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Materias dentro de su búsqueda.
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2001
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2002
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2003
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2004por Schönauer, Horst Otto“…The paper describes the CERN approach for a proton driver for a Neutrino Factory. Two main layouts are presented: the so-called CERN Reference Scenario, based on a 2.2 GeV linac and an alternative one, based on a 30 GeV synchrotron. …”
Publicado 2001
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2005por Goswami, S, Rangarajan, R, Agashe, K, Bandyopadhyay, A, Bhattacharya, K K, Brahmachari, B, Burgess, C, Chun, E J, Choudhury, D, Das-Prasanta, Kumar, Dighe, Amol S, Godbole, Rohini M, Gupta, N, Kaplinghat, M, Indumathi, D, Forshaw, J, Keum, Yu Y, Layek, B, Majumdar, D, Mahajan, N, Mehta, P, Mohapatra, Rabindra N, Mondal, N K, More, S, Nir, Y, Pakvasa, S, Parida, M K, Ravikumar, M, Rajasekaran, G, Ramadevi, P, Rindani, S D, Roy, D P, Roy, P, Sahu, N, Samanta, A, Shadmi, Y, Srivastava, A M, Sankar, S U, Vaidya, R, Yajnik, U“…This is the report of neutrino and astroparticle physics working group at WHEPP-8. …”
Publicado 2004
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2006
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2007
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2008
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2009por Migliozzi, P“…This paper reviews the current status and the physics program of the OPERA experiment with the future CNGS long baseline neutrino beam from CERN to the Gran Sasso Laboratory. …”
Publicado 2003
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2010“…Energy spectra, intensity and composition of the CERN to Gran Sasso CNGS neutrino beam for nu_mu-->nu_tau and nu_mu-->nu_e oscillation searches are presented. …”
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2011por Robbins, S“…The observation of neutrino flavour transformations of atmospheric neutrinos measured in Super-Kamiokande demands a theoretical explanation. …”
Publicado 2004
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2012
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2013
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2014“…We propose an explanation of the LSND evidence for electron antineutrino appearance based on neutrino decay. We introduce a heavy neutrino, which is produced in pion and muon decays because of a small mixing with muon neutrinos, and then decays into a scalar particle and a light neutrino, predominantly of the electron type. …”
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2015
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2016
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2017
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2018
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2019
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2020