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001     390903
005     20250730103920.0
024 7 _ |a 10.1088/1361-6471/44/5/054006
|2 doi
024 7 _ |a 0305-4616
|2 ISSN
024 7 _ |a 0954-3899
|2 ISSN
024 7 _ |a 1361-6471
|2 ISSN
024 7 _ |a arXiv:1607.02671
|2 arXiv
024 7 _ |a WOS:000399127900001
|2 WOS
024 7 _ |a inspire:1475004
|2 inspire
024 7 _ |a altmetric:9615483
|2 altmetric
024 7 _ |a 10.3204/PUBDB-2017-09958
|2 datacite_doi
024 7 _ |a openalex:W2595337983
|2 openalex
037 _ _ |a PUBDB-2017-09958
041 _ _ |a English
082 _ _ |a 530
088 1 _ |a arXiv:1607.02671
088 _ _ |a arXiv:1607.02671
|2 arXiv
100 1 _ |a Aartsen, M. G.
|b 0
245 _ _ |a PINGU: A Vision for Neutrino and Particle Physics at the South Pole
260 _ _ |a Bristol
|c 2017
|b IOP Publ.
336 7 _ |a article
|2 DRIVER
336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Report
|0 PUB:(DE-HGF)29
|2 PUB:(DE-HGF)
|m report
336 7 _ |a Journal Article
|b journal
|m journal
|0 PUB:(DE-HGF)16
|s 1518088198_17291
|2 PUB:(DE-HGF)
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a Journal Article
|0 0
|2 EndNote
500 _ _ |a 28 pages, 10 figures, submitted to J. Phys. G
520 _ _ |a The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill extension to the IceCube Neutrino Observatory. With detection technology modeled closely on the successful IceCube example, PINGU will provide a 6 Mton effective mass for neutrino detection with an energy threshold of a few GeV. With an unprecedented sample of over 60 000 atmospheric neutrinos per year in this energy range, PINGU will make highly competitive measurements of neutrino oscillation parameters in an energy range over an order of magnitude higher than long-baseline neutrino beam experiments. PINGU will measure the mixing parameters ${\theta }_{23}$ and ${\rm{\Delta }}{m}_{32}^{2}$, including the octant of ${\theta }_{23}$ for a wide range of values, and determine the neutrino mass ordering at $3\sigma $ median significance within five years of operation. PINGU’s high precision measurement of the rate of ${\nu }_{\tau }$ appearance will provide essential tests of the unitarity of the 3 × 3 PMNS neutrino mixing matrix. PINGU will also improve the sensitivity of searches for low mass dark matter in the Sun, use neutrino tomography to directly probe the composition of the Earth’s core, and improve IceCube’s sensitivity to neutrinos from Galactic supernovae. Reoptimization of the PINGU design has permitted substantial reduction in both cost and logistical requirements while delivering performance nearly identical to configurations previously studied.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF3-613)
|0 G:(DE-HGF)POF3-613
|c POF3-613
|f POF III
|x 0
588 _ _ |a Dataset connected to CrossRef, INSPIRE
650 _ 7 |a neutrino: mixing
|2 INSPIRE
650 _ 7 |a neutrino: mass
|2 INSPIRE
650 _ 7 |a neutrino: oscillation
|2 INSPIRE
650 _ 7 |a neutrino: mixing angle
|2 INSPIRE
650 _ 7 |a neutrino: mass difference
|2 INSPIRE
650 _ 7 |a neutrino/tau: particle identification
|2 INSPIRE
650 _ 7 |a neutrino: atmosphere
|2 INSPIRE
650 _ 7 |a neutrino: beam
|2 INSPIRE
650 _ 7 |a energy: threshold
|2 INSPIRE
650 _ 7 |a dark matter: mass: low
|2 INSPIRE
650 _ 7 |a dark matter: solar
|2 INSPIRE
650 _ 7 |a WIMP: solar
|2 INSPIRE
650 _ 7 |a PINGU
|2 INSPIRE
650 _ 7 |a IceCube
|2 INSPIRE
650 _ 7 |a sensitivity
|2 INSPIRE
650 _ 7 |a precision measurement
|2 INSPIRE
650 _ 7 |a observatory
|2 INSPIRE
650 _ 7 |a performance
|2 INSPIRE
650 _ 7 |a unitarity
|2 INSPIRE
650 _ 7 |a neutrino: supernova
|2 INSPIRE
650 _ 7 |a upgrade
|2 INSPIRE
650 _ 7 |a galaxy
|2 INSPIRE
650 _ 7 |a pole
|2 INSPIRE
650 _ 7 |a experimental results
|2 INSPIRE
693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
|5 EXP:(DE-MLZ)NOSPEC-20140101
|e No specific instrument
|x 0
700 1 _ |a Abraham, K.
|b 1
700 1 _ |a Ackermann, Markus
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700 1 _ |a Adams, J.
