Results 71 to 80 of about 7,170 (161)
Precision measurements on δ CP in MOMENT
Journal of High Energy Physics, 2019 As it is very promising to expect a discovery of CP violation in the leptonic sector, the precision measurement of the Dirac CP phase δ CP is going to be one of the key interests in the future neutrino oscillation experiments.Jian Tang, Sampsa Vihonen, Tse-Chun Wangdoaj +1 more sourceSupersymmetric Dark Matter Detection at Post-LEP Benchmark Points [PDF]
, 2001 We review the prospects for discovering supersymmetric dark matter in a
recently proposed set of post-LEP supersymmetric benchmark scenarios. We
consider direct detection through spin-independent nuclear scattering, as well
as indirect detection through ...Ellis, John, Feng, Jonathan L., Ferstl, Andrew, Matchev, Konstantin T., Olive, Keith A. +4 morecore +1 more sourceThe Cosmology Large Angular Scale Surveyor
, 2016 The Cosmology Large Angular Scale Surveyor (CLASS) is a four telescope array
designed to characterize relic primordial gravitational waves from inflation
and the optical depth to reionization through a measurement of the polarized
cosmic microwave ...Ali, Aamir, Appel, John W., Bennett, Charles L., Boone, Fletcher, Brewer, Michael, Chan, Manwei, Chuss, David T., Colazo, Felipe, Dahal, Sumit, Denis, Kevin, Dünner, Rolando, Eimer, Joseph, Essinger-Hileman, Thomas, Fluxa, Pedro, Halpern, Mark, Harrington, Kathleen, Hilton, Gene, Hinshaw, Gary F., Hubmayr, Johannes, Iuliano, Jeffery, Karakla, John, Marriage, Tobias, McMahon, Jeff, Miller, Nathan T., Moseley, Samuel H., Palma, Gonzalo, Parker, Lucas, Petroff, Matthew, Pradenas, Bastián, Rostem, Karwan, Sagliocca, Marco, Valle, Deniz, Watts, Duncan, Wollack, Edward, Xu, Zhilei, Zeng, Lingzhen +35 morecore +1 more sourceHigh-energy astroparticle physics
, 2009 In these three lectures I discuss the present status of high-energy
astroparticle physics including Ultra-High-Energy Cosmic Rays (UHECR),
high-energy gamma rays, and neutrinos. The first lecture is devoted to
ultra-high-energy cosmic rays. After a brief Semikoz, D.core +2 more sourcesTritium beta decay with additional emission of new light bosons
Journal of High Energy Physics, 2019 We consider tritium beta decay with additional emission of light pseudoscalar or vector bosons coupling to electrons or neutrinos. The electron energy spectrum for all cases is evaluated and shown to be well estimated by approximated analytical ...Giorgio Arcadi, Julian Heeck, Florian Heizmann, Susanne Mertens, Farinaldo S. Queiroz, Werner Rodejohann, Martin Slezák, Kathrin Valerius +7 moredoaj +1 more sourceA binned likelihood for stochastic models
Journal of High Energy Physics, 2019 Metrics of model goodness-of-fit, model comparison, and model parameter estimation are the main categories of statistical problems in science. Bayesian and frequentist methods that address these questions often rely on a likelihood function, which is the C. A. Argüelles, A. Schneider, T. Yuandoaj +1 more sourceHigh energy cosmic-rays: puzzles, models, and giga-ton neutrino
telescopes
, 2003 The existence of cosmic rays of energies exceeding 10^20 eV is one of the
mysteries of high energy astrophysics. The spectrum and the high energy to
which it extends rule out almost all suggested source models.A Achterberg, A M Hillas, Arons, D Band, D Casper, D J Bird, D J Bird, E Boldt, E Waxman, E Waxman, E Waxman, E Waxman, E. Waxman, F Halzen, G L Fogli, G T Zatsepin, J Bednarz, J Bloom, J Hjorth, J N Bahcall, J N Bahcall, J N Bahcall, K Greisen, K Z Stanek, M Drees, M Milgrom, M Nagano, M Schmidt, M Vietri, N Hayashida, N N Efimov, P Bhattacharjee, P Mészáros, R Blandford, T Abu-Zayyad, T J Galama, T Piran, W I Axford, Y Fukuda +38 morecore +1 more sourceMeasurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCA
