Materias dentro de su búsqueda.
Materias dentro de su búsqueda.
-
2801“…In this work we will describe the analysis for secluded dark matter coming from the Sun with ANTARES in three different cases: a) detection of di-muons that result of the mediator decay, or neutrino detection from: b) mediator that decays into di-muon and, in turn, into neutrinos, and c) mediator that directly decays into neutrinos. …”
Enlace del recurso
-
2802por Bassi, L, Cennini, P, Cittolin, Sergio, Di Ciaccio, Anna, Gonidec, A, Mazzone, L, Muñoz, R, Müller, T, Muratori, G, Rubbia, Carlo, Schinzel, D, Schmidt, W, Buckley, E, Ciaffoni, O, Ciocio, A, Di Pirro, G, Pallotta, M, Picchi, P, Trasatti, L, Piano Mortari, G, Baldo-Ceolin, Massimilla, Bettini, A, Braggiotti, A, Centro, Sandro, Casoli, P, Dainese, B, Dal Corso, F, Gasparini, F, Huzita, H, Pietropaolo, F, Rossi, P, Suzuki, S, Cheng, M, Cline, D, Park, J, Zhou, MEnlace del recurso
Publicado 1989
-
2803
-
2804por Edgecock, T R“…EUROnu is a European Commission Framework Programme 7 project undertaking a Design Study of possible future neutrino oscillation facilities for Europe. The three main candidates being studied are a CERN to Frjus Superbeam, a Neutrino Factory and a Beta Beam. …”
Publicado 2010
Enlace del recurso
Enlace del recurso
-
2805
-
2806“…The neutrino factory is one of the designs proposed for a future intense neutrino beam facility. …”
Enlace del recurso
Enlace del recurso
-
2807por Pascoli, S“…The recent evidence of neutrino oscillations has opened a new perspective on neutrino physics, implying that neutrinos are massive and mix. …”
Publicado 2010
Enlace del recurso
Enlace del recurso
-
2808por Audren, Benjamin, Bellini, Emilio, Cuesta, Antonio J, Gontcho, Satya Gontcho A, Lesgourgues, Julien, Niro, Viviana, Pellejero-Ibanez, Marcos, Pérez-Ràfols, Ignasi, Poulin, Vivian, Tram, Thomas, Tramonte, Denis, Verde, Licia“…We conclude that it is possible to make a robust statement about the detection of the cosmic neutrino background by CMB experiments.…”
Publicado 2014
Enlace del recurso
Enlace del recurso
-
2809
-
2810“…We identify the inos with sterile right-handed neutrinos. The possible mass range of up to a few tens of keV, obtained independently from the galactic structure and dark matter astroparticle physics, points towards an important role of the right-handed neutrinos in the cosmic structure.…”
Enlace del recurso
Enlace del recurso
-
2811por Allaby, James V, Amaldi, Ugo, Barbiellini, Guido, Baubillier, M, Bergsma, F, Capone, A, Flegel, Wilfried, Lanceri, L, Metcalf, M, Nieuwenhuis, C, Pain, R, Panman, J, Winter, Klaus, Abt, I, Blobel, Volker, Büngener, A, Büsser, F W, Gall, P D, Hebbeker, T, Niebergall, F, Stähelin, P, Gorbunov, P, Grigoriev, E A, Khovanskii, V D, Rosanov, A, Borgia, B, Diemoz, M, Dionisi, C, Dore, U, Ferroni, F, Longo, E, Loverre, P F, Luminari, L, Monacelli, P, Morganti, S, De Notaristefani, F, Santacesaria, R, Santoni, CEnlace del recurso
Publicado 1989
Enlace del recurso
-
2812por Palanque-Delabrouille, Nathalie, Yèche, Christophe, Baur, Julien, Magneville, Christophe, Rossi, Graziano, Lesgourgues, Julien, Borde, Arnaud, Burtin, Etienne, LeGoff, Jean-Marc, Rich, James, Viel, Matteo, Weinberg, David“…Combining BOSS Ly$\alpha$ with Planck CMB constrains the sum of neutrino masses to $\sum m_\nu < 0.12$ eV (95\% C.L.) including all identified systematic uncertainties, tighter than our previous limit (0.15 eV) and more robust. …”
Publicado 2015
Enlace del recurso
Enlace del recurso
-
2813
-
