Results 1 to 10 of about 633 (111)

Neutrino interactions in the late universe [PDF]

Journal of High Energy Physics, 2021
The cosmic neutrino background is both a dramatic prediction of the hot Big Bang and a compelling target for current and future observations. The impact of relativistic neutrinos in the early universe has been observed at high significance in a number of
Daniel Green, David E. Kaplan, Surjeet Rajendran   +2 more
doaj   +2 more sources

Reconstructing Neutrino Energy using CNNs for GeV Scale IceCube Events [PDF]

International Conference on Rebooting Computing, 2021
Measurements of neutrinos at and below 10 GeV provide unique constraints of neutrino oscillation parameters as well as probes of potential Non-Standard Interactions (NSI).
J. Micallef
semanticscholar   +1 more source

Wide angle acceptance and high-speed track recognition in nuclear emulsion [PDF]

Progress of Theoretical and Experimental Physics, 2021
A nuclear emulsion film is a three-dimensional tracking device that is widely used in cosmic-ray and high energy physics experiments. Scanning with a wide angle acceptance is crucial for obtaining track information in emulsion films.
Y. Suzuki, T. Fukuda, H. Kawahara, R. Komatani, M. Naiki, T. Nakano, T. Odagawa, M. Yoshimoto   +7 more
semanticscholar   +1 more source

Measurement of sound speed vs. depth in South Pole ice for neutrino astronomy [PDF]

Astroparticle Physics, 2010
14 pages, 7 ...
Abbasi R., Abdou Y., Ackermann M., Adams J., Aguilar J. A., Ahlers M., Andeen K., Auffenberg J., Bai X., Baker M., Barwick S. W., Bay R., Bazo Alba J. L., Beattie K., Beatty J. J., Bechet S., Becker J. K., Becker K. -H., Benabderrahmane M. L., Berdermann J., Berghaus P., Berley D., Bernardini E., Bertrand D., Besson D. Z., Bissok M., Blaufuss E., Boersma D. J., Bohm C., Bolmont J., Boser S., Botner O., Bradley L., Braun J., Breder D., Castermans T., Chirkin D., Christy B., Clem J., Cohen S., Cowen D. F., D'Agostino M. V., Danninger M., Day C. T., De Clercq C., Demirors L., Depaepe O., Descamps F., Desiati P., De Vries-Uiterweerd G., Deyoung T., Diaz-Velez J. C., Dreyer J., Dumm J. P., Duvoort M. R., Edwards W. R., Ehrlich R., Eisch J., Ellsworth R. W., Engdegrd O., Euler S., Evenson P. A., Fadiran O., Fazely A. R., Feusels T., Filimonov K., Finley C., Foerster M. M., Fox B. D., Franckowiak A., Franke R., Gaisser T. K., Gallagher J., Ganugapati R., Gerhardt L., Gladstone L., Goldschmidt A., Goodman J. A., Gozzini R., Grant D., Griesel T., Gross A., Grullon S., Gunasingha R. M., Gurtner M., Ha C., Hallgren A., Halzen F., Han K., Hanson K., Hasegawa Y., Heise J., Helbing K., Herquet P., Hickford S., Hill G. C., Hoffman K. D., Hoshina K., Hubert D., Huelsnitz W., Hulss J. -P., Hulth P. O., Hultqvist K., Hussain S., Imlay R. L., Inaba M., Ishihara A., Jacobsen J., Japaridze G. S., Johansson H., Joseph J. M., Kampert K. -H., Kappes A., Karg T., Karle A., Kelley J. L., Kenny P., Kiryluk J., Kislat F., Klein S. R., Klepser S., Knops S., Kohnen G., Kolanoski H., Kopke L., Kowalski M., Kowarik T., Krasberg M., Kuehn K., Kuwabara T., Labare M., Lafebre S., Laihem K., Landsman H., Lauer R., Leich H., Lennarz D., Lucke A., Lundberg J., Lunemann J., Madsen J., Majumdar P., Maruyama R., Mase K., Matis H. S., McParland C. P., Meagher K., Merck M., Meszaros P., Middell E., Milke N., Miyamoto H., Mohr A., Montaruli T., Morse R., Movit S. M., Munich K., Nahnhauer R., Nam J. W., Niessen P., Nygren D. R., Odrowski S., Olivas A., Olivo M., Ono M., Panknin S., Patton S., Perez De Los Heros C., Petrovic J., Piegsa A., Pieloth D., Pohl A. C., Porrata R., Potthoff N., Price P. B., Prikockis M., Przybylski G. T., Rawlins K., Redl P., Resconi E., Rhode W., Ribordy M., Rizzo A., Rodrigues J. P., Roth P., Rothmaier F., Rott C., Roucelle C., Rutledge D., Ryckbosch D., Sander H. -G., Sarkar S., Satalecka K., Schlenstedt S., Schmidt T., Schneider D., Schukraft A., Schulz O., Schunck M., Seckel D., Spiczak G. M., Taboada I., Ter-Antonyan S., Wiebusch C. H., Yoshida S.   +204 more
openaire   +13 more sources

