Results 11 to 20 of about 77,537 (257)

Neutrino factory near detector [PDF]

Physical Review Special Topics. Accelerators and Beams, 2013
The neutrino factory is a facility for future precision studies of neutrino oscillations. A so-called near detector is essential for reaching the required precision for a neutrino oscillation analysis. The main task of the near detector is to measure the
M. Bogomilov, Y. Karadzhov, R. Matev, R. Tsenov, A. Laing, F. J. P. Soler   +5 more
doaj   +4 more sources

Invisible Labor and the "Ghost Particle": Underground Physics at the Kolar Gold Fields. [PDF]

Ber Wiss
Abstract When cosmic rays—high‐energy particles from outer space—encounter the Earth's atmosphere, they produce particles called neutrinos. To detect them, physicists go underground inside deep mines where the overlying rock can filter out the cosmic‐ray background radiation.
Rao N.
europepmc   +2 more sources

Theia: an advanced optical neutrino detector [PDF]

The European Physical Journal C, 2020
AbstractNew developments in liquid scintillators, high-efficiency, fast photon detectors, and chromatic photon sorting have opened up the possibility for building a large-scale detector that can discriminate between Cherenkov and scintillation signals.
Askins, M., Bagdasarian, Z., Barros, N., Beier, E. W., Blucher, E., Bonventre, R., Bourret, E., Callaghan, E. J., Caravaca, J., Diwan, M., Dye, S. T., Eisch, J., Elagin, A., Enqvist, T., Fischer, V., Frankiewicz, K., Grant, C., Guffanti, D., Hagner, C., Hallin, A., Jackson, C. M., Jiang, R., Kaptanoglu, T., Klein, J. R., Kolomensky, Yu. G., Kraus, C., Krennrich, F., Kutter, T., Lachenmaier, T., Land, B., Lande, K., Learned, J. G., Lozza, V., Ludhova, L., Malek, M., Manecki, S., Maneira, J., Maricic, J., Martyn, J., Mastbaum, A., Mauger, C., Moretti, F., Napolitano, J., Naranjo, B., Nieslony, M., Oberauer, L., Orebi , Gann, G. D., Ouellet, J., Pershing, T., Petcov, S. T., Pickard, L., Rosero, R., Sanchez, M. C., Sawatzki, J., Seo, S. H., Smiley, M., Smy, M., Stahl, A., Steiger, H., Stock, M. R., Sunej, H., Svoboda, R., Tiras, E., Trzaska, W. H., Tzanov, M., Vagins, M., Vilela, C., Wang, Z., Wang, J., Wetstein, M., Wilking, M. J., Winslow, L., Wittich, P., Wonsak, B., Worcester, E., Wurm, M., Yang, G., Yeh, M., Zimmerman, E. D., Zsoldos, S., Zuber, K.   +81 more
openaire   +11 more sources

Stodolsky's Theorem and Neutrino Oscillation Phases -- for pedestrians [PDF]

, 2002
Neutrino oscillations are experimentally observable only as a result of interference between neutrino states with different masses and THE SAME ENERGY.
Lipkin, Harry J.
core   +6 more sources

Physics Potential of the ICAL detector at the India-based Neutrino Observatory (INO) [PDF]