2814por Eichten, T, Faissner, Helmut, Hasert, F J, Kabe, S, Krenz, W, Von Krogh, J, Morfín, J G, Schultze, K, Bertrand-Coremans, G H, Sacton, J, Van Doninck, W K, Vilain, P, Cundy, Donald C, Haidt, Dieter, Jaffré, M, Natali, S, Musset, P, Pattison, John Bryan M, Perkins, Donald Hill, Pullia, Antonio, Rousset, A, Venus, W A, Wachsmuth, H W, Brisson, V, Degrange, B, Haguenauer, Maurice, Kluberg, L, Nguyen-Khac, U, Petiau, P, Belotti, E, Bonetti, S, Cavalli, D, Conta, C, Fiorini, Ettore, Franzinetti, Carlo, Rollier, M, Aubert, Bernard, Chounet, L M, Heusse, P, Jauneau, L, Lutz, A M, Pascaud, C, Vialle, J P, Bullock, F W, Derrick, Malcolm, Esten, M J, Jones, T W, McKenzie, J, Michette, A G, Myatt, Gerald, Scott, W GEnlace del recurso
Publicado 1973
Enlace del recurso
-
2815por Adrián-Martínez, S., Albert, A., André, M., Anton, G., Ardid, M., Aubert, J.-J., Baret, B., Barrios-Martí, J., Basa, S., Bertin, V., Biagi, S., Bogazzi, C., Bormuth, R., Bou-Cabo, M., Bouwhuis, M.C., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Chiarusi, T., Circella, M., Coniglione, R., Costantini, H., Coyle, P., Creusot, A., Dekeyser, I., Deschamps, A., De Bonis, G., Distefano, C., Donzaud, C., Dornic, D., Drouhin, D., Dumas, A., Eberl, T., Elsässer, D., Enzenhöfer, A., Fehn, K., Felis, I., Fermani, P., Flaminio, V., Folger, F., Fusco, L.A., Galatà, S., Gay, P., Geißelsöder, S., Geyer, K., Giordano, V., Gleixner, A., Gracia-Ruiz, R., Gómez-González, J.P., Graf, K., van Haren, H., Heijboer, A.J., Hello, Y., Hernández-Rey, J.J., Herrero, A., Hößl, J., Hofestädt, J., Hugon, C., James, C.W., de Jong, M., Kadler, M., Kalekin, O., Katz, U., Kießling, D., Kooijman, P., Kouchner, A., Kreykenbohm, I., Kulikovskiy, V., Lahmann, R., Lambard, G., Lattuada, D., Lefèvre, D., Leonora, E., Loucatos, S., Mangano, S., Marcelin, M., Margiotta, A., Marinelli, A., Martínez-Mora, J.A., Martini, S., Mathieu, A., Michael, T., Migliozzi, P., Moussa, A., Mueller, C., Neff, M., Nezri, E., Păvălaş, G.E., Pellegrino, C., Perrina, C., Piattelli, P., Popa, V., Pradier, T., Racca, C., Riccobene, G., Richter, R., Roensch, K., Rostovtsev, A., Saldaña, M., Samtleben, D.F.E., Sánchez-Losa, A., Sanguineti, M., Sapienza, P., Schmid, J., Schnabel, J., Schulte, S., Schüssler, F., Seitz, T., Sieger, C., Spurio, M., Steijger, J.J.M., Stolarczyk, Th., Taiuti, M., Tamburini, C., Trovato, A., Tselengidou, M., Tönnis, C., Turpin, D., Vallage, B., Vallée, C., Van Elewyck, V., Visser, E., Vivolo, D., Wagner, S., Wilms, J., Zornoza, J.D., Zúñiga, J.“…It searches for astrophysical neutrinos collecting the Cherenkov light induced by the charged particles, mainly muons, produced in neutrino interactions around the detector. …”
Publicado 2015
Enlace del recurso
Enlace del recurso
-
2816
-
2817por Alunni Solestizi, Luisa“…No excess has been observed in the di-muon and di-jetchannel; while the di-tau and di-jet signature has not yet been explored forthe heavy neutrinos specific search, but only for the leptoquarks, with a b ort jet tagging.A benchmark process with a same flavour di-lepton plus di-jet signature, inthe frame of composite neutrinos and contact interactions, is taken into con-sideration to clarify the nature of the excess and to extend the mass limit forthe heavy neutrinos, exploiting the run 2 of CMS.…”
Publicado 2015
Enlace del recurso
-
2818por Mitsou, Vasiliki A.“…In this paper, we discuss RPV scenarios where neutrino masses are naturally generated, namely RPV through bilinear terms (bRPV) and the $\mu$-from-$\nu$ supersymmetric standard model ($\mu\nu$SSM). …”
Publicado 2015
Enlace del recurso
Enlace del recurso
-
2819por Stanco, Luca“…The OPERA experiment at the CNGS beam has observed muon to tau neutrino oscillations in the atmospheric sector. Based on this result new limits on the mixing parameters of a massive sterile neutrino may be set. …”
Publicado 2015
Enlace del recurso
Enlace del recurso
-
2820