Results 51 to 60 of about 126,591 (192)
Neutrino masses [PDF]
Reports on Progress in Physics, 1995 This is a review for Reports of Progress in Physics. After an introduction we start by explaining the different neutrino masses corresponding to different types of neutrinos, Dirac or Majorana, in section 2. In section 3 we discuss the main elementary particle models for neutrino masses and their distinctive phenomenological consequences.Gelmini, Graciela, Roulet, Estebanopenaire +2 more sourcesAtmospheric and Astrophysical Neutrinos above 1 TeV Interacting in
IceCube [PDF]
, 2015 The IceCube Neutrino Observatory was designed primarily to search for
high-energy (TeV--PeV) neutrinos produced in distant astrophysical objects. A
search for $\gtrsim 100$~TeV neutrinos interacting inside the instrumented
volume has recently provided ...Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Altmann, D., Anderson, T., Arguelles, C., Arlen, T. C., Auffenberg, J., Bai, X., Barwick, S. W., Baum, V., Bay, R., Beatty, J. J., Becker Tjus, J., Becker, K.-H., BenZvi, S., Berghaus, P., Berley, D., Bernardini, E., Bernhard, A., Besson, D. Z., Binder, G., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohm, C., Bos, F., Bose, D., Botner, O., Brayeur, L., Bretz, H.-P., Brown, A. M., Buzinsky, N., Böser, S., Casey, J., Casier, M., Cheung, E., Chirkin, D., Christov, A., Christy, B., Clark, K., Classen, L., Clevermann, F., Coenders, S., Cowen, D. F., Cruz Silva, A. H., Danninger, M., Daughhetee, J., Davis, J. C., Day, M., de André, J. P. A. M., De Clercq, C., De Ridder, S., de Vries, K. D., de With, M., Desiati, P., DeYoung, T., Dunkman, M., Díaz-Vélez, J. C., Eagan, R., Eberhardt, B., Eichmann, B., Eisch, J., Euler, S., Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feintzeig, J., Felde, J., Feusels, T., Filimonov, K., Finley, C., Fischer-Wasels, T., Flis, S., Franckowiak, A., Frantzen, K., Fuchs, T., Gaior, R., Gaisser, T. K., Gallagher, J., Gerhardt, L., Gier, D., Gladstone, L., Glüsenkamp, T., Goldschmidt, A., Golup, G., Gonzalez, J. G., Goodman, J. A., Grant, D., Gretskov, P., Groh, J. C., Groß, A., Góra, D., Ha, C., Haack, C., Haj Ismail, A., Hallen, P., Hallgren, A., Halzen, F., Hanson, K., Hebecker, D., Heereman, D., Heinen, D., Helbing, K., Hellauer, R., Hellwig, D., Hickford, S., Hill, G. C., Hoffman, K. D., Hoffmann, R., Homeier, A., Hoshina, K., Huang, F., Huelsnitz, W., Hulth, P. O., Hultqvist, K., Hussain, S., IceCube Collaboration, Ishihara, A., Jacobi, E., Jacobsen, J., Jagielski, K., Japaridze, G. S., Jero, K., Jlelati, O., Jurkovic, M., Kaminsky, B., Kappes, A., Karg, T., Karle, A., Kauer, M., Keivani, A., Kelley, J. L., Kheirandish, A., Kiryluk, J., Klein, S. R., Kläs, J., Kohnen, G., Kolanoski, H., Koob, A., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Kriesten, A., Krings, K., Kroll, G., Kroll, M., Kunnen, J., Kurahashi, N., Kuwabara, T., Köhne, J.