Academic Bibliography

 Search 200 years of publications by Ghent University researchers.
Advanced search
1 file | 2.73 MB
Add to list
  1. Search results
  2. PINGU : a vision for neutrino and par...

PINGU : a vision for neutrino and particle physics at the South Pole

MG Aartsen, K Abraham, M Ackermann, J Adams, JA Aguilar, M Ahlers, M Ahrens, D Altmann, K Andeen, T Anderson, et al.
(2017) JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS. 44(5).
Author
Organization
Abstract
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 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(T) appearance will provide essential tests of the unitarity of the 3 x 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.
Keywords
neutrino oscillations, atmospheric neutrinos, IceCube Neutrino Observatory, PINGU, ATMOSPHERIC NEUTRINOS, SUPERNOVA DETECTION, OSCILLATIONS, ICECUBE, SYSTEM, MATTER, KM3NET

Downloads

  • Download
    094.pdf
    • full text
    • |
    • open access
    • |
    • PDF
    • |
    • 2.73 MB

Citation

Please use this url to cite or link to this publication:

MLA
Aartsen, MG, et al. “PINGU : A Vision for Neutrino and Particle Physics at the South Pole.” JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS, vol. 44, no. 5, 2017, doi:10.1088/1361-6471/44/5/054006.
APA
Aartsen, M., Abraham, K., Ackermann, M., Adams, J., Aguilar, J., Ahlers, M., … Zoll, M. (2017). PINGU : a vision for neutrino and particle physics at the South Pole. JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS, 44(5). https://doi.org/10.1088/1361-6471/44/5/054006
Chicago author-date
Aartsen, MG, K Abraham, M Ackermann, J Adams, JA Aguilar, M Ahlers, M Ahrens, et al. 2017. “PINGU : A Vision for Neutrino and Particle Physics at the South Pole.” JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS 44 (5). https://doi.org/10.1088/1361-6471/44/5/054006.
Chicago author-date (all authors)
Aartsen, MG, K Abraham, M Ackermann, J Adams, JA Aguilar, M Ahlers, M Ahrens, D Altmann, K Andeen, T Anderson, I Ansseau, G Anton, M Archinger, C Arguelles, TC Arlen, J Auffenberg, S Axani, X Bai, I Bartos, SW Barwick, V Baum, R Bay, JJ Beatty, J Becker Tjus, K-H Becker, S BenZvi, P Berghaus, D Berley, E Bernardini, A Bernhard, DZ Besson, G Binder, D Bindig, M Bissok, E Blaufuss, S Blot, DJ Boersma, C Bohm, M Boerner, F Bos, D Bose, S Boeser, O Botner, J Braun, L Brayeur, H-P Bretz, A Burgman, T Carver, M Casier, E Cheung, D Chirkin, A Christov, K Clark, L Classen, S Coenders, GH Collin, JM Conrad, DF Cowen, R Cross, M Day, JPAM de Andre, C De Clercq, E Pino del Rosendo, H Dembinski, Sam De Ridder, P Desiati, KD de Vries, G de Wasseige, M de With, T DeYoung, JC Diaz-Velez, V di Lorenzo, H Dujmovic, JP Dumm, M Dunkman, B Eberhardt, T Ehrhardt, B Eichmann, P Eller, S Euler, JJ Evans, PA Evenson, S Fahey, AR Fazely, J Feintzeig, J Felde, K Filimonov, C Finley, S Flis, C-C Foesig, A Franckowiak, E Friedman, T Fuchs, TK Gaisser, J Gallagher, L Gerhardt, K Ghorbani, W Giang, L Gladstone, M Glagla, T Gluesenkamp, A Goldschmidt, G Golup, JG Gonzalez, D Grant, Z Griffith, C Haack, Abd Al Karim Haj Ismail, A Hallgren, F Halzen, E Hansen, B Hansmann, T Hansmann, K Hanson, J Haugen, D Hebecker, D Heereman, K Helbing, R Hellauer, S Hickford, J Hignight, GC Hill, KD Hoffman, R Hoffmann, K Holzapfel, K Hoshina, F Huang, M Huber, K Hultqvist, S In, A Ishihara, E Jacobi, GS Japaridze, M Jeong, K Jero, BJP Jones, M Jurkovic, O Kalekin, A Kappes, G Karagiorgi, T Karg, A Karle, T Katori, U Katz, M Kauer, A Keivani, JL Kelley, J Kemp, A Kheirandish, M Kim, T Kintscher, J Kiryluk, T Kittler, SR Klein, G Kohnen, R Koirala, H Kolanoski, R Konietz, L Koepke, C Kopper, S Kopper, DJ Koskinen, M Kowalski, CB Krauss, K Krings, M Kroll, G Krueckl, C Krueger, J Kunnen, S Kunwar, N Kurahashi, T