, 2017
The upcoming 50 kt magnetized iron calorimeter (ICAL) detector at the India-based Neutrino Observatory (INO) is designed to study the atmospheric neutrinos and antineutrinos separately over a wide range of energies and path lengths.
Acharya, B. S., Agarwalla, Sanjib Kumar, Ahmed, Shakeel, Ajmi, Ali, Athar, M. Sajjad, Banerjee, Sudeshna, Bari, Waseem, Behera, Prafulla, Behera, Shiba Prasad, Bhatnagar, Vipin, Bhattacharya, Kolahal, Bhattacharya, Sudeb, Biswas, Saikat, Bose, Suvendu, Chacko, Aleena, Chandratre, Vinay B., Chatterjee, Animesh, Chattopadhyay, Subhasis, Choubey, Sandhya, Choudhary, Brajesh C., Dasgupta, Sudeshna, Dash, Nitali, Datar, Vivek M., Devi, Moon Moon, Dighe, Amol, Ganai, Rajesh, Gandhi, Raj, Gangopadhyay, Gautam, Gaur, Ankit, Ghosal, Ambar, Ghosh, Anushree, Ghosh, Monojit, Ghosh, Tapasi, Ghoshal, Pomita, Goswami, Srubabati, Gupta, Chandan, Hasan, Rashid, Inbanathan, S. S. R., Indumathi, D., Jafer, Sadiq, Jash, Abhik, Kanishka, R., Kar, Kamalesh, Kashyap, V. K. S., Kaur, Daljeet, Khatun, Amina, Krishnaveni, S., Kumar, A., Kumar, Ashok, Kumar, Sanjeev, Lakshmi, S. M., Libby, James, Mahapatra, Swapna, Majumdar, Debasish, Majumdar, Nayana, Majumder, Gobinda, Malik, Manzoor A., Meghna, K., Mehta, Poonam, Mohanty, Ajit K., Mondal, Naba K., Mukhopadhyay, Supratik, Murthy, M. V. N., Naimuddin, Md., Pal, Sumanta, Pant, Lalit M., Rajasekaran, G., Ranganathaiah, C., Raut, Sushant, Raveendrababu, K., Ravikumar, C. D., Ravikumar, H. B., Raychaudhuri, Amitava, Rebin, K. R., Redij, Asmita, Saha, Satyajit, Salim, Mohammad, Samuel, Deepak, Sankar, S. Uma, Satyanarayana, B., Shahi, J. S., Singh, J. B., Singh, Jyotsna, Singh, S. K., Singh, Venktesh, Sinha, Nita, Subrahmanyam, V. S., Thakore, Tarak, The ICAL Collaboration, Tiwari, Deepak, Vinodkumar, A. M., Viyogi, Y. P.   +91 more
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A xenon solar neutrino detector [PDF]

Astroparticle Physics, 1997
The neutrino capture by $^{131}$Xe with a threshold at 352 keV as reaction to detect solar neutrinos is examined. The most important feature of this process is its high sensitivity to beryllium neutrinos, which contribute approximately 40% to the total capture rate (45 SNU) assuming the fluxes predicted by the Standard Solar Model.
Georgadze, A. Sh., Klapdor-Kleingrothaus, H. V., Päs, H., Zdesenko, Yu. G.   +3 more
openaire   +2 more sources

MINERvA: a dedicated neutrino scattering experiment at NuMI [PDF]

, 2006
MINERvA is a dedicated neutrino cross-section experiment planned for the near detector hall of the NuMI neutrino beam at Fermilab. I summarize the detector design and physics capabilities of the experiment.Comment: Comments: to appear in the proceedings ...
Arrington, Baker, Drakoulakos, Fisyak, Harris, Hasegawa, K.S. McFarland, Kitagaki, Miller, Zeller   +9 more
core   +3 more sources

Double neutrino production and detection in neutrino detectors [PDF]

Physical Review D, 2013
Large, high-energy ($E>100$ GeV) cosmic neutrino telescopes are now quite mature. IceCube, for example, observes about 50,000 well-reconstructed single atmospheric neutrino events/year, with energies above 100 GeV. Although the neutrino detection probability is small, current detectors are large enough so that it is possible to detect two neutrinos ...
van der Drift, Don, Klein, Spencer R.
openaire   +2 more sources