-H., Köpke, L., Labare, M., Larsen, D. T., Larson, M. J., Lesiak-Bzdak, M., Leuermann, M., Leute, J., Lünemann, J., Madsen, J., Maggi, G., Maruyama, R., Mase, K., Matis, H. S., Maunu, R., McNally, F., Meagher, K., Medici, M., Meli, A., Meures, T., Miarecki, S., Middell, E., Middlemas, E., Milke, N., Miller, J., Mohrmann, L., Montaruli, T., Morse, R., Nahnhauer, R., Naumann, U., Niederhausen, H., Nowicki, S. C., Nygren, D. R., Obertacke, A., Odrowski, S., Olivas, A., Omairat, A., O’Murchadha, A., Palczewski, T., Paul, L., Penek, Ö., Pepper, J. A., Pfendner, C., Pieloth, D., Pinat, E., Posselt, J., Price, P. B., Przybylski, G. T., Pérez de los Heros, C., Pütz, J., Quinnan, M., Rameez, M., Rawlins, K., Redl, P., Rees, I., Reimann, R., Relich, M., Resconi, E., Rhode, W., Richman, M., Riedel, B., Robertson, S., Rodrigues, J. P., Rongen, M., Rott, C., Ruhe, T., Ruzybayev, B., Ryckbosch, D., Rädel, L., Saba, S. M., Sander, H.-G., Sandroos, J., Santander, M., Sarkar, S., Schatto, K., Scheriau, F., Schmidt, T., Schmitz, M., Schoenen, S., Schukraft, A., Schulte, L., Schulz, O., Schöneberg, S., Schönwald, A., Seckel, D., Sestayo, Y., Seunarine, S., Shanidze, R., Smith, M. W. E., Soldin, D., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stanisha, N. A., Stasik, A., Stezelberger, T., Stokstad, R. G., Strahler, E. A., Strotjohann, N. L., Ström, R., Stößl, A., Sullivan, G. W., Taavola, H., Taboada, I., Tamburro, A., Tepe, A., Ter-Antonyan, S., Terliuk, A., Tešić, G., Tilav, S., Toale, P. A., Tobin, M. N., Tosi, D., Tselengidou, M., Unger, E., Usner, M., Vallecorsa, S., van Eijndhoven, N., van Santen, J., Vandenbroucke, J., Vehring, M., Voge, M., Vraeghe, M., Walck, C., Wallraff, M., Weaver, Ch., Wellons, M., Wendt, C., Westerhoff, S., Whelan, B. J., Whitehorn, N., Wichary, C., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Xu, D. L., Xu, X. W., Yanez, J. P., Yodh, G., Yoshida, S., Zarzhitsky, P., Ziemann, J., Zierke, S., Zoll, M. +305 morecore +3 more sourcesClockwork neutrinos [PDF]
Journal of High Energy Physics, 2019 Abstract Clockwork (CW) mechanism can explain the smallness of neutrino masses without introducing unnaturally small input parameters. In this paper we study the simplest CW neutrino model, the “uniform” clockwork, as well as a broader class of “generalized” clockwork models.Hong, Sungwoo, Kurup, Gowri, Perelstein, Maxim +2 moreopenaire +3 more sourcesTau Neutrinos Favored over Sterile Neutrinos in Atmospheric Muon
Neutrino Oscillations [PDF]
, 2000 The previously published atmospheric neutrino data did not distinguish
whether muon neutrinos were oscillating into tau neutrinos or sterile
neutrinos, as both hypotheses fit the data.A. de Gouvea, A. Habig, A. Kibayashi, A. L. Stachyra, A. Okada, A. Sakai, A. Suzuki, A. T. Suzuki, B. Adeva, B. K. Kim, B. Viren, C. Athanassopoulos, C. K. Jung, C. Mauger, C. McGrew, C. Mitsuda, C. Saji, C. W. Walter, C. Yanagisawa, D. Casper, D. Decamp, D. Kielczewska, D. L. Anderson, D. Takemori, E. Akhmedov, E. Blaufuss, E. Kearns, E. Sharkey, G. Alexander, G. Guillian, G. W. Sullivan, H. Fujiyasu, H. Ishino, H. Okazawa, H. Takeuchi, H. W. Sobel, J. A. Goodman, J. G. Learned, J. Hill, J. Kameda, J. L. Stone, J. N. Bahcall, J. Shirai, K. Inoue, K. Ishihara, K. K. Young, K. Kaneyuki, K. Kobayashi, K. Martens, K. Miyano, K. Nakamura, K. Nishijima, K. Nishikawa, K. Nitta, K. Okumura, K. S. Ganezer, K. Scholberg, L. R. Price, L. R. Sulak, L. Wolfenstein, M. D. Messier