Results 1 to 10 of about 1,899 (32)
A Time Projection Chamber with GEM-Based Readout [PDF]
, 2016 For the International Large Detector concept at the planned International
Linear Collider, the use of time projection chambers (TPC) with micro-pattern
gas detector readout as the main tracking detector is investigated.Attié, David, Behnke, Ties, Bellerive, Alain, Bezshyyko, Oleg, Bhattacharya, Deb Sankar, Bhattacharya, Purba, Bhattacharya, Sudeb, Caiazza, Stefano, Colas, Paul, De Lentdecker, Gilles, Dehmelt, Klaus, Desch, Klaus, Diener, Ralf, Dixit, Madhu, Fleck, Ivor, Fujii, Keisuke, Fusayasu, Takahiro, Ganjour, Serguei, Gao, Yuanning, Gros, Philippe, Hayman, Peter, Hedberg, Vincent, Ikematsu, Katsumasa, Jönsson, Leif, Kaminski, Jochen, Kato, Yukihiro, Kawada, Shin-ichi, Killenberg, Martin, Kleinwort, Claus, Kobayashi, Makoto, Krylov, Vladyslav, Li, Bo, Li, Yulan, Lundberg, Björn, Lupberger, Michael, Majumdar, Nayana, Matsuda, Takeshi, Mehdiyev, Rashid, Mjörnmark, Ulf, Mukhopadhyay, Supratik, Müller, Felix, Münnich, Astrid, Ogawa, Tomohisa, Oskarsson, Anders, Peterson, Daniel, Riallot, Marc, Rosemann, Christoph, Roth, Stefan, Schade, Peter, Schäfer, Oliver, Settles, Ronald Dean, Shirazi, Amir Noori, Smirnova, Oxana, Sugiyama, Akira, Takahashi, Tohru, The LCTPC Collaboration, Tian, Junping, Timmermans, Jan, Titov, Maksym, Tsionou, Dimitra, Vauth, Annika, Wang, Wenxin, Watanabe, Takashi, Werthenbach, Ulrich, Yang, Yifan, Yang, Zhenwei, Yonamine, Ryo, Zenker, Klaus, Zhang, Fan, Österman, Lennart +69 morecore +2 more sourcesA Dark Matter Hurricane: Measuring the S1 Stream with Dark Matter
Detectors [PDF]
, 2018 The recently discovered S1 stream passes through the Solar neighbourhood on a
low inclination, counter-rotating orbit. The progenitor of S1 is a dwarf galaxy
with a total mass comparable to the present-day Fornax dwarf spheroidal, so the
stream is ...Belokurov, Vasily, Evans, N. Wyn, McCabe, Christopher, Myeong, GyuChul, O'Hare, Ciaran A. J. +4 morecore +3 more sourcesFirst Demonstration of a Pixelated Charge Readout for Single-Phase
Liquid Argon Time Projection Chambers
, 2018 Liquid Argon Time Projection Chambers (LArTPCs) have been selected for the
future long-baseline Deep Underground Neutrino Experiment (DUNE). To allow
LArTPCs to operate in the high-multiplicity near detector environment of DUNE,
a new charge readout ...Asaadi, J., Auger, M., Ereditato, A., Goeldi, D., Haenni, R., Kose, U., Kreslo, I, Lorca, D., Luethi, M., Sinclair, J. R., Stocker, F., Tognina, C., Von Rohr, C. Rudolf, Weber, M. +13 morecore +1 more sourceProjected WIMP sensitivity of the LUX-ZEPLIN dark matter experiment [PDF]
, 2020 LUX-ZEPLIN (LZ) is a next-generation dark matter direct detection experiment that will operate 4850 feet underground at the Sanford Underground Research Facility (SURF) in Lead, South Dakota, USA. Using a two-phase xenon detector with an active mass of 7 Akerib, DS, Akerlof, CW, Alsum, SK, Araújo, HM, Arthurs, M, Bai, X, Bailey, AJ, Balajthy, J, Balashov, S, Bauer, D, Belle, J, Beltrame, P, Benson, T, Bernard, EP, Biesiadzinski, TP, Boast, KE, Boxer, B, Brás, P, Buckley, JH, Bugaev, VV, Burdin, S, Busenitz, JK, Carels, C, Carlsmith, DL, Carlson, B, Carmona-Benitez, MC, Chan, C, Cherwinka, JJ, Cole, A, Cottle, A, Craddock, WW, Currie, A, Cutter, JE, Dahl, CE, De Viveiros, L, Dobi, A, Dobson, JEY, Druszkiewicz, E, Edberg, TK, Edwards, WR, Fan, A, Fayer, S, Fiorucci, S, Fruth, T, Gaitskell, RJ, Genovesi, J, Ghag, C, Gilchriese, MGD, Hall, CR, Hans, S, Hanzel, K, Haselschwardt, SJ, Hertel, SA, Hillbrand, S, Hjemfelt, C, Hoff, MD, Hor, JYK, Huang, DQ, Ignarra, CM, Ji, W, Kaboth, AC, Kamdin, K, Keefner, J, Khaitan, D, Khazov, A, Kim, YD, Kocher, CD, Korolkova, EV, Kraus, H, Krebs, HJ, Kreczko, L, Krikler, B, Kudryavtsev, VA, Kyre, S, Lee, J, Lenardo, BG, Leonard, DS, Lesko, KT, Levy, C, Li, J, Liao, FT, Liao, J, Lin, J, Lindote, A, Linehan, R, Lippincott, WH, Liu, X, Lopes, MI, Lorenzon, W, Luitz, S, Lyle, JM, López Paredes, B, Majewski, P, Manalaysay, A, Mannino, RL, Maupin, C, McKinsey, DN, Meng, Y, Miller, EH, Van Der Grinten, MGD +99 morecore +1 more sourceBaby MIND: A magnetized segmented neutrino detector for the WAGASCI
