Search Results - "E. Aprile"

Liquid-phase purification for multi-tonne xenon detectors by Plante, G., Aprile, E., Howlett, J., Zhang, Y.

“…As liquid xenon detectors grow in scale, novel techniques are required to maintain sufficient purity for charges to survive across longer drift paths. The…”
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Liquid xenon detectors for particle physics and astrophysics by Aprile, E., Doke, T.

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Dark matter results from 225 live days of XENON100 data by 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-T, Choi, B, Cline, D, Colijn, A P, Contreras, H, Cussonneau, J P, Decowski, M P, Duchovni, E, Fattori, S, Ferella, A D, Fulgione, W, Gao, F, Garbini, M, Ghag, C, Giboni, K-L, Goetzke, L W, Grignon, C, Gross, E, Hampel, W, Kaether, F, Kish, A, Lamblin, J, Landsman, H, Lang, R F, Le Calloch, M, Levy, C, Lim, K E, Lin, Q, Lindemann, S, Lindner, M, Lopes, J A M, Lung, K, Marrodán Undagoitia, T, Massoli, F V, Melgarejo Fernandez, A J, Meng, Y, Molinario, A, Nativ, E, Ni, K, Oberlack, U, Orrigo, S E A, Pantic, E, Persiani, R, Plante, G, Priel, N, Rizzo, A, Rosendahl, S, dos Santos, J M F, Sartorelli, G, Schreiner, J, Schumann, M, Scotto Lavina, L, Scovell, P R, Selvi, M, Shagin, P, Simgen, H, Teymourian, A, Thers, D, Vitells, O, Wang, H, Weber, M, Weinheimer, C

“…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…”
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Dark matter results from 100 live days of XENON100 data by Aprile, E, Arisaka, K, Arneodo, F, Askin, A, Baudis, L, Behrens, A, Bokeloh, K, Brown, E, Bruch, T, Bruno, G, Cardoso, J M R, Chen, W-T, Choi, B, Cline, D, Duchovni, E, Fattori, S, Ferella, A D, Gao, F, Giboni, K-L, Gross, E, Kish, A, Lam, C W, Lamblin, J, Lang, R F, Levy, C, Lim, K E, Lin, Q, Lindemann, S, Lindner, M, Lopes, J A M, Lung, K, Undagoitia, T Marrodán, Mei, Y, Fernandez, A J Melgarejo, Ni, K, Oberlack, U, Orrigo, S E A, Pantic, E, Persiani, R, Plante, G, Ribeiro, A C C, Santorelli, R, dos Santos, J M F, Sartorelli, G, Schumann, M, Selvi, M, Shagin, P, Simgen, H, Teymourian, A, Thers, D, Vitells, O, Wang, H, Weber, M, Weinheimer, C

“…We present results from the direct search for dark matter with the XENON100 detector, installed underground at the Laboratori Nazionali del Gran Sasso of INFN,…”
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Search for light dark matter in XENON10 data by Angle, J, Aprile, E, Arneodo, F, Baudis, L, Bernstein, A, Bolozdynya, A I, Coelho, L C C, Dahl, C E, DeViveiros, L, Ferella, A D, Fernandes, L M P, Fiorucci, S, Gaitskell, R J, Giboni, K L, Gomez, R, Hasty, R, Kastens, L, Kwong, J, Lopes, J A M, Madden, N, Manalaysay, A, Manzur, A, McKinsey, D N, Monzani, M E, Ni, K, Oberlack, U, Orboeck, J, Plante, G, Santorelli, R, dos Santos, J M F, Schulte, S, Shagin, P, Shutt, T, Sorensen, P, Winant, C, Yamashita, M