Kuwabara, Mathieu Labare, JL Lanfranchi, MJ Larson, F Lauber, D Lennarz, M Lesiak-Bzdak, M Leuermann, J Leuner, J LoSecco, L Lu, J Lunemann, J Madsen, G Maggi, KBM Mahn, S Mancina, S Mandalia, M Mandelartz, S Marka, Z Marka, R Maruyama, K Mase, R Maunu, F McNally, K Meagher, M Medici, M Meier, Athina Meli, T Menne, G Merino, T Meures, S Miarecki, L Mohrmann, T Montaruli, RW Moore, M Moulai, R Nahnhauer, U Naumann, G Neer, H Niederhausen, SC Nowicki, DR Nygren, A Obertacke Pollmann, A Olivas, A O’Murchadha, A Palazzo, T Palczewski, H Pandya, DV Pankova, Oe Penek, JA Pepper, C Perez de los Heros, TC Petersen, D Pieloth, E Pinat, JL Pinfold, PB Price, GT Przybylski, M Quinnan, C Raab, L Raedel, M Rameez, K Rawlins, R Reimann, B Relethford, M Relich, E Resconi, W Rhode, M Richman, B Riedel, S Robertson, M Rongen, C Rott, T Ruhe, Dirk Ryckbosch, D Rysewyk, L Sabbatini, SE Sanchez Herrera, A Sandrock, J Sandroos, P Sandstrom, S Sarkar, K Satalecka, M Schimp, P Schlunder, T Schmidt, S Schoenen, S Schoeneberg, L Schumacher, D Seckel, S Seunarine, MH Shaevitz, D Soldin, S Soeldner-Rembold, M Song, GM Spiczak, C Spiering, M Stahlberg, T Stanev, A Stasik, A Steuer, T Stezelberger, RG Stokstad, A Stoessl, R Strom, NL Strotjohann, GW Sullivan, M Sutherland, H Taavola, I Taboada, A Taketa, HKM Tanaka, J Tatar, F Tenholt, S Ter-Antonyan, A Terliuk, G Tesic, S Tilav, PA Toale, MN Tobin, S Toscano, D Tosi, M Tselengidou, A Turcati, E Unger, M Usner, J Vandenbroucke, N van Eijndhoven, Sander Vanheule, M van Rossem, J van Santen, J Veenkamp, M Vehring, M Voge, Matthias Vraeghe, C Walck, A Wallace, M Wallraff, N Wandkowsky, Ch Weaver, MJ Weiss, C Wendt, S Westerhoff, BJ Whelan, S Wickmann, K Wiebe, CH Wiebusch, L Wille, DR Williams, L. Wills, M Wolf, TR Wood, E Woolsey, K Woschnagg, S Wren, DL Xu, XW Xu, Y Xu, JP Yanez, G Yodh, S Yoshida, and M Zoll. 2017. “PINGU : A Vision for Neutrino and Particle Physics at the South Pole.” JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS 44 (5). doi:10.1088/1361-6471/44/5/054006.
Vancouver
1.
Aartsen M, Abraham K, Ackermann M, Adams J, Aguilar J, Ahlers M, et al. PINGU : a vision for neutrino and particle physics at the South Pole. JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS. 2017;44(5).
IEEE
[1]
M. Aartsen et al., “PINGU : a vision for neutrino and particle physics at the South Pole,” JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS, vol. 44, no. 5, 2017.
@article{8565622,
  abstract     = {{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 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(T) appearance will provide essential tests of the unitarity of the 3 x 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.}},
  articleno    = {{054006}},
  author       = {{Aartsen, MG and Abraham, K and Ackermann, M and Adams, J and Aguilar, JA and Ahlers, M and Ahrens, M and Altmann, D and Andeen, K and Anderson, T and Ansseau, I and Anton, G and Archinger, M and Arguelles, C and Arlen, TC and Auffenberg, J and Axani, S and Bai, X and Bartos, I and Barwick, SW and Baum, V and Bay, R and Beatty, JJ and Becker Tjus, J and Becker, K-H and BenZvi, S and Berghaus, P and Berley, D and Bernardini, E and Bernhard, A and Besson, DZ and Binder, G and Bindig, D and Bissok, M and Blaufuss, E and Blot, S and Boersma, DJ and Bohm, C and Boerner, M and Bos, F and Bose, D and Boeser, S and Botner, O and Braun, J and Brayeur, L and Bretz, H-P and Burgman, A and Carver, T and Casier, M and Cheung, E and Chirkin, D and Christov, A and Clark, K and Classen, L and Coenders, S and Collin, GH and Conrad, JM and Cowen, DF and Cross, R and Day, M and de Andre, JPAM and De Clercq, C and Pino del Rosendo, E and Dembinski, H and De Ridder, Sam and Desiati, P and de Vries, KD and de Wasseige, G and de With, M and DeYoung, T and