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700 1 _ |a Aguilar, J. A.
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700 1 _ |a Ahlers, M.
|b 5
700 1 _ |a Ahrens, M.
|b 6
700 1 _ |a Altmann, D.
|b 7
700 1 _ |a Andeen, K.
|b 8
700 1 _ |a Anderson, T.
|b 9
700 1 _ |a Ansseau, I.
|b 10
700 1 _ |a Anton, G.
|b 11
700 1 _ |a Archinger, M.
|b 12
700 1 _ |a Arguelles, C.
|b 13
700 1 _ |a Arlen, T. C.
|b 14
700 1 _ |a Auffenberg, J.
|b 15
700 1 _ |a Axani, S.
|b 16
700 1 _ |a Bai, X.
|b 17
700 1 _ |a Bartos, I.
|b 18
700 1 _ |a Barwick, S. W.
|b 19
700 1 _ |a Baum, V.
|b 20
700 1 _ |a Bay, R.
|b 21
700 1 _ |a Beatty, J. J.
|b 22
700 1 _ |a Tjus, J. Becker
|b 23
700 1 _ |a Becker, K. H.
|b 24
700 1 _ |a BenZvi, S.
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700 1 _ |a Berghaus, P.
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700 1 _ |a Berley, D.
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700 1 _ |a Bernardini, E.
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|b 28
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700 1 _ |a Bernhard, A.
|b 29
700 1 _ |a Besson, D. Z.
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700 1 _ |a Binder, G.
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700 1 _ |a Bindig, D.
|b 32
700 1 _ |a Bissok, M.
|b 33
700 1 _ |a Blaufuss, E.
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700 1 _ |a Blot, S.
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|b 35
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700 1 _ |a Bohm, C.
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700 1 _ |a Borner, M.
|b 38
700 1 _ |a Bos, F.
|b 39
700 1 _ |a Bose, D.
|b 40
700 1 _ |a Boser, S.
|b 41
700 1 _ |a Botner, O.
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700 1 _ |a Braun, J.
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700 1 _ |a Casier, M.
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700 1 _ |a Cheung, E.
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700 1 _ |a Chirkin, D.
|b 50
700 1 _ |a Christov, A.
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700 1 _ |a Clark, K.
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700 1 _ |a Classen, L.
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700 1 _ |a Coenders, S.
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700 1 _ |a Collin, G. H.
|b 55
700 1 _ |a Conrad, J. M.
|b 56
700 1 _ |a Cowen, D. F.
|b 57
700 1 _ |a Cross, R.
|b 58
700 1 _ |a Day, M.
|b 59
700 1 _ |a de Andre, J. P. A. M.
|b 60
700 1 _ |a De Clercq, C.
|b 61
700 1 _ |a del Pino Rosendo, E.
|b 62
700 1 _ |a Dembinski, H.
|b 63
700 1 _ |a De Ridder, S.
|b 64
700 1 _ |a Desiati, P.
|b 65
700 1 _ |a de Vries, K. D.
|b 66
700 1 _ |a de Wasseige, G.
|b 67
700 1 _ |a de With, M.
|b 68
700 1 _ |a DeYoung, T.
|b 69
700 1 _ |a Diaz-Velez, J. C.
|b 70
700 1 _ |a di Lorenzo, V.
|b 71
700 1 _ |a Dujmovic, H.
|b 72
700 1 _ |a Dumm, J. P.
|b 73
700 1 _ |a Dunkman, M.
|b 74
700 1 _ |a Eberhardt, B.
|b 75
700 1 _ |a Ehrhardt, T.
|b 76
700 1 _ |a Eichmann, B.
|b 77
700 1 _ |a Eller, P.
|b 78
700 1 _ |a Euler, S.
|b 79
700 1 _ |a Evans, J. J.
|b 80
700 1 _ |a Evenson, P. A.
|b 81
700 1 _ |a Fahey, S.
|b 82
700 1 _ |a Fazely, A. R.