, M. Earl, M. Etoh, M. Goldhaber, M. Honda, M. Ishitsuka, M. Kirisawa, M. Kohama, M. Koike, M. Koshiba, M. L. Chen, M. Malek, M. Miura, M. Morii, M. Nakahata, M. R. Vagins, M. Sakuda, M. Shiozawa, M. Smy, M. Takahashi, M. Takahata, M. Takita, M. Yoshida, N. Sakurai, O. Sasaki, P. Abreu, P. Lipari, P. Lipari, Q. Y. Liu, Q. Y. Liu, R. J. Wilkes, R. Sanford, R. Svoboda, R. W. Ellsworth, S. B. Kim, S. C. Boyd, S. Fukuda, S. Inaba, S. Matsuno, S. Mine, S. Moriyama, S. Nakayama, S. P. Mikheyev, S. P. Mikheyev, S. P. Mikheyev, S. Tasaka, S. Yamada, T. Barszczak, T. Hasegawa, T. Inagaki, T. Ishii, T. Ishizuka, T. J. Haines, T. Kajita, T. Kobayashi, T. Maruyama, T. Toshito, U. Golebiewska, V. Agrawal, V. Barger, W. E. Keig, W. Gajewski, W. R. Kropp, Y. Fukuda, Y. Fukuda, Y. Fukuda, Y. Fukuda, Y. Fukuda, Y. Fukuda, Y. Gando, Y. Hatakeyama, Y. Hayato, Y. Ichikawa, Y. Itow, Y. Koshio, Y. Nagashima, Y. Obayashi, Y. Oyama, Y. Suzuki, Y. Takeuchi, Y. Totsuka, Y. Watanabe +141 morecore +2 more sourcesNEUTRINO CLOUDS
International Journal of Modern Physics A, 1998 We consider the possibility that neutrinos (but no other light fermions) are coupled very weakly to an extremely light scalar boson. We first analyze the simple problem of one generation of neutrino and show that, for ranges of parameters that are allowed by existing data, such a system can have serious consequences for the evolution of stars and ...Stephenson Jr., G. J., Goldman, T., McKellar, B. H. J. +2 moreopenaire +2 more sourcesMirror model for sterile neutrinos
, 2003 Sterile neutrinos are studied as subdominant contribution to solar neutrino
physics. The mirror-matter neutrinos are considered as sterile neutrinos. We
use the symmetric mirror model with gravitational communication between mirror
and visible sectors ...Abdurashitov, Aglietta, Aguilar, Ahmad, Ahmad, Akhmedov, Akmal, Ambrosio, Apollonio, Aulakh, Bahcall, Bahcall, Bahcall, Bajc, Barbieri, Barger, Benakli, Berezhiani, Berezhiani, Berezhiani, Berezhiani, Berezinsky, Berezinsky, Berezinsky, Berezinsky, Berezinsky, Berezinsky, Blinnikov, Burrows, Carlson, Chacko, Chiu, Chun, Chun, Cleaver, Creminelli, Crocker, Dazeley, de Holanda, Dighe, Dolgov, Dutta, Elgaroy, Enqvist, Fargion, Fodor, Fodor, Fogli, Foot, Foot, Foot, Foot, Foot, Foot, Foot, Francesco Vissani, Fryer, Fukuda, Gelmini, Glashow, Gonzalez-Garcia, Gursey, Hall, Hewett, Hirsch, Holdom, Kachelriess, Kallosh, Keil, Khlopov, Kirilova, Kirilova, Kobzarev, Kolb, Krastev, Landau, Langacker, Lee, Liebendorfer, Loredo, Ma, Maltoni, Maltoni, Mikheyev, Minakata, Mohan Narayan, Mohapatra, Okun, Päs, Raghavan, Raghavan, Salam, Shi, Silagadze, Silagadze, Strumia, Strumia, Takahashi, Veniamin Berezinsky, Vissani, Weiler, Weinberg, Wolfenstein +102 morecore +1 more sourceExtremely High Energy Neutrinos and their Detection [PDF]
, 1996 We discuss in some detail the production of extremely high energy (EHE)
neutrinos with energies above 10^18 eV. The most certain process for producing
such neutrinos results from photopion production by EHE cosmic rays in the
cosmic background photon ...Dai, Hongyue, Jui, Charles C. H., Sommers, Paul, Yoshida, Shigeru +3 morecore +4 more sources