Probing invisible neutrino decay with KM3NeT/ORCA

Journal of High Energy Physics, 2023
In the era of precision measurements of the neutrino oscillation parameters, upcoming neutrino experiments will also be sensitive to physics beyond the Standard Model.
The KM3NeT collaboration, S. Aiello, A. Albert, S. Alves Garre, Z. Aly, A. Ambrosone, F. Ameli, M. Andre, M. Anghinolfi, M. Anguita, M. Ardid, S. Ardid, J. Aublin, C. Bagatelas, L. Bailly-Salins, B. Baret, S. Basegmez du Pree, Y. Becherini, M. Bendahman, F. Benfenati, E. Berbee, V. Bertin, S. Biagi, M. Boettcher, M. Bou Cabo, J. Boumaaza, M. Bouta, M. Bouwhuis, C. Bozza, H. Brânzaş, R. Bruijn, J. Brunner, R. Bruno, E. Buis, R. Buompane, J. Busto, B. Caiffi, D. Calvo, S. Campion, A. Capone, F. Carenini, V. Carretero, P. Castaldi, S. Celli, L. Cerisy, M. Chabab, N. Chau, A. Chen, R. Cherkaoui El Moursli, S. Cherubini, V. Chiarella, T. Chiarusi, M. Circella, R. Cocimano, J. A. B. Coelho, A. Coleiro, R. Coniglione, P. Coyle, A. Creusot, A. Cruz, G. Cuttone, R. Dallier, Y. Darras, A. De Benedittis, B. De Martino, V. Decoene, R. Del Burgo, I. Di Palma, A. F. Díaz, D. Diego-Tortosa, C. Distefano, A. Domi, C. Donzaud, D. Dornic, M. Dörr, E. Drakopoulou, D. Drouhin, T. Eberl, A. Eddyamoui, T. van Eeden, M. Eff, D. van Eijk, I. El Bojaddaini, S. El Hedri, A. Enzenhöfer, V. Espinosa, G. Ferrara, M. D. Filipović, F. Filippini, L. A. Fusco, J. Gabriel, T. Gal, J. García Méndez, A. Garcia Soto, F. Garufi, C. Gatius Oliver, N. Geißelbrecht, L. Gialanella, E. Giorgio, A. Girardi, I. Goos, S. R. Gozzini, R. Gracia, K. Graf, D. Guderian, C. Guidi, B. Guillon, M. Gutiérrez, L. Haegel, H. van Haren, A. Heijboer, A. Hekalo, L. Hennig, J. J. Hernández-Rey, F. Huang, W. Idrissi Ibnsalih, G. Illuminati, C. W. James, D. Janezashvili, M. de Jong, P. de Jong, B. J. Jung, P. Kalaczyński, O. Kalekin, U. F. Katz, N. R. Khan Chowdhury, G. Kistauri, F. van der Knaap, P. Kooijman, A. Kouchner, V. Kulikovskiy, M. Labalme, R. Lahmann, A. Lakhal, M. Lamoureux, G. Larosa, C. Lastoria, A. Lazo, R. Le Breton, S. Le Stum, G. Lehaut, E. Leonora, N. Lessing, G. Levi, S. Liang, M. Lindsey Clark, F. Longhitano, L. Maderer, J. Majumdar, J. Mańczak, A. Margiotta, A. Marinelli, C. Markou, L. Martin, J. A. Martínez-Mora, A. Martini, F. Marzaioli, M. Mastrodicasa, S. Mastroianni, K. W. Melis, S. Miccichè, G. Miele, P. Migliozzi, E. Migneco, P. Mijakowski, C. M. Mollo, L. Morales-Gallegos, C. Morley-Wong, A. Moussa, R. Muller, M. R. Musone, M. Musumeci, L. Nauta, S. Navas, C. A. Nicolau, B. Nkosi, B. Ó Fearraigh, A. Orlando, E. Oukacha, J. Palacios González, G. Papalashvili, R. Papaleo, E. J. Pastor Gomez, A. M. Păun, G. E. Păvălaş, C. Pellegrino, S. Peña Martínez, M. Perrin-Terrin, J. Perronnel, V. Pestel, P. Piattelli, O. Pisanti, C. Poirè, V. Popa, T. Pradier, S. Pulvirenti, G. Quéméner, U. Rahaman, N. Randazzo, S. Razzaque, I. C. Rea, D. Real, S. Reck, G. Riccobene, J. Robinson, A. Romanov, F. Salesa Greus, D. F. E. Samtleben, A. Sánchez Losa, M. Sanguineti, C. Santonastaso, D. Santonocito, P. Sapienza, A. Sathe, J. Schnabel, M. F. Schneider, J. Schumann, H. M. Schutte, J. Seneca, I. Sgura, R. Shanidze, A. Sharma, A. Simonelli, A. Sinopoulou, M. V. Smirnov, B. Spisso, M. Spurio, D. Stavropoulos, S. M. Stellacci, M. Taiuti, K. Tavzarashvili, Y. Tayalati, H. Tedjditi, T. Thakore, H. Thiersen, S. Tsagkli, V. Tsourapis, E. Tzamariudaki, V. Van Elewyck, G. Vannoye, G. Vasileiadis, F. Versari, S. Viola, D. Vivolo, H. Warnhofer, J. Wilms, E. de Wolf, H. Yepes-Ramirez, T. Yousfi, S. Zavatarelli, A. Zegarelli, D. Zito, J. D. Zornoza, J. Zúñiga, N. Zywucka   +254 more
doaj   +1 more source

