Improving Photoelectron Counting and Particle Identification in Scintillation Detectors with Bayesian Techniques

Autor: Laurelle Maria Veloce, I. T. Lawson, P. Liimatainen, J. R. Klein, Y. Chen, B. Buck, K. Graham, S. Jaditz, T. Sonley, T. S. Caldwell, Natalia Guerrero, V. E. Guiseppe, Dongming Mei, D. Gastler, M. Bodmer, M. Kuźniak, B. T. Cleveland, T. Pollmann, J. Wang, F. Giuliani, G. D. Orebi Gann, E. O'Dwyer, C. M. Nantais, P. Amaudruz, Martin Ward, M. Akashi-Ronquest, A. Muir, C. Zhang, C. J. Jillings, Keith Rielage, James Nikkel, Andrew Hime, B. Beltran, C. Kachulis, J. Kelsey, R. W. Schnee, K. Dering, Jocelyn Monroe, C. Ouellet, S. MacMullin, A. Mastbaum, J. Walding, O. Li, A. B. McDonald, S. Linden, V. V. Golovko, P. Skensved, R. Mathew, F. Duncan, F. Retiere, B. Wang, Bei Cai, A. Butcher, A. Latorre, K. McFarlane, A. L. Hallin, P. Rau, B. Broerman, M. Gold, E. Vázquez-Jáuregui, Daniel McKinsey, J. Hofgartner, Min Chen, K. S. Olsen, Reyco Henning, Joseph A. Formaggio, J. Lidgard, K. Palladino, P. Pasuthip, E. Kearns, E. Grace, P. J. Harvey, K. Nicolics, R. Gagnon, C. Hearns, Kevin J. Coakley, P. Gorel, M. Batygov, S. Seibert, T. Noble, G. Perumpilly, Mark Guy Boulay

Publikováno v: arXiv

Many current and future dark matter and neutrino detectors are designed to measure scintillation light with a large array of photomultiplier tubes (PMTs). The energy resolution and particle identification capabilities of these detectors depend in par

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https://ora.ox.ac.uk/objects/uuid:ec965ed6-4b60-4f86-b9b9-e95bed844ccc

SEARCHES FOR HIGH-FREQUENCY VARIATIONS IN THE B-8 SOLAR NEUTRINO FLUX AT THE SUDBURY NEUTRINO OBSERVATORY

Autor: E. D. Hallman, G. Prior, Benjamin Monreal, E. D. Earle, P. J. Doe, S. J. M. Peeters, K. J. Keeter, T. Tsui, F. A. Duncan, P. Skensved, M. DiMarco, K. Boudjemline, Yuen-Dat Chan, J. M. Wouters, J. Heise, S. Habib, K. Graham, X. Dai, S. M. Oser, J. A. Detwiler, Keith Rielage, H. Wan Chan Tseung, M. L. Miller, A. B. McDonald, R. D. Martin, Andrew Hime, I. Levine, Jocelyn Monroe, Alain Bellerive, D. L. Wark, R. J. Ford, T. J. Sonley, R. L. Hahn, H. Fergani, R. G. H. Robertson, M. H. Schwendener, R. MacLellan, Monica Dunford, J. Maneira, B. Beltran, Mark Guy Boulay, Bei Cai, David A. Sinclair, C. A. Duba, F. Zhang, J. Law, D. Chauhan, Peter Watson, B. Jamieson, A. W. P. Poon, Christopher C. M. Kyba, P.-L. Drouin, N. Tolich, C. B. Krauss, N. S. Oblath, B. Aharmim, T.H. Burritt, Kai Zuber, C. D. Tunnell, A. L. Hallin, R. L. Helmer, B. Morissette, J. A. Secrest, I. T. Lawson, C. Kraus, B. T. Cleveland, S. R. Seibert, D. Waller, G. A. Cox, R. A. Ott, N. West, W. J. Heintzelman, K. T. Lesko, J. R. Wilson, M. Kos, A. Wright, O. Simard, E. W. Beier, B.A. VanDevender, L. C. Stonehill, C. Howard, J. Farine, A. J. Noble, C. J. Virtue, B. C. Robertson, G. Doucas, E. Guillian, T. Kutter, N. Barros, Joseph A. Formaggio, Minfang Yeh, J. C. Loach, N. A. Jelley, Hal Evans, S. D. Reitzner, S. N. Ahmed, Joshua R. Klein, M. Bergevin, N. McCauley, R. Van Berg, M. L. Chen, S. Majerus, L. L. Kormos, G. T. Ewan, N. Gagnon, R. Hazama, G. D. Orebi Gann, H. Deng, B. L. Wall, H. M. O'Keeffe, H. B. Mak, S. McGee, S. D. Biller, Bernie G. Nickel, P. J. Harvey, J. F. Wilkerson, Steven Elliott, M. A. Howe, M. Huang, G. Tešić, J. R. Leslie, F. Fleurot, A. E. Anthony, J. Tm. Goon