Upgrade of Honda atmospheric neutrino flux calculation with implementing recent hadron interaction measurements

International Conference on Rebooting Computing, 2021
ATMospheric Muon Neutrino Calculation code • Developed by M. Honda [1] • Simulate air shower →calculate atm. ν flux at a given detector pos. • provide full and 3D simulation • High speed calculation by inclusive code • Have been used for atm.
Kazufumi Sato, H. Menjo, Y. Itow, M. Honda   +3 more
semanticscholar   +1 more source

Measurement of CNGS muon neutrino speed with Borexino [PDF]

Physics Letters B, 2012
We have measured the speed of muon neutrinos with the Borexino detector using short-bunch CNGS beams. The final result for the difference in time-of-flight between a =17 GeV muon neutrino and a particle moving at the speed of light in vacuum is t = 0.8 \pm 0.7stat \pm 2.9sys ns, well consistent with zero.
P. Alvarez Sanchez, BARZAGHI, RICCARDO, G. Bellini, J. Benziger, BETTI, BARBARA, BIAGI, LUDOVICO GIORGIO ALDO, D. Bick, G. Bonfini, D. Bravo, M. Buizza Avanzini, B. Caccianiga, L. Cadonati, F. Calaprice, C. Carraro, P. Cavalcante, G. Cerretto, A. Chavarria, D. D’Angelo, S. Davini, DE GAETANI, CARLO IAPIGE, A. Derbin, A. Etenko, H. Esteban, K. Fomenko, D. Franco, C. Galbiati, S. Gazzana, C. Ghiano, M. Giammarchi, M. G ̈oger Ne, A. Goretti, L. Grandi, E. Guardincerri, S. Hardy, Aldo Ianni, Andrea Ianni, A. Kayunov, V. Kobychev, D. Korablev, G. Korga, Y. Koshio, D. Kryn, M. Laubenstein, T. Lewke, E. Litvinovich, B. Loer, P. Lombardi, F. Lombardi, L. Ludhova, I. Machulin, S. Manecki, W. Maneschg, G. Manuzio, Q. Meindl, E. Meroni, L. Miramonti, M. Misiaszek, D. Missiaen, D. Montanari, P. Mosteiro, V. Muratova, L. Oberauer, M. Obolensky, F. Ortica, K. Otis, M. Pallavicini, L. Papp, D. Passoni, PINTO, LIVIO, L. Perasso, S. Perasso, V. Pettiti, C. Plantard, A. Pocar, R. S. Raghavan, G. Ranucci, A. Razeto, A. Re, A. Romani, N. Rossi, A. Sabelnikov, R. Saldanha, C. Salvo, S. Sch ̈onert, J. Serrano, H. Simgen, M. Skorokhvatov, O. Smirnov, A. Sotnikov, P. Spinnato, S. Sukhotin, Y. Suvorov, R. Tartaglia, G. Testera, D. Vignaud, VISCONTI, MARIA GRAZIA, R. B. Vogelaar, F. von Feilitzsch, J. Winter, M. Wojcik, A. Wright, M. Wurm, J. Xu, O. Zaimidoroga, S. Zavatarelli, G. Zuzel   +105 more
openaire   +10 more sources

Updating non-standard neutrinos properties with Planck-CMB data and full-shape analysis of BOSS and eBOSS galaxies [PDF]

Journal of Cosmology and Astroparticle Physics, 2022
Using the latest observational data from Planck-CMB and its combination with the pre-reconstructed full-shape (FS) galaxy power spectrum measurements from the BOSS DR12 sample and eBOSS LRG DR16 sample, we report the observational constraints on the ...
Suresh Kumar, Rafael C. Nunes, P. Yadav
semanticscholar   +1 more source

Can apparent superluminal neutrino speeds be explained as a quantum weak measurement? [PDF]

Journal of Physics A: Mathematical and Theoretical, 2011
10 pages, 1 ...
Berry, M. V., Brunner, N., Popescu, S., Shukla, P.   +3 more
openaire   +5 more sources

Enabling a new detection channel for beyond standard model physics with in-situ measurements of ice luminescence [PDF]

International Conference on Rebooting Computing, 2019
The IceCube neutrino observatory uses $1\,\mathrm{km}^{3}$ of the natural Antarctic ice near the geographic South Pole as optical detection medium. When charged particles, such as particles produced in neutrino interactions, pass through the ice with ...
A. Pollmann
semanticscholar   +1 more source

Measuring speed of gravitational waves by observations of photons and neutrinos from compact binary mergers and supernovae [PDF]

Physical Review D, 2014
Detection of gravitational waves (GW) provides us an opportunity to test general relativity in strong and dynamical regimes of gravity. One of the tests is checking whether GW propagates with the speed of light or not. This test is crucial because the velocity of GW has not ever been directly measured.
Nishizawa, Atsushi, Nakamura, Takashi
openaire   +4 more sources