Journal of High Energy PhysicsKM3NeT/ORCA is a water Cherenkov neutrino detector under construction and anchored at the bottom of the Mediterranean Sea. The detector is designed to study oscillations of atmospheric neutrinos and determine the neutrino mass ordering.The KM3NeT collaboration, S. Aiello, A. Albert, A. R. Alhebsi, M. Alshamsi, S. Alves Garre, A. Ambrosone, F. Ameli, M. Andre, L. Aphecetche, M. Ardid, S. Ardid, H. Atmani, J. Aublin, F. Badaracco, L. Bailly-Salins, Z. Bardačová, B. Baret, A. Bariego-Quintana, Y. Becherini, M. Bendahman, F. Benfenati, M. Benhassi, M. Bennani, D. M. Benoit, E. Berbee, V. Bertin, S. Biagi, M. Boettcher, D. Bonanno, A. B. Bouasla, J. Boumaaza, M. Bouta, M. Bouwhuis, C. Bozza, R. M. Bozza, H. Brânzaş, F. Bretaudeau, M. Breuhaus, R. Bruijn, J. Brunner, R. Bruno, E. Buis, R. Buompane, J. Busto, B. Caiffi, D. Calvo, A. Capone, F. Carenini, V. Carretero, T. Cartraud, P. Castaldi, V. Cecchini, S. Celli, L. Cerisy, M. Chabab, A. Chen, S. Cherubini, T. Chiarusi, M. Circella, R. Cocimano, J. A. B. Coelho, A. Coleiro, A. Condorelli, R. Coniglione, P. Coyle, A. Creusot, G. Cuttone, R. Dallier, A. De Benedittis, B. De Martino, G. De Wasseige, V. Decoene, I. Del Rosso, L. S. Di Mauro, I. Di Palma, A. F. Díaz, D. Diego-Tortosa, C. Distefano, A. Domi, C. Donzaud, D. Dornic, E. Drakopoulou, D. Drouhin, J.-G. Ducoin, R. Dvornický, T. Eberl, E. Eckerová, A. Eddymaoui, T. van Eeden, M. Eff, D. van Eijk, I. El Bojaddaini, S. El Hedri, V. Ellajosyula, A. Enzenhöfer, G. Ferrara, M. D. Filipović, F. Filippini, D. Franciotti, L. A. Fusco, S. Gagliardini, T. Gal, J. García Méndez, A. Garcia Soto, C. Gatius Oliver, N. Geißelbrecht, E. Genton, H. Ghaddari, L. Gialanella, B. K. Gibson, E. Giorgio, I. Goos, P. Goswami, S. R. Gozzini, R. Gracia, C. Guidi, B. Guillon, M. Gutiérrez, C. Haack, H. van Haren, A. Heijboer, L. Hennig, J. J. Hernández-Rey, W. Idrissi Ibnsalih, G. Illuminati, D. Joly, M. de Jong, P. de Jong, B. J. Jung, G. Kistauri, C. Kopper, A. Kouchner, Y. Y. Kovalev, V. Kueviakoe, V. Kulikovskiy, R. Kvatadze, M. Labalme, R. Lahmann, M. Lamoureux, G. Larosa, C. Lastoria, A. Lazo, S. Le Stum, G. Lehaut, V. Lemaître, E. Leonora, N. Lessing, G. Levi, M. Lindsey Clark, F. Longhitano, F. Magnani, J. Majumdar, L. Malerba, F. Mamedov, J. Mańczak, A. Manfreda, M. Marconi, A. Margiotta, A. Marinelli, C. Markou, L. Martin, M. Mastrodicasa, S. Mastroianni, J. Mauro, G. Miele, P. Migliozzi, E. Migneco, M. L. Mitsou, C. M. Mollo, L. Morales-Gallegos, A. Moussa, I. Mozun Mateo, R. Muller, M. R. Musone, M. Musumeci, S. Navas, A. Nayerhoda, C. A. Nicolau, B. Nkosi, B. Ó Fearraigh, V. Oliviero, A. Orlando, E. Oukacha, D. Paesani, J. Palacios González, G. Papalashvili, V. Parisi, E. J. Pastor Gomez, A. M. Păun, G. E. Păvălaş, S. Peña Martínez, M. Perrin-Terrin, V. Pestel, R. Pestes, P. Piattelli, A. Plavin, C. Poirè, V. Popa, T. Pradier, J. Prado, S. Pulvirenti, C. A. Quiroz-Rangel, N. Randazzo, S. Razzaque, I. C. Rea, D. Real, G. Riccobene, J. Robinson, A. Romanov, E. Ros, A. Šaina, F. Salesa Greus, D. F. E. Samtleben, A. Sánchez Losa, S. Sanfilippo, M. Sanguineti, D. Santonocito, P. Sapienza, J. Schnabel, J. Schumann, H. M. Schutte, J. Seneca, I. Sgura, R. Shanidze, A. Sharma, Y. Shitov, F. Šimkovic, A. Simonelli, A. Sinopoulou, B. Spisso, M. Spurio, D. Stavropoulos, I. Štekl, S. M. Stellacci, M. Taiuti, Y. Tayalati, H. Thiersen, S. Thoudam, I. Tosta e Melo, B. Trocmé, V. Tsourapis, A. Tudorache, E. Tzamariudaki, A. Ukleja, A. Vacheret, V. Valsecchi, V. Van Elewyck, G. Vannoye, G. Vasileiadis, F. Vazquez de Sola, A. Veutro, S. Viola, D. Vivolo, A. van Vliet, E. de Wolf, I. Lhenry-Yvon, S. Zavatarelli, A. Zegarelli, D. Zito, J. D. Zornoza, J. Zúñiga, N. Zywucka +262 moredoaj +1 more sourceHigh-Energy Neutrinos from Cosmic Rays
, 2002 We introduce neutrino astronomy from the observational fact that Nature
accelerates protons and photons to energies in excess of 10^{20} and 10^{13}
eV, respectively. Although the discovery of cosmic rays dates back close to a
century, we do not know how Halzen, F.core +2 more sources
