Publications [#362624] of Phillip S. Barbeau
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Gouvea, AD; Pitts, K; Scholberg, K; Zeller, GP; Alonso, J; Bernstein, A; Bishai, M; Elliott, S; Heeger, K; Hoffman, K; Huber, P; Kaufman, LJ; Kayser, B; Link, J; Lunardini, C; Monreal, B; Morfin, JG; Robertson, H; Tayloe, R; Tolich, N; Abazajian, K; Akiri, T; Albright, C; Asaadi, J; Babu, KS; Balantekin, AB; Barbeau, P; Bass, M; Blake, A; Blondel, A; Blucher, E; Bowden, N; Brice, SJ; Bross, A; Carls, B; Cavanna, F; Choudhary, B; Coloma, P; Connolly, A; Conrad, J; Convery, M; Cooper, RL; Cowen, D; Motta, HD; Young, TD; Lodovico, FD; Diwan, M; Djurcic, Z; Dracos, M; Dodelson, S; Efremenko, Y; Ekelof, T; Feng, JL; Fleming, B; Formaggio, J; Friedland, A; Fuller, G; Gallagher, H; Geer, S; Gilchriese, M; Goodman, M; Grant, D; Gratta, G; Hall, C; Halzen, F; Harris, D; Heffner, M; Henning, R; Hewett, JL; Hill, R; Himmel, A; Horton-Smith, G; Karle, A; Katori, T; Kearns, E; Kettell, S; Klein, J; Kim, Y; Kim, YK; Kolomensky, Y; Kordosky, M; Kudenko, Y; Kudryavtsev, VA; Lande, K; Lang, K; Lanza, R; Lau, K; Lee, H; Li, Z; Littlejohn, BR; Lin, CJ; Liu, D; Liu, H; Long, K; Louis, W; Luk, KB; Marciano, W; Mariani, C; Marshak, M; Mauger, C; McDonald, KT; McFarland, K; McKeown, R; Messier, M; Mishra, SR; Mosel, U; Mumm, P; Nakaya, T; Nelson, JK; Nygren, D; Gann, GDO; Osta, J; Palamara, O; Paley, J; Papadimitriou, V; Parke, S; Parsa, Z; Patterson, R; Piepke, A; Plunkett, R; Poon, A; Qian, X; Raaf, J; Rameika, R; Ramsey-Musolf, M; Rebel, B; Roser, R; Rosner, J; Rott, C; Rybka, G; Sahoo, H; Sangiorgio, S; Schmitz, D; Shrock, R; Shaevitz, M; Smith, N; Smy, M; Sobel, H; Sorensen, P; Sousa, A; Spitz, J; Strauss, T; Svoboda, R; Tanaka, HA; Thomas, J; Tian, X; Tschirhart, R; Tully, C; Bibber, KV; Water, RGVD; Vahle, P; Vogel, P; Walter, CW; Wark, D; Wascko, M; Webber, D; Weerts, H; White, C; White, H; Whitehead, L; Wilson, RJ; Winslow, L; Wongjirad, T; Worcester, E; Yokoyama, M; Yoo, J; Zimmerman, ED, Neutrinos
(October, 2013) .
Abstract:
This document represents the response of the Intensity Frontier Neutrino
Working Group to the Snowmass charge. We summarize the current status of
neutrino physics and identify many exciting future opportunities for studying
the properties of neutrinos and for addressing important physics and
astrophysics questions with neutrinos.
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