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700 1 _ |a Feintzeig, J.
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700 1 _ |a Felde, J.
|b 85
700 1 _ |a Filimonov, K.
|b 86
700 1 _ |a Finley, C.
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700 1 _ |a Flis, S.
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700 1 _ |a Friedman, E.
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|b 94
700 1 _ |a Gerhardt, L.
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700 1 _ |a Ghorbani, K.
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|b 104
700 1 _ |a Griffith, Z.
|b 105
700 1 _ |a Haack, C.
|b 106
700 1 _ |a Haj Ismail, A.
|b 107
700 1 _ |a Hallgren, A.
|b 108
700 1 _ |a Halzen, F.
|b 109
700 1 _ |a Hansen, E.
|b 110
700 1 _ |a Hansmann, B.
|b 111
700 1 _ |a Hansmann, T.
|b 112
700 1 _ |a Hanson, K.
|b 113
700 1 _ |a Haugen, J.
|b 114
700 1 _ |a Hebecker, D.
|b 115
700 1 _ |a Heereman, D.
|b 116
700 1 _ |a Helbing, K.
|b 117
700 1 _ |a Hellauer, R.
|b 118
700 1 _ |a Hickford, S.
|b 119
700 1 _ |a Hignight, J.
|b 120
700 1 _ |a Hill, G. C.
|b 121
700 1 _ |a Hoffman, K. D.
|b 122
700 1 _ |a Hoffmann, R.
|b 123
700 1 _ |a Holzapfel, K.
|b 124
700 1 _ |a Hoshina, K.
|b 125
700 1 _ |a Huang, F.
|b 126
700 1 _ |a Huber, M.
|b 127
700 1 _ |a Hultqvist, K.
|b 128
700 1 _ |a In, S.
|b 129
700 1 _ |a Ishihara, A.
|b 130
700 1 _ |a Jacobi, E.
|0 P:(DE-H253)PIP1014043
|b 131
|u desy
700 1 _ |a Japaridze, G. S.
|b 132
700 1 _ |a Jeong, M.
|b 133
700 1 _ |a Jero, K.
|b 134
700 1 _ |a Jones, B. J. P.
|b 135
700 1 _ |a Jurkovic, M.
|b 136
700 1 _ |a Kalekin, O.
|b 137
700 1 _ |a Kappes, A.
|b 138
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|b 139
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700 1 _ |a Karle, A.
|b 141
700 1 _ |a Katori, T.
|b 142
700 1 _ |a Katz, U.
|b 143
700 1 _ |a Kauer, M.
|b 144
700 1 _ |a Keivani, A.
|b 145
700 1 _ |a Kelley, J. L.
|b 146
700 1 _ |a Kemp, J.
|b 147
700 1 _ |a Kheirandish, A.
|b 148
700 1 _ |a Kim, M.
|b 149
700 1 _ |a Kintscher, T.
|0 P:(DE-H253)PIP1014842
|b 150
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|b 151
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|b 152
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|b 153
700 1 _ |a Kohnen, G.
|b 154
700 1 _ |a Koirala, R.
|b 155
700 1 _ |a Kolanoski, H.
|b 156
700 1 _ |a Konietz, R.
|b 157
700 1 _ |a Kopke, L.
|b 158
700 1 _ |a Kopper, C.
|b 159
700 1 _ |a Kopper, S.
|b 160
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|b 161
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|0 P:(DE-H253)PIP1006050
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|b 163
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|b 167
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|b 168
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|b 169
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|b 170
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|b 172
700 1 _ |a Lanfranchi, J. L.
|b 173
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|b 175
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|b 178
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700 1 _ |a Lu, L.
|b 181
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|b 182
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|b 183
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|b 184
700 1 _ |a Mahn, K. B. M.
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700 1 _ |a Mancina, S.
|b 186
700 1 _ |a Mandalia, S.
|b 187
700 1 _ |a Mandelartz, M.
|b 188
700 1 _ |a Marka, S.
|b 189
700 1 _ |a Marka, Z.
|b 190
700 1 _ |a Maruyama, R.
|b 191
700 1 _ |a Mase, K.
|b 192
700 1 _ |a Maunu, R.
|b 193
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|b 194
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|b 195
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700 1 _ |a Menne, T.
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700 1 _ |a Meures, T.
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700 1 _ |a Pollmann, A. Obertacke
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700 1 _ |a Olivas, A.