We have performed three searches for high-frequency signals in the solar neutrino flux measured by the Sudbury Neutrino Observatory (SNO), motivated by the possibility that solar $g$-mode oscillations could affect the production or propagation of sol

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https://doi.org/10.1088/0004-637x/710/1/540

Astroparticle physics with a customized low-background broad energy Germanium detector

Autor: L. E. Leviner, L. Mizouni, Paul N. Luke, S. R. Elliott, Andrew Hime, Craig E. Aalseth, W. Bugg, Reynold J. Cooper, H. Salazar, A. S. Barabash, H. A. Farach, S. I. Konovalov, M. L. Miller, Chao Zhang, J. I. Collar, O.I. Kochetov, K. Gusey, J. Strain, G. K. Giovanetti, S. Zimmerman, D. Steele, V. Egorov, R. D. Martin, F. T. Avignone, Henning O. Back, Eric W. Hoppe, R. L. Varner, Mark Amman, Yu. Efremenko, D.A. Peterson, Reyco Henning, C. Keller, Harry S. Miley, H. Yaver, A. Knecht, Keenan Thomas, V. V. Timkin, Dongming Mei, J. Esterline, J. Kephart, D. G. Phillips, J. Qian, James E. Fast, M. Bergevin, P. J. Doe, J. C. Loach, Yuen-Dat Chan, R. G. H. Robertson, G. C. Harper, J. Diaz, E. Yakushev, A. L. Hallin, T. D. Van Wechel, W. Xiang, M. F. Kidd, K. J. Keeter, V.B. Brudanin, Keith Rielage, M. Shirchenko, Alexis G. Schubert, Erin S. Fuller, N. Fields, R.A. Johnson, John L. Orrell, B. K. Fujikawa, K. P. Rykaczewski, Michael G. Marino, L. Rodriguez, Albert Young, Tatsushi Shima, S. MacMullin, F. E. Bertrand, M. A. Howe, R. J. Creswick, M. Boswell, H. Ejiri, Todd W. Hossbach, G. Capps, Chang-Hong Yu, V. M. Gehman, V. E. Guiseppe, Kai Vetter, Masaharu Nomachi, Ryuta Hazama, G. Swift, James H. Ely, Martin E. Keillor, Richard T. Kouzes, Werner Tornow, D. C. Radford, G. Prior, Matthew Busch, J. F. Wilkerson, P. Finnerty, B. A. Wolfe, P. S. Barbeau, Vladimir Yumatov, T.H. Burritt, Alan Poon, J. A. Detwiler, I. Vanyushin, A. W. Meyers

Publikováno v: Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 652:692-695

The MAJORANA Collaboration is building the MAJORANA DEMONSTRATOR, a 60 kg array of high purity germanium detectors housed in an ultra-low background shield at the Sanford Underground Laboratory in Lead, SD. The MAJORANA DEMONSTRATOR will search for n

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https://doi.org/10.1016/j.nima.2010.08.100