“…We report results of a search for light (≲10  GeV) particle dark matter with the XENON10 detector. The event trigger was sensitive to a single electron, with…”
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Limits on spin-dependent WIMP-nucleon cross sections from 225 live days of XENON100 data by Aprile, E, Alfonsi, M, Arisaka, K, Arneodo, F, Balan, C, Baudis, L, Bauermeister, B, Behrens, A, Beltrame, P, Bokeloh, K, Brown, A, Brown, E, Bruno, G, Budnik, R, Cardoso, J M R, Chen, W-T, Choi, B, Colijn, A P, Contreras, H, Cussonneau, J P, Decowski, M P, Duchovni, E, Fattori, S, Ferella, A D, Fulgione, W, Gao, F, Garbini, M, Ghag, C, Giboni, K-L, Goetzke, L W, Grignon, C, Gross, E, Hampel, W, Kaether, F, Kish, A, Lamblin, J, Landsman, H, Lang, R F, Le Calloch, M, Lellouch, D, Levy, C, Lim, K E, Lin, Q, Lindemann, S, Lindner, M, Lopes, J A M, Lung, K, Marrodán Undagoitia, T, Massoli, F V, Melgarejo Fernandez, A J, Meng, Y, Messina, M, Molinario, A, Ni, K, Oberlack, U, Orrigo, S E A, Pantic, E, Persiani, R, Plante, G, Priel, N, Rizzo, A, Rosendahl, S, dos Santos, J M F, Sartorelli, G, Schreiner, J, Schumann, M, Scotto Lavina, L, Scovell, P R, Selvi, M, Shagin, P, Simgen, H, Teymourian, A, Thers, D, Vitells, O, Wang, H, Weber, M, Weinheimer, C

“…We present new experimental constraints on the elastic, spin-dependent WIMP-nucleon cross section using recent data from the XENON100 experiment, operated in…”
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The XENON100 dark matter experiment by Aprile, E., Arisaka, K., Arneodo, F., Askin, A., Baudis, L., Behrens, A., Brown, E., Cardoso, J.M.R., Choi, B., Cline, D., Fattori, S., Ferella, A.D., Giboni, K.L., Kish, A., Lam, C.W., Lang, R.F., Lim, K.E., Lopes, J.A.M., Marrodán Undagoitia, T., Mei, Y., Melgarejo Fernandez, A.J., Ni, K., Oberlack, U., Orrigo, S.E.A., Pantic, E., Plante, G., Ribeiro, A.C.C., Santorelli, R., dos Santos, J.M.F., Schumann, M., Shagin, P., Teymourian, A., Tziaferi, E., Wang, H., Yamashita, M.

“…► XENON100 is currently one of the most sensitive experiments to detect WIMP dark matter. ► Detector design and active/passive shielding reduce the radioactive…”
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First dark matter results from the XENON100 experiment by Aprile, E, Arisaka, K, Arneodo, F, Askin, A, Baudis, L, Behrens, A, Bokeloh, K, Brown, E, Cardoso, J M R, Choi, B, Cline, D B, Fattori, S, Ferella, A D, Giboni, K-L, Kish, A, Lam, C W, Lamblin, J, Lang, R F, Lim, K E, Lopes, J A M, Marrodán Undagoitia, T, Mei, Y, Melgarejo Fernandez, A J, Ni, K, Oberlack, U, Orrigo, S E A, Pantic, E, Plante, G, Ribeiro, A C C, Santorelli, R, Dos Santos, J M F, Schumann, M, Shagin, P, Teymourian, A, Thers, D, Tziaferi, E, Wang, H, Weinheimer, C

“…The XENON100 experiment, in operation at the Laboratori Nazionali del Gran Sasso in Italy, is designed to search for dark matter weakly interacting massive…”
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First results from the XENON10 dark matter experiment at the Gran Sasso National Laboratory by Angle, J, Aprile, E, Arneodo, F, Baudis, L, Bernstein, A, Bolozdynya, A, Brusov, P, Coelho, L C C, Dahl, C E, DeViveiros, L, Ferella, A D, Fernandes, L M P, Fiorucci, S, Gaitskell, R J, Giboni, K L, Gomez, R, Hasty, R, Kastens, L, Kwong, J, Lopes, J A M, Madden, N, Manalaysay, A, Manzur, A, McKinsey, D N, Monzani, M E, Ni, K, Oberlack, U, Orboeck, J, Plante, G, Santorelli, R, dos Santos, J M F, Shagin, P, Shutt, T, Sorensen, P, Schulte, S, Winant, C, Yamashita, M

“…The XENON10 experiment at the Gran Sasso National Laboratory uses a 15 kg xenon dual phase time projection chamber to search for dark matter weakly interacting…”
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Simultaneous measurement of ionization and scintillation from nuclear recoils in liquid xenon for a dark matter experiment by Aprile, E, Dahl, C E, de Viveiros, L, Gaitskell, R J, Giboni, K L, Kwong, J, Majewski, P, Ni, K, Shutt, T, Yamashita, M

