Gouvea, A. D.Pitts, K.Scholberg, K.Zeller, Geralyn P.Alonso, J.Bernstein, A.Bishai, M.Elliott, S.Heeger, K.Hoffman, K.Huber, PatrickKaufman, L. J.Kayser, B.Link, Jonathan M.Lunardini, C.Monreal, B.Morfin, J. G.Robertson, H.Tayloe, R.Tolich, N.Abazajian, Kevork N.Akiri, T.Albright, C. H.Asaadi, J.Babu, K. S.Balantekin, A. B.Barbeau, P. S.Bass, M.Blake, A.Blondel, A.Blucher, E.Bowden, N. S.Brice, S. J.Bross, A.Carls, B.Cavanna, F.Choudhary, B.Coloma, P.Connolly, A.Conrad, J.Convery, M.Cooper, R. L.Cowen, D.Motta, H. D.Young, T. D.Lodovico, F. D.Diwan, M.Djurcic, ZelimirDracos, M.Dodelson, S.Efremenko, Y.Ekelof, T.Feng, J. L.Fleming, B.Formaggio, J. A.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, J. L.Hill, R.Himmel, A.Horton-Smith, Glenn A.Karle, A.Katori, T.Kearns, E.Kettell, S. H.Klein, J.Kim, Y.Kim, Y.-K.Kolomensky, Y. G.Kordosky, M.Kudenko, Y.Kudryavtsev, V. A.Lande, K.Lang, K.Lanza, R.Lau, K.Lee, H.Li, Z.Littlejohn, B. R.Lin, C. J.Liu, D.Liu, H.Long, K.Louis, W.Luk, K. B.Marciano, W. J.Mariani, CamilloMarshak, M.Mauger, C.McDonald, K. T.McFarland, K. S.McKeown, R.Messier, M.Mishra, S. R.Mosel, U.Mumm, P.Nakaya, T.Nelson, J. K.Nygren, D.Orebi Gann, G. D.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, Marjorie HansenSmith, N.Smy, M.Sobel, H.Sorensen, P.Sousa, A.Spitz, JoshuaStrauss, T.Svoboda, R.Tanaka, H. A.Thomas, J.Tian, X.Tschirhart, R.Tully, C.Bibber, K. V.Water, R. G. V. D.Vahle, P.Vogel, P.Walter, C. W.Wark, D.Wascko, M. O.Webber, D.Weerts, H.White, C.White, H.Whitehead, L.Wilson, R. J.Winslow, L.Wongjirad, T.Worcester, E.Yokoyama, M.Yoo, J.Zimmerman, E. D.2016-11-142016-11-142013-10-16http://hdl.handle.net/10919/73433This 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.In Copyrighthep-exhep-phReport