Advances in High Energy Physics

Autor: Jilei Xu, O. Smirnov, A. Alton, Y. Suvurov, Nicomede Pelliccia, B. Reinhold, N. Canci, D. A. Semenov, D. Sablone, M. D. Skorokhvatov, L. Grandi, M. Montuschi, An. Ianni, Mariano Cadoni, E. Pantic, K. Herner, P. J. Mosteiro, L. Crippa, I. N. Machulin, A. Nelson, Bob Parsells, G. Lukyachenko, Al. Ianni, Y. Q. Ma, L. Marini, M. Bossa, Peter Daniel Meyers, John L. Orrell, V. N. Muratova, E. Segreto, D. M. Asner, G. Zuzel, N. Rossi, A. Mandarano, R. Milincic, Hui Wang, Henning O. Back, M. Wada, K. Biery, J. Yoo, Marco Pallavicini, Stefano Maria Mari, S. Westerdale, Y. Guardincerri, E. Edkins, A. Fan, S. Parmeggiano, D. A. Pugachev, D. D'Angelo, F. Budano, Livia Ludhova, L. Perasso, A. Kurlej, R. Tartaglia, Alan Watson, V. V. Kobychev, A. M. Goretti, A. S. Chepurnov, G. Forster, M. Orsini, D. E. Jaffe, F. Di Eusanio, M. De Deo, K. Arisaka, E. Meroni, J. Tatarowicz, Aldo Romani, A. V. Derbin, G. Fiorillo, K. Fomenko, P. Humble, S. Kidner, P. Agnes, Gioacchino Ranucci, D. Franco, S. Davini, Marcin Wójcik, E. V. Unzhakov, E. V. Hungerford, W. Zhong, Cécile Jollet, A. Devoto, Samuele Sangiorgio, Sandra Zavatarelli, M. Cariello, L. Pagani, C. L. Kendziora, M. D'Incecco, Anselmo Meregaglia, P. X. Li, T. Miletic, H. Qian, A. Sotnikov, P. Saggese, J. Brodsky, E. Shields, Craig E. Aalseth, W. Sands, S. Perasso, B. Rossi, G. Bonfini, B. Yu, K. Recine, H. Cao, K. Randle, B. Baldin, Andrzej Odrzywolek, R. Saldanha, S. Walker, R. Williams, Marcello Lissia, S. D. Rountree, S. Pordes, F. Gabriele, Michael Foxe, Paolo Lombardi, D. Markov, B. R. Hackett, G. Koh, A. Empl, S. Odrowski, M. E. Monzani, A. Tonazzo, Yanchu Wang, A. Pocar, A. Candela, Chung-Yao Yang, G. Testera, Augusto Brigatti, C. Condon, K. Pelczar, Cristiano Galbiati, P. Musico, J. Martoff, M. Gromov, D. Montanari, Andrew Hime, M. Smallcomb, J. Maricic, S. Luitz, A. Razeto, B. J. Mount, A. G. Cocco, D. Korablev, K. J. Keeter, Frank Calaprice, R. B. Vogelaar, Laura Cadonati, A. L. Renshaw, Fausto Ortica, P. Cavalcante, Min-Xin Guan, G. Korga

Publikováno v: Advances in High Energy Physics, Vol 2015 (2015)
ResearcherID
Advances in High Energy Physics

Although the existence of dark matter is supported by many evidences, based on astrophysical measurements, its nature is still completely unknown. One major candidate is represented by weakly interacting massive particles (WIMPs), which could in prin

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http://hdl.handle.net/11588/593379

The proposed Majorana 76Ge double-beta decay experiment

Autor: John L. Orrell, Kai Vetter, Albert Young, R. Hazma, R. G. Van de Water, R. W. Creswick, Robert C. Runkle, S. R. Elliott, V. B. Brudanin, F. T. Avignone, Yu. Efremenko, Harry S. Miley, Craig E. Aalseth, K. Saburov, J. F. Wilkerson, T. V. Cianciolo, H. Ejiri, Reyco Henning, Todd W. Hossbach, Richard J. Arthur, A. O. Macchiavelli, G. S. King, H. A. Farach, S. I. Konovalov, T. Ball, W. Bugg, A. L. Hallin, V. Egerov, David V. Jordan, K. P. Rykaczewski, Richard T. Kouzes, Martina Descovich, Andrew Sonnenschein, I. Vanushin, Alan Poon, V. M. Gehman, Y. Sandukovsky, J. H. Reeves, J. M. Wouters, Masaharu Nomachi, J. M. Palms, Paul N. Luke, A. B. McDonald, M. Di Marco, A. Mokhtarani, J. Kephart, A. S. Barabash, J. I. Collar, F. E. Bertrand, P. J. Doe, Yuen-Dat Chan, G. B. Mills, Dongming Mei, P. Fallon, R. J. Gaitskell, R. G. H. Robertson, Ronald L. Brodzinski, C. Baktash, O.I. Kochetov, Arthur E Champagne, M. Luzum, R. A. Warner, Robert Grzywacz, Andrew Hime, G. Dunham, D. Anderson, K. T. Lesko, K. Kazkaz, Werner Tornow, C. E. Tull, D. C. Radford, Vladimir Yumatov, A. Emanuel

Publikováno v: Nuclear Physics B - Proceedings Supplements. 138:217-220

The proposed Majorana experiment is based on an array of segmented intrinsic Ge detectors with a total mass of 500 kg of Ge isotopically enriched to 86% in 76 Ge. Background reduction will be accomplished by: material selection, detector segmentation

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::12bef27c34b2cb70adb6313a93ec1f03
https://doi.org/10.1016/j.nuclphysbps.2004.11.052