Results 11 to 20 of about 171,820 (251)

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   +5 more sources

High-rate neutrino detectors for neutrino factories [PDF]

Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 2000
Three types of high rate neutrino detectors for neutrino interaction physics at neutrino factories are discussed. High performance general-purpose detectors might collect event samples on the order of a billion events or more. This could greatly improve on existing analyses of neutrino interactions and also lead to new and important analysis topics ...
B.J. King
openalex   +5 more sources

A relic neutrino detector [PDF]

Second international workshop on particle physics and the early universe (COSMO-98), 1999
Probably the most promising way of detecting cosmic neutrinos is measuring the mechanical force exerted by elastic scattering of cosmic neutrinos from macroscopic targets. The expected acceleration is $\sim 10^{-23} cm/s^2$ for Dirac neutrinos of mass $\sim 10 eV$ and local density $\sim 10^7/ cm^3$. A novel torsion balance design is presented.
C. Hagmann
openalex   +6 more sources

Toroidal magnetized iron neutrino detector for a neutrino factory [PDF]

Physical Review Special Topics. Accelerators and Beams, 2013
A neutrino factory has unparalleled physics reach for the discovery and measurement of CP violation in the neutrino sector. A far detector for a neutrino factory must have good charge identification with excellent background rejection and a large mass ...
A. Bross, R. Wands, R. Bayes, A. Laing, F. J. P. Soler, A. Cervera Villanueva, T. Ghosh, J. J. Gómez Cadenas, P. Hernández, J. Martín-Albo, J. Burguet-Castell   +10 more
doaj   +6 more sources

Neutrino physics with an opaque detector [PDF]

Communications Physics, 2021
AbstractIn 1956 Reines & Cowan discovered the neutrino using a liquid scintillator detector. The neutrinos interacted with the scintillator, producing light that propagated across transparent volumes to surrounding photo-sensors. This approach has remained one of the most widespread and successful neutrino detection technologies used since.
A. Cabrera, A. Abusleme, J. dos Anjos, T. J. C. Bezerra, M. Bongrand, C. Bourgeois, D. Breton, C. Buck, J. Busto, E. Calvo, E. Chauveau, M. Chen, P. Chimenti, F. Dal Corso, G. De Conto, S. Dusini, G. Fiorentini, C. Frigerio Martins, A. Givaudan, P. Govoni, B. Gramlich, M. Grassi, Y. Han, J. Hartnell, C. Hugon, S. Jiménez, H. de Kerret, A. Le Nevé, P. Loaiza, J. Maalmi, F. Mantovani, L. Manzanillas, C. Marquet, J. Martino, D. Navas-Nicolás, H. Nunokawa, M. Obolensky, J. P. Ochoa-Ricoux, G. Ortona, C. Palomares, F. Pessina, A. Pin, J. C. C. Porter, M. S. Pravikoff, M. Roche, B. Roskovec, N. Roy, C. Santos, S. Schoppmann, A. Serafini, L. Simard, M. Sisti, L. Stanco, V. Strati, J.-S. Stutzmann, F. Suekane, A. Verdugo, B. Viaud, C. Volpe, C. Vrignon, S. Wagner, F. Yermia   +61 more
openaire   +10 more sources

Atmospheric neutrino physics with the MACRO detector [PDF]

Nuclear Physics B - Proceedings Supplements, 2000
7 pages, 7 figures. Invited talk at 6th Topical Seminar on Neutrino and AstroParticle Physics, San Miniato, Italy, 17-21 May ...
M. Spurio
openalex   +7 more sources

Neutrino Astronomy with the MACRO Detector [PDF]