“…We report the first measurements of the absolute ionization yield of nuclear recoils in liquid xenon, as a function of energy and electric field. Independent…”
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Online [Formula omitted]Rn removal by cryogenic distillation in the XENON100 experiment by Aprile, E, Aalbers, J, Agostini, F, Alfonsi, M, Amaro, F. D, Anthony, M, Arneodo, F

“…We describe the purification of xenon from traces of the radioactive noble gas radon using a cryogenic distillation column. The distillation column was…”
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Low-energy calibration of XENON1T with an internal $$^{{\textbf {37}}}$$Ar source by Aprile, E, Abe, K, Agostini, F, Ahmed Maouloud, S, Alfonsi, M, Althueser, L, Andrieu, B

“…Abstract A low-energy electronic recoil calibration of XENON1T, a dual-phase xenon time projection chamber, with an internal $^{37}$$ 37 Ar source was…”
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Likelihood approach to the first dark matter results from XENON100 by Aprile, E., Arisaka, K., Arneodo, F., Askin, A., Baudis, L., Behrens, A., Bokeloh, K., Brown, E., Bruch, T., Cardoso, J. M. R., Choi, B., Cline, D., Duchovni, E., Fattori, S., Ferella, A. D., Giboni, K.-L., Gross, E., Kish, A., Lam, C. W., Lamblin, J., Lang, R. F., Lim, K. E., Lindemann, S., Lindner, M., Lopes, J. A. M., Marrodán Undagoitia, T., Mei, Y., Melgarejo Fernandez, A. J., Ni, K., Oberlack, U., Orrigo, S. E. A., Pantic, E., Plante, G., Ribeiro, A. C. C., Santorelli, R., dos Santos, J. M. F., Schumann, M., Shagin, P., Teymourian, A., Thers, D., Tziaferi, E., Vitells, O., Wang, H., Weber, M., Weinheimer, C.

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Erratum to: Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of 136Xe by Agostini, F., Maouloud, S. E. M. Ahmed, Althueser, L., Amaro, F., Antunovic, B., Aprile, E., Baudis, L., Baur, D., Biondi, Y., Bismark, A., Breur, P. A., Brown, A., Bruno, G., Budnik, R., Capelli, C., Cardoso, J., Cichon, D., Clark, M., Colijn, A. P., Cuenca-García, J. J., Cussonneau, J. P., Decowski, M. P., Depoian, A., Dierle, J., Gangi, P. Di, Giovanni, A. Di, Diglio, S., Santos, J. M. F. dos, Drexlin, G., Eitel, K., Engel, R., Ferella, A. D., Fischer, H., Galloway, M., Gao, F., Girard, F., Glück, F., Grandi, L., Größle, R., Gumbsheimer, R., Hansmann-Menzemer, S., Jörg, F., Khundzakishvili, G., Kopec, A., Kuger, F., Krauss, L. M., Landsman, H., Lang, R. F., Lindemann, S., Lindner, M., Lopes, J. A. M., Villalpando, A. Loya, Macolino, C., Manfredini, A., Undagoitia, T. Marrodán, Masbou, J., Masson, E., Meinhardt, P., Milutinovic, S., Molinario, A., Monteiro, C. M. B., Murra, M., Oberlack, U. G., Pandurovic, M., Peres, R., Pienaar, J., Pierre, M., Pizzella, V., Qin, J., García, D. Ramírez, Reichard, S., Rupp, N., Sanchez-Lucas, P., Sartorelli, G., Schulte, D., Schumann, M., Lavina, L. Scotto, Selvi, M., Silva, M., Simgen, H., Steidl, M., Terliuk, A., Therreau, C., Thers, D., Thieme, K., Trotta, R., Tunnell, C. D., Valerius, K., Volta, G., Vorkapic, D., Weinheimer, C., Wittweg, C., Wolf, J., Zopounidis, J. P., Zuber, K.