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700 1 _ |a O'Murchadha, A.
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700 1 _ |a Palazzo, A.
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700 1 _ |a Palczewski, T.
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700 1 _ |a Pandya, H.
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700 1 _ |a Pankova, D. V.
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700 1 _ |a Penek, O.
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700 1 _ |a Pepper, J. A.
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700 1 _ |a Perez de los Heros, C.
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700 1 _ |a Pinat, E.
|b 225
700 1 _ |a Pinfold, J. L.
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700 1 _ |a Price, P. B.
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700 1 _ |a Przybylski, G. T.
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700 1 _ |a Quinnan, M.
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700 1 _ |a Raab, C.
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700 1 _ |a Radel, L.
|b 231
700 1 _ |a Rameez, M.
|b 232
700 1 _ |a Rawlins, K.
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700 1 _ |a Rhode, W.
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|b 241
700 1 _ |a Rongen, M.
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700 1 _ |a Rott, C.
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700 1 _ |a Ryckbosch, D.
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700 1 _ |a Rysewyk, D.
|b 246
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700 1 _ |a Sanchez Herrera, S. E.
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700 1 _ |a Sandrock, A.
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700 1 _ |a Sandstrom, P.
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|0 P:(DE-H253)PIP1005697
|b 253
|u desy
700 1 _ |a Schimp, M.
|b 254
700 1 _ |a Schlunder, P.
|b 255
700 1 _ |a Schmidt, T.
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700 1 _ |a Schoenen, S.
|b 257
700 1 _ |a Schoneberg, S.
|b 258
700 1 _ |a Schumacher, L.
|b 259
700 1 _ |a Seckel, D.
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700 1 _ |a Seunarine, S.
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700 1 _ |a Shaevitz, M. H.
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700 1 _ |a Soldin, D.
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700 1 _ |a Soldner-Rembold, S.
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700 1 _ |a Song, M.
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700 1 _ |a Stahlberg, M.
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|b 270
700 1 _ |a Steuer, A.
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|b 280
700 1 _ |a Taketa, A.
|b 281
700 1 _ |a Tanaka, H. K. M.
|b 282
700 1 _ |a Tatar, J.
|b 283
700 1 _ |a Tenholt, F.
|b 284
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|b 285
700 1 _ |a Terliuk, A.
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|b 289
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|b 290
700 1 _ |a Toscano, S.
|b 291
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|b 292
700 1 _ |a Tselengidou, M.
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700 1 _ |a Vraeghe, M.
|b 305
700 1 _ |a Walck, C.
|b 306
700 1 _ |a Wallace, A.
|b 307
700 1 _ |a Wallraff, M.
|b 308
700 1 _ |a Wandkowsky, N.
|b 309
700 1 _ |a Weaver, Ch.
|b 310
700 1 _ |a Weiss, M. J.
|b 311
700 1 _ |a Wendt, C.
|b 312
700 1 _ |a Westerhoff, S.
|b 313
700 1 _ |a Whelan, B. J.
|b 314
700 1 _ |a Wickmann, S.
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700 1 _ |a Wiebe, K.
|b 316
700 1 _ |a Wiebusch, C. H.
|b 317
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|b 318
700 1 _ |a Williams, D. R.
|b 319
700 1 _ |a Wills, L.
|b 320
700 1 _ |a Wolf, M.
|b 321
700 1 _ |a Wood, T. R.
|b 322
700 1 _ |a Woolsey, E.
|b 323
700 1 _ |a Woschnagg, K.
|b 324
700 1 _ |a Wren, S.
|b 325
700 1 _ |a Xu, D. L.
|b 326
700 1 _ |a Xu, X. W.
|b 327
700 1 _ |a Xu, Y.
|b 328
700 1 _ |a Yanez, J. P.
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|b 329
|u desy
700 1 _ |a Yodh, G.
|b 330
700 1 _ |a Yoshida, S.
|b 331
700 1 _ |a Zoll, M.
|b 332
700 1 _ |a IceCube Collaboration
|0 P:(DE-HGF)0
|b 333
|e Collaboration author
773 _ _ |a 10.1088/1361-6471/44/5/054006
|g Vol. G44, no. 5, p. 054006 -
|0 PERI:(DE-600)1472964-7
|n 5
|p 054006 -
|t Journal of physics / G
|v 44
|y 2017
|x 1361-6471
856 4 _ |y OpenAccess
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