Results 1 to 10 of about 2,643,304 (148)

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 {\delta}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
arxiv   +14 more sources

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

Astropart.Phys.33:277-286,2010, 2009
We have measured the speed of both pressure waves and shear waves as a function of depth between 80 and 500 m depth in South Pole ice with better than 1% precision. The measurements were made using the South Pole Acoustic Test Setup ({SPATS}), an array of transmitters and sensors deployed in the ice at South Pole Station in order to measure the ...
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
arxiv   +15 more sources

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

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   +7 more sources

Precision measurement of the speed of propagation of neutrinos using the MINOS detectors

Physical Review D, 2015
10 pages, six figures, after refereeing re-submitted to ...
Adamson, P, Anghel, I, Ashby, N, Aurisano, A, Barr, G, Bishai, M, Blake, A, Bock, GJ, Bogert, D, Bumgarner, R, Cao, SV, Castromonte, CM, Childress, S, Coelho, JAB, Corwin, L, Cronin-Hennessy, D, de Jong, JK, Devan, AV, Devenish, NE, Diwan, MV, Escobar, CO, Evans, JJ, Falk, E, Feldman, GJ, Fonville, B, Frohne, MV, Gallagher, HR, Gomes, RA, Goodman, MC, Gouffon, P, Graf, N, Gran, R, Grzelak, K, Habig, A, Hahn, SR, Hartnell, J, Hatcher, R, Hirschauer, J, Holin, A, Huang, J, Hylen, J, Irwin, GM, Isvan, Z, James, C, Jefferts, SR, Jensen, D, Kafka, T, Kasahara, SMS, Koizumi, G, Kordosky, M, Kreymer, A, Lang, K, Ling, J, Litchfield, PJ, Lucas, P, Mann, WA, Marshak, ML, Matsakis, D, Mayer, N, McKinley, A, McGivern, C, Medeiros, MM, Mehdiyev, R, Meier, JR, Messier, MD, Miller, WH, Mishra, SR, Mitchell, S, Sher, SM, Moore, CD, Mualem, L, Musser, J, Naples, D, Nelson, JK, Newman, HB, Nichol, RJ, Nowak, JA, O'Connor, J, Orchanian, M, Pahlka, RB, Paley, J, Parker, TE, Patterson, RB, Pawloski, G, Perch, A, Phan-Budd, S, Plunkett, RK, Poonthottathil, N, Powers, E, Qiu, X, Radovic, A, Rebel, B, Ridl, K, Roemisch, S, Rosenfeld, C, Rubin, HA, Sanchez, MC, Schneps, J, Schreckenberger, A, Schreiner, P, Sharma, R, Sousa, A, Tagg, N, Talaga, RL, Thomas, J, Thomson, MA, Tian, X, Timmons, A, Tognini, SC, Toner, R, Torretta, D, Urheim, J, Vahle, P, Viren, B, Weber, A, Webb, RC, White, C, Whitehead, L, Whitehead, LH, Wojcicki, SG, Wright, J, Zhang, V, Zwaska, R   +122 more
  +11 more sources

Consequences of Neutrino Lorentz Violation For Leptonic Meson Decays [PDF]

Phys. Rev. D 84, 091902(R) (2011), 2011
If the observation by OPERA of apparently superluminal neutrinos is correct, the Lagrangian for second-generation leptons must break Lorentz invariance. We calculate the effects of an energy-independent change in the neutrino speed on another observable, the charged pion decay rate.
Altschul, Brett
arxiv   +5 more sources

Probing WIMP particle physics and astrophysics with direct detection and neutrino telescope data [PDF]

Phys. Rev. D 91, 103533 (2015), 2014
With positive signals from multiple direct detection experiments it will, in principle, be possible to measure the mass and cross sections of weakly-interacting massive particle (WIMP) dark matter. Recent work has shown that, with a polynomial parameterisation of the WIMP speed distribution, it is possible to make an unbiased measurement of the WIMP ...
B. Kavanagh, M. Fornasa, A. Green
arxiv   +3 more sources

Measuring Speed of Gravitational Waves by Observations of Photons and Neutrinos from Compact Binary Mergers and Supernovae [PDF]

Phys. Rev. D 90, 044048 (2014), 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
arxiv   +6 more sources

The influence of Earth rotation in neutrino speed measurements between CERN and the OPERA detector

, 2011
2 ...
Markus Kuhn
openaire   +4 more sources

Planetary influence on the young Sun's evolution: the solar neutrino probe [PDF]

, 2013
Recent observations of solar twin stars with planetary systems like the Sun, have uncovered that these present a peculiar surface chemical composition. This is believed to be related to the formation of earth-like planets.
Lopes, Ilidio, Silk, Joseph
core   +2 more sources