The Astrophysical Journal, 2001
High energy gamma ray astronomy is now a well established field and several sources have been discovered in the region from a few GeV up to several TeV. If sources involving hadronic processes exist, the production of photons would be accompanied by neutrinos too.
A. Sciubba, C. De Marzo, Alec Habig, A. Rainò, V. Bisi, Mario Sitta, Donato Nicolo, Donato Nicolo, L. R. Sulak, M. Vakili, N. Giglietto, G. Mandrioli, M. De Vincenzi, E. Vilela, O. Palamara, D. Bakari, L. Perrone, M. Spinetti, J. Derkaoui, Eugenio Scapparone, F. Maaroufi, Halina Bilokon, C. Bemporad, G. Giannini, G. Giannini, A. A. Grillo, D. Levin, R. Pazzi, E. Lamanna, E. Lamanna, M. Grassi, S. L. Mufson, Kael Hanson, Annarita Margiotta, C. Satriano, M. Brigida, P. Bernardini, P. Spinelli, R. Antolini, G. Battistoni, F. Cafagna, S. Petrera, J. Reynoldson, Maurizio Spurio, P. Monacelli, M. Carboni, C. Forti, C. Favuzzi, E. Iarocci, L. Miller, L. Miller, Severino Angelo Maria Bussino, H. Dekhissi, M. Ouchrif, C. Bloise, C. Okada, R. Steinberg, S. Kyriazopoulou, R.M. Heinz, P. Serra, A. Marzari-Chiesa, L. Patrizii, Michael J. Longo, Frederic Jean Ronga, J. A. Musser, A. Baldini, Erik Katsavounidis, A. Di Credico, Roberto Bellotti, Paolo Lipari, D. Campana, Vincenzo Patera, Shahid Manzoor, Shahid Manzoor, Marco Monteno, Andrea Carlo Marini, S. Cecchini, J. L. Stone, C. W. Peck, C. W. Walter, C. W. Walter, M. Calicchio, C. Gustavino, F. Loparco, V. Chiarella, C. Orth, Gregory Tarle, Ioannis Katsavounidis, Kate Scholberg, C. R. Bower, G. Auriemma, D. G. Michael, V. Popa, E. Kearns, G. Mancarella, Np Longley, Np Longley, Lindsey Gray, R. Nolty, G. Giacomelli, O. Enriquez, G. de Cataldo, L. Satta, Hyun-Chul Kim, F. Guarino, Maximiliano Sioli, Teresa Montaruli, V. Togo, A. Surdo, G. C. Barbarino, R. C. Webb, M. N. Mazziotta, M. Ambrosio, P. Pistilli, S P Mikheyev, S P Mikheyev, M. Giorgini, S. Coutu, S. Coutu, I. De Mitri, Barry C. Barish, Fabrizio Cei, D. Martello, C. E. Lane, P. Fusco, G. Osteria, B. C. Choudhary   +126 more
openaire   +11 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.
Joshua R. Klein, Julia Sawatzki, S. T. Petcov, A. Mastbaum, S. Manecki, S. Manecki, M. Nieslony, R. Bonventre, M. Tzanov, Yu G. Kolomensky, Yu G. Kolomensky, Timo Enqvist, V. Lozza, J. Wang, Jonathan Ouellet, Tobias Lachenmaier, Minfang Yeh, H. Steiger, S. Zsoldos, S. Zsoldos, E. J. Callaghan, E. J. Callaghan, G. Yang, M. Askins, M. Askins, B. J. Land, B. J. Land, B. J. Land, N. Barros, N. Barros, E. Blucher, A. Elagin, M. V. Diwan, T. Kutter, Livia Ludhova, Frank Krennrich, J. D. Eisch, D. Guffanti, L. Oberauer, Peter Wittich, John G. Learned, T. Kaptanoglu, M. J. Wilking, M. Vagins, C. Grant, Ziyue Wang, K. Lande, Jim Napolitano, B. Naranjo, Stephen T. Dye, J. Maneira, E. D. Zimmerman, E. Tiras, Caren Hagner, L. Pickard, Matthias Raphael Stock, R. Jiang, Z. Bagdasarian, E. W. Beier, Lindley Winslow, J. Maricic, J. Martyn, Bjoern Wonsak, J. Caravaca, J. Caravaca, G. D. Orebi Gann, G. D. Orebi Gann, T. Pershing, A. L. Hallin, Michael Wurm, E. Worcester, E. Worcester, Kai Zuber, M. Smiley, M. Smiley, F. Moretti, M. Malek, Achim Stahl, M. C. Sanchez, C. Vilela, H. Sunej, C. Mauger, Robert Svoboda, S. H. Seo, C. M. Jackson, E. Bourret, R. Rosero, M. Wetstein, K. Frankiewicz, V. Fischer, Wladyslaw Henryk Trzaska, Michael B. Smy, C. Kraus   +92 more
openaire   +10 more sources

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.
Hans Volker Klapdor-Kleingrothaus, A.Sh. Georgadze, Yu.G. Zdesenko, H. Päs   +3 more
openaire   +4 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 ...
Don van der Drift, S. R. Klein
openaire   +3 more sources