Diaz-Velez, JC and di Lorenzo, V and Dujmovic, H and Dumm, JP and Dunkman, M and Eberhardt, B and Ehrhardt, T and Eichmann, B and Eller, P and Euler, S and Evans, JJ and Evenson, PA and Fahey, S and Fazely, AR and Feintzeig, J and Felde, J and Filimonov, K and Finley, C and Flis, S and Foesig, C-C and Franckowiak, A and Friedman, E and Fuchs, T and Gaisser, TK and Gallagher, J and Gerhardt, L and Ghorbani, K and Giang, W and Gladstone, L and Glagla, M and Gluesenkamp, T and Goldschmidt, A and Golup, G and Gonzalez, JG and Grant, D and Griffith, Z and Haack, C and Haj Ismail, Abd Al Karim and Hallgren, A and Halzen, F and Hansen, E and Hansmann, B and Hansmann, T and Hanson, K and Haugen, J and Hebecker, D and Heereman, D and Helbing, K and Hellauer, R and Hickford, S and Hignight, J and Hill, GC and Hoffman, KD and Hoffmann, R and Holzapfel, K and Hoshina, K and Huang, F and Huber, M and Hultqvist, K and In, S and Ishihara, A and Jacobi, E and Japaridze, GS and Jeong, M and Jero, K and Jones, BJP and Jurkovic, M and Kalekin, O and Kappes, A and Karagiorgi, G and Karg, T and Karle, A and Katori, T and Katz, U and Kauer, M and Keivani, A and Kelley, JL and Kemp, J and Kheirandish, A and Kim, M and Kintscher, T and Kiryluk, J and Kittler, T and Klein, SR and Kohnen, G and Koirala, R and Kolanoski, H and Konietz, R and Koepke, L and Kopper, C and Kopper, S and Koskinen, DJ and Kowalski, M and Krauss, CB and Krings, K and Kroll, M and Krueckl, G and Krueger, C and Kunnen, J and Kunwar, S and Kurahashi, N and Kuwabara, T and Labare, Mathieu and Lanfranchi, JL and Larson, MJ and Lauber, F and Lennarz, D and Lesiak-Bzdak, M and Leuermann, M and Leuner, J and LoSecco, J and Lu, L and Lunemann, J and Madsen, J and Maggi, G and Mahn, KBM and Mancina, S and Mandalia, S and Mandelartz, M and Marka, S and Marka, Z and Maruyama, R and Mase, K and Maunu, R and McNally, F and Meagher, K and Medici, M and Meier, M and Meli, Athina and Menne, T and Merino, G and Meures, T and Miarecki, S and Mohrmann, L and Montaruli, T and Moore, RW and Moulai, M and Nahnhauer, R and Naumann, U and Neer, G and Niederhausen, H and Nowicki, SC and Nygren, DR and Obertacke Pollmann, A and Olivas, A and O'Murchadha, A and Palazzo, A and Palczewski, T and Pandya, H and Pankova, DV and Penek, Oe and Pepper, JA and Perez de los Heros, C and Petersen, TC and Pieloth, D and Pinat, E and Pinfold, JL and Price, PB and Przybylski, GT and Quinnan, M and Raab, C and Raedel, L and Rameez, M and Rawlins, K and Reimann, R and Relethford, B and Relich, M and Resconi, E and Rhode, W and Richman, M and Riedel, B and Robertson, S and Rongen, M and Rott, C and Ruhe, T and Ryckbosch, Dirk and Rysewyk, D and Sabbatini, L and Sanchez Herrera, SE and Sandrock, A and Sandroos, J and Sandstrom, P and Sarkar, S and Satalecka, K and Schimp, M and Schlunder, P and Schmidt, T and Schoenen, S and Schoeneberg, S and Schumacher, L and Seckel, D and Seunarine, S and Shaevitz, MH and Soldin, D and Soeldner-Rembold, S and Song, M and Spiczak, GM and Spiering, C and Stahlberg, M and Stanev, T and Stasik, A and Steuer, A and Stezelberger, T and Stokstad, RG and Stoessl, A and Strom, R and Strotjohann, NL and Sullivan, GW and Sutherland, M and Taavola, H and Taboada, I and Taketa, A and Tanaka, HKM and Tatar, J and Tenholt, F and Ter-Antonyan, S and Terliuk, A and Tesic, G and Tilav, S and Toale, PA and Tobin, MN and Toscano, S and Tosi, D and Tselengidou, M and Turcati, A and Unger, E and Usner, M and Vandenbroucke, J and van Eijndhoven, N and Vanheule, Sander and van Rossem, M and van Santen, J and Veenkamp, J and Vehring, M and Voge, M and Vraeghe, Matthias and Walck, C and Wallace, A and Wallraff, M and Wandkowsky, N and Weaver, Ch and Weiss, MJ and Wendt, C and Westerhoff, S and Whelan, BJ and Wickmann, S and Wiebe