experiment [PDF]
, 2017 T2K (Tokai-to-Kamioka) is a long-baseline neutrino experiment in Japan
designed to study various parameters of neutrino oscillations. A near detector
complex (ND280) is located 280~m downstream of the production target and
measures neutrino beam ...Antonova, M., Asfandiyarov, R., Bayes, R., Benoit, P., Blondel, A., Bogomilov, M., Bross, A., Cadoux, F., Cervera, A., Chikuma, N., Da Silva, H. Pais, Dudarev, A., Ekelöf, T., Favre, Y., Fedotov, S., Hallsjö, S-P., Izmaylov, A., Karadzhov, Y., Kate, H. Ten, Khabibullin, M., Khotyantsev, A., Kleymenova, A., Koga, T., Kostin, A., Kudenko, Y., Likhacheva, V., Martinez, B., Matev, R., Medvedeva, M., Mefodiev, A., Minamino, A., Mineev, O., Nessi, M., Nicola, L., Noah, E., Ovsiannikova, T., Parsa, S., Rayner, M., Rolando, G., Shaykhiev, A., Simion, P., Soler, F. J. P., Suvorov, S., Tsenov, R., Vankova-Kirilova, G., Yershov, N. +45 morecore +2 more sourcesSimulation of VUV electroluminescence in micropattern gaseous detectors:
the case of GEM and MHSP
, 2012 Electroluminescence produced during avalanche development in gaseous
avalanche detectors is an useful information for triggering, calorimetry and
tracking in gaseous detectors.Biagi, S., Correia, P. M. M., Ferreira, A. L., Monteiro, C. M. B., Oliveira, C. A. B., Santos, J. M. F. dos, Schindler, H., Veenhof, R., Veloso, J. F. C. A. +8 morecore +1 more sourceTime Response of Water-based Liquid Scintillator from X-ray Excitation
, 2020 Water-based liquid scintillators (WbLS) present an attractive target medium
for large-scale detectors with the ability to enhance the separation of
Cherenkov and scintillation signals from a single target.Bourret, Edith D., Caravaca, Javier, Gann, Gabriel D. Orebi, Moretti, Federico, Onken, Drew R., Yeh, Minfang +5 morecore +1 more sourceRemoving krypton from xenon by cryogenic distillation to the ppq level [PDF]
, 2017 The XENON1T experiment aims for the direct detection of dark matter in a
cryostat filled with 3.3 tons of liquid xenon. In order to achieve the desired
sensitivity, the background induced by radioactive decays inside the detector
has to be sufficiently ...A. Brown, A. D. Ferella, A. Di Giovanni, A. Fieguth, A. Gallo Rosso, A. Kish, A. Manfredini, A. Molinario, A. P. Colijn, A. Rizzo, A. Stein, A. Tiseni, B. Bauermeister, B. Kaminsky, B. Miguez, B. Pelssers, C. Geis, C. Grignon, C. Hasterok, C. Huhmann, C. Reuter, C. Tunnell, C. Weinheimer, D. Cichon, D. Coderre, D. Franco, D. Lellouch, D. Masson, D. Mayani, D. Thers, E. Aprile, E. Brown, E. Duchovni, E. Hogenbirk, E. Shockley, F. Agostini, F. Arneodo, F. D. Amaro, F. Gao, F. Piastra, F. V. Massoli, G. Bruno, G. Eurin, G. Kessler, G. Plante, G. Sartorelli, G. Trinchero, H. Landsman, H. Simgen, H. Wang, I. Cristescu, I. Maris, J. A. M. Lopes, J. Aalbers, J. Calvén, J. Conrad, J. Fei, J. M. F. dos Santos, J. M. R. Cardoso, J. Masbou, J. Naganoma, J. P. Cussonneau, J. Pienaar, J. Schreiner, J. Wulf, J. Ye, K. Micheneau, K. Ni, L. Baudis, L. Bütikofer, L. Grandi, L. Levinson, L. Rauch, L. Scotto Lavina, L. W. Goetzke, M. Alfonsi, M. Anthony, M. Cervantes, M. Galloway, M. Garbini, M. L. Benabderrahmane, M. Le Calloch, M. Lindner, M. Messina, M. Murra, M. P. Decowski, M. Scheibelhut, M. Schumann, M. Selvi, M. Silva, M. v. Sivers, M.-C. Piro, N. Priel, N. Rupp, N. Upole, P. A. Breur, P. Barrow, P. de Perio, P. Di Gangi, P. Pakarha, P. Shagin, Q. Lin, R. Budnik, R. F. Lang, R. Itay, R. Persiani, R. Saldanha, S. Bruenner, S. Diglio, S. E. A. Orrigo, S. Lindemann, S. Reichard, S. Rosendahl, S. Schindler, T. Berger, T. Marrodán Undagoitia, U. Oberlack, V. Pizzella, W. Fulgione, XENON Collaboration, Y. Meng, Y. Wei, Y. Zhang, Z. Greene +123 morecore +5 more sources
