffected

Details

Language :
English
ISSN :
15507998 and 15502368
Database :
OpenAIRE
Journal :
Physical Review D. Particles, Fields, Gravitation, and Cosmology, 88(1). American Institute of Physics, Physical Review D, Physical Review D, American Physical Society, 2013, 88, pp.012006. ⟨10.1103/PhysRevD.88.012006⟩, Repositório Científico de Acesso Aberto de Portugal, Repositório Científico de Acesso Aberto de Portugal (RCAAP), instacron:RCAAP
Accession number :
edsair.doi.dedup.....acf83cd814b9c4eb31304dd9bbb71eff
Full Text :
https://doi.org/10.1103/PhysRevD.88.012006⟩