Calibration of Super-Kamiokande Using an Electron Linac [PDF]

, 1998
In order to calibrate the Super-Kamiokande experiment for solar neutrino measurements, a linear accelerator (LINAC) for electrons was installed at the detector.
A Habig, A Hasegawa, A Kibayashi, A Okada, A Sakai, A Suzuki, A.L Stachyra, A.T Suzuki, Abdurashitov, B Viren, B.K Kim, C Mauger, C McGrew, C Saji, C Yanagisawa, C.K Jung, C.W Walter, D Casper, D Kielczewska, D Takemori, E Blaufuss, E Ichihara, E Kearns, E Sharkey, F Reines, F Tsushima, Fukuda, G.W Sullivan, H Ishino, H Kobayashi, H Ogawa, H Okazawa, H.W Sobel, Hampel, Hata, Hirata, J Hill, J Hsu, J Kameda, J Kanzaki, J Shirai, J.A Goodman, J.G Learned, J.L Stone, J.S George, J.W Flanagan, K Fujita, K Inoue, K Ishihara, K Kaneyuki, K Kobayashi, K Martens, K Miyano, K Nakamura, K Nishijima, K Nishikawa, K Okumura, K Scholberg, K.K Young, K.S Ganezer, L.L Wai, L.R Price, L.R Sulak, M Earl, M Etoh, M Goldhaber, M Koga, M Kohama, M Koshiba, M Miura, M Nakahata, M Nemoto, M Sakuda, M Shiozawa, M Smy, M Takahata, M Takita, M Yoshida, M.D Messier, M.L Chen, M.R Vagins, N Sakurai, O Sasaki, P.G Halverson, R Sanford, R Svoboda, R.A Doyle, R.J Wilkes, R.W Ellsworth, S Echigo, S Hatakeyama, S Kasuga, S Matsuno, S Mine, S Nakayama, S Tasaka, S Yamada, S.B Kim, Suzuki, T Barszczak, T Futagami, T Hasegawa, T Hayakawa, T Ishii, T Iwamoto, T Kajita, T Kobayashi, T Maruyama, T Yamaguchi, T.J Haines, V.J Stenger, W Doki, W Gajewski, W.E Keig, W.R Kropp, Y Fukuda, Y Hayato, Y Itow, Y Kanaya, Y Kobayashi, Y Koshio, Y Nagashima, Y Oyama, Y Suzuki, Y Takeuchi, Y Totsuka, Y Watanabe, Z Conner   +127 more
core   +2 more sources