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arxiv 1310.4340 v1 pith:EFVVF3A4 submitted 2013-10-16 hep-ex hep-ph

Neutrinos

A. de Gouvea , K. Pitts , K. Scholberg , G.P. Zeller , J. Alonso , A. Bernstein , M. Bishai , S. Elliott
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K. Heeger K. Hoffman P. Huber L.J. Kaufman B. Kayser J. Link C. Lunardini B. Monreal J.G. Morfin H. Robertson R. Tayloe N. Tolich K. Abazajian T. Akiri C. Albright J. Asaadi K.S Babu A.B. Balantekin P. Barbeau M. Bass A. Blake A. Blondel E. Blucher N. Bowden S.J. Brice A. Bross B. Carls F. Cavanna B. Choudhary P. Coloma A. Connolly J. Conrad M. Convery R.L. Cooper D. Cowen H. da Motta T. de Young F. Di Lodovico M. Diwan Z. Djurcic M. Dracos S. Dodelson Y. Efremenko T. Ekelof J.L. Feng B. Fleming J. Formaggio A. Friedland G. Fuller H. Gallagher S. Geer M. Gilchriese M. Goodman D. Grant G. Gratta C. Hall F. Halzen D. Harris M. Heffner R. Henning J.L. Hewett R. Hill A. Himmel G. Horton-Smith A. Karle T. Katori E. Kearns S. Kettell J. Klein Y. Kim Y.K. Kim Yu. Kolomensky M. Kordosky Yu. Kudenko V.A. Kudryavtsev K. Lande K. Lang R. Lanza K. Lau H. Lee Z. Li B.R. Littlejohn C.J. Lin D. Liu H. Liu K. Long W. Louis K.B. Luk W. Marciano C. Mariani M. Marshak C. Mauger K.T. McDonald K. McFarland R. McKeown M. Messier S.R. Mishra U. Mosel P. Mumm T. Nakaya J.K. Nelson D. Nygren G.D. Orebi Gann J. Osta O. Palamara J. Paley V. Papadimitriou S. Parke Z. Parsa R. Patterson A. Piepke R. Plunkett A. Poon X. Qian J. Raaf R. Rameika M. Ramsey-Musolf B. Rebel R. Roser J. Rosner C. Rott G. Rybka H. Sahoo S. Sangiorgio D. Schmitz R. Shrock M. Shaevitz N. Smith M. Smy H. Sobel P. Sorensen A. Sousa J. Spitz T. Strauss R. Svoboda H.A. Tanaka J. Thomas X. Tian R. Tschirhart C. Tully K. Van Bibber R.G. Van de Water P. Vahle P. Vogel C.W. Walter D. Wark M. Wascko D. Webber H. Weerts C. White H. White L. Whitehead R.J. Wilson L. Winslow T Wongjirad E. Worcester M. Yokoyama J. Yoo E.D. Zimmerman
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keywords neutrinosneutrinophysicsaddressingastrophysicschargecurrentdocument
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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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