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  Response of the XENON100 dark matter detector to nuclear recoils

XENON Collaboration, Aprile, E., Alfonsi, M., Arisaka, K., Arneodo, F., Balan, C., et al. (2013). Response of the XENON100 dark matter detector to nuclear recoils. Physical Review D, 88(1): 012006, pp. 1-10. doi:10.1103/PhysRevD.88.012006.

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Datensatz-Permalink: http://hdl.handle.net/11858/00-001M-0000-0014-48AC-9 Versions-Permalink: http://hdl.handle.net/11858/00-001M-0000-0015-7A8A-F
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1304.1427v2Xenon100.pdf (Preprint), 690KB
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Results from the nuclear recoil calibration of the XENON100 dark matter detector installed un- derground 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 eciency Le . 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 conrm the validity of the derived signal acceptance in earlier reported dark matter searches of the XENON100 experiment.
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1304.1427v2Xenon100.pdf (Preprint), 690KB
Name:
1304.1427v2Xenon100.pdf
Beschreibung:
Results from the nuclear recoil calibration of the XENON100 dark matter detector installed un- derground 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 eciency Le . 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 conrm the validity of the derived signal acceptance in earlier reported dark matter searches of the XENON100 experiment.
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http://link.aps.org/doi/10.1103/PhysRevD.88.012006 (Verlagsversion)
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XENON Collaboration, Autor              
Aprile, E.1, Autor
Alfonsi, M.2, Autor
Arisaka, K.3, Autor
Arneodo, F.4, Autor
Balan, C.5, Autor
Baudis, L.6, Autor
Bauermeister, B.7, Autor
Behrens, A.6, Autor
Beltrame, P.8, Autor
Beltrame, P.3, Autor
Bokeloh, K.9, Autor
Brown, A.10, Autor
Brown, E.9, Autor
Brünner, Stefan11, Autor              
Bruno, G.4, Autor
Budnik, R.1, Autor
Cardoso, J. M. R.5, Autor
Chen, W. -T.12, Autor
Choi, B.1, Autor
Colijn, A. P.2, AutorContreras, H.1, AutorCussonneau, J. P.12, AutorDecowski, M. P.2, AutorDuchovni, E.8, AutorFattori, S.7, AutorFerella, A. D.4, AutorFerella, A. D.6, AutorFulgione, W.13, AutorGao, F.14, AutorGarbini, M.15, AutorGeis, C.7, AutorGhag, C.3, AutorGiboni, K. -L.1, AutorGoetzke, L. W.1, AutorGrignon, C.7, AutorGross, E.8, AutorHampel, W.11, Autor              Itay, R.8, AutorKaether, F.11, Autor              Kessler, G.6, AutorKish, A.6, AutorLamblin, J., AutorLandsman, H.8, AutorLang, R. F.10, AutorCalloch, M. Le12, AutorLevy, C.9, AutorLim, K. E.1, AutorLin, Q.14, AutorLindemann, Sebastian11, Autor              Lindner, M.11, Autor              Lopes, J. A. M.5, AutorLung, K.3, AutorMarrodan Undagoitia, Teresa11, Autor              Undagoitia, T. Marrodan6, AutorFernandez, A. J. Melgarejo1, AutorMeng, Y.3, AutorMessina, M.1, AutorMolinario, A.13, AutorNi, K.14, AutorOberlack, U.7, AutorOrrigo, S. E. A.5, AutorPantic, E.3, AutorPersiani, R.15, AutorPlante, G.1, AutorPriel, N.8, AutorRizzo, A.1, AutorRosendahl, S.9, AutorSantos, J. M. F. dos5, AutorSartorelli, G.15, AutorSchreiner, J.11, Autor              Schumann, M.16, AutorSchumann, M.6, AutorLavina, L. Scotto12, AutorScovell, P. R.3, AutorSelvi, M.15, AutorShagin, P.17, AutorSimgen, H.11, Autor              Teymourian, A.3, AutorThers, D.12, AutorVitells, O.8, AutorWang, H.3, AutorWeber, Marc11, Autor              Weinheimer, C.9, AutorSchuhmacher, H.18, AutorWiegel, B.18, Autor mehr..
Affiliations:
1Physics Department, Columbia University, New York, NY 10027, USA, ou_904549              
2Nikhef and the University of Amsterdam, Amsterdam, Netherlands, ou_persistent22              
3Physics and Astronomy Department, University of California, Los Angeles, USA, ou_persistent22              
4INFN, Laboratori Nazionali del Gran Sasso, Assergi, 67100, Italy, ou_persistent22              
5Department of Physics, University of Coimbra, R. Larga, 3004-516, Coimbra, Portugal, ou_persistent22              
6Physics Institute, University of Zürich, Winterthurerstr. 190, CH-8057 Zürich, Switzerland, ou_persistent22              
7Institute of Physics & PRISMA Cluster of Excellence, Johannes Gutenberg University Mainz, 55099 Mainz, Germany, ou_persistent22              
8Department of Particle Physics and Astrophysics, Weizmann Institute of Science, 76100 Rehovot, Israel, ou_persistent22              
9Institut für Kernphysik, Wilhelms-Universität Münster, 48149 Münster, Germany, ou_persistent22              
10Department of Physics, Purdue University, West Lafayette, IN 47907, USA, ou_persistent22              
11Division Prof. Dr. Manfred Lindner, MPI for Nuclear Physics, Max Planck Society, ou_904549              
12SUBATECH, Ecole des Mines de Nantes, Université de Nantes, 44307 Nantes, France, ou_persistent22              
13INFN-Torino and Osservatorio Astrofisico di Torino, 10100 Torino, Italy, ou_persistent22              
14Department of Physics, Shanghai Jiao Tong University, Shanghai, 200240, China, ou_persistent22              
15University of Bologna and INFN-Bologna, Bologna, Italy, ou_persistent22              
16Albert Einstein Center for Fundamental Physics, University of Bern, Sidlerstraße 5, 3012 Bern, Switzerland, ou_persistent22              
17Department of Physics and Astronomy, Rice University, Houston, TX 77005-1892, USA, ou_persistent22              
18Physikalisch-Technische Bundesanstalt, Bundesallee 100, 38116 Braunschweig, Germany, ou_persistent22              

Inhalt

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Schlagwörter: Astrophysics, Instrumentation and Methods for Astrophysics, astro-ph.IM,Astrophysics, Cosmology and Extragalactic Astrophysics, astro-ph.CO
 Zusammenfassung: 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.

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 Datum: 2013-04-042013-07-182013-07-30
 Publikationsstatus: Online publiziert
 Seiten: 10 pages, 10 figures. Matches version accepted by PRD. Contains revised representation of expected WIMP event signature. Conclusions remain unaffected
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
 Art der Begutachtung: Expertenbegutachtung
 Identifikatoren: arXiv: 1304.1427
DOI: 10.1103/PhysRevD.88.012006
 Art des Abschluß: -

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Titel: Physical Review D
  Andere : Phys. Rev. D.
Genre der Quelle: Zeitschrift
 Urheber:
Affiliations:
Ort, Verlag, Ausgabe: Lancaster, Pa. : Published for the American Physical Society by the American Institute of Physics
Seiten: - Band / Heft: 88 (1) Artikelnummer: 012006 Start- / Endseite: 1 - 10 Identifikator: ISSN: 0556-2821
CoNE: /journals/resource/111088197762258