“…We correct an overestimation of the production rate of 137 Xe in the DARWIN detector operated at LNGS. This formerly dominant intrinsic background source is…”
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Erratum to: Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of $$^{136}$$Xe by Agostini, F, Maouloud, S. E. M. Ahmed, Althueser, L, Amaro, F, Antunovic, B, Aprile, E, Baudis, L

“…Abstract We correct an overestimation of the production rate of $$^{137}$$ 137 Xe in the DARWIN detector operated at LNGS. This formerly dominant intrinsic…”
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Design and performance of the XENON10 dark matter experiment by Aprile, E., Angle, J., Arneodo, F., Baudis, L., Bernstein, A., Bolozdynya, A., Brusov, P., Coelho, L.C.C., Dahl, C.E., DeViveiros, L., Ferella, A.D., Fernandes, L.M.P., Fiorucci, S., Gaitskell, R.J., Giboni, K.L., Gomez, R., Hasty, R., Kastens, L., Kwong, J., Lopes, J.A.M., Madden, N., Manalaysay, A., Manzur, A., McKinsey, D.N., Monzani, M.E., Ni, K., Oberlack, U., Orboeck, J., Orlandi, D., Plante, G., Santorelli, R., dos Santos, J.M.F., Shagin, P., Shutt, T., Sorensen, P., Schulte, S., Tatananni, E., Winant, C., Yamashita, M.

“…XENON10 is the first two-phase xenon time projection chamber (TPC) developed within the XENON dark matter search program. The TPC, with an active liquid xenon…”
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Limits on spin-dependent WIMP-nucleon cross sections from the XENON10 experiment by Angle, J, Aprile, E, Arneodo, F, Baudis, L, Bernstein, A, Bolozdynya, A, Coelho, L C C, Dahl, C E, DeViveiros, L, Ferella, A D, Fernandes, L M P, Fiorucci, S, Gaitskell, R J, Giboni, K L, Gomez, R, Hasty, R, Kastens, L, Kwong, J, Lopes, J A M, Madden, N, Manalaysay, A, Manzur, A, McKinsey, D N, Monzani, M E, Ni, K, Oberlack, U, Orboeck, J, Plante, G, Santorelli, R, dos Santos, J M F, Shagin, P, Shutt, T, Sorensen, P, Schulte, S, Winant, C, Yamashita, M

“…XENON10 is an experiment to directly detect weakly interacting massive particles (WIMPs), which may comprise the bulk of the nonbaryonic dark matter in our…”
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Material screening and selection for XENON100 by Aprile, E., Arisaka, K., Arneodo, F., Askin, A., Baudis, L., Behrens, A., Bokeloh, K., Brown, E., Cardoso, J.M.R., Choi, B., Cline, D., Fattori, S., Ferella, A.D., Giboni, K.L., Kish, A., Lam, C.W., Lamblin, J., Lang, R.F., Lim, K.E., Lopes, J.A.M., Marrodán Undagoitia, T., Mei, Y., Melgarejo Fernandez, A.J., Ni, K., Oberlack, U., Orrigo, S.E.A., Pantic, E., Plante, G., Ribeiro, A.C.C., Santorelli, R., dos Santos, J.M.F., Schumann, M., Shagin, P., Teymourian, A., Thers, D., Tziaferi, E., Wang, H., Weinheimer, C., Laubenstein, M., Nisi, S.

“…► Material selection based on their intrinsic radioactive contaminations is crucial for low background experiments. ► We present detailed results from the…”
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Study of the electromagnetic background in the XENON100 experiment by Aprile, E., Arisaka, K., Arneodo, F., Askin, A., Baudis, L., Behrens, A., Bokeloh, K., Brown, E., Cardoso, J. M. R., Choi, B., Cline, D., Fattori, S., Ferella, A. D., Giboni, K.-L., Kish, A., Lam, C. W., Lamblin, J., Lang, R. F., Lim, K. E., Lin, Q., Lindemann, S., Lindner, M., Lopes, J. A. M., Lung, K., Marrodán Undagoitia, T., Mei, Y., Melgarejo Fernandez, A. J., Ni, K., Oberlack, U., Orrigo, S. E. A., Pantic, E., Plante, G., Ribeiro, A. C. C., Santorelli, R., dos Santos, J. M. F., Schumann, M., Shagin, P., Simgen, H., Teymourian, A., Thers, D., Tziaferi, E., Wang, H., Weber, M., Weinheimer, C.

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Detection of liquid xenon scintillation light with a silicon photomultiplier by Aprile, E., Cushman, P., Ni, K., Shagin, P.

“…We have studied the feasibility of a silicon photomultiplier (SiPM) to detect liquid xenon (LXe) scintillation light. The SiPM was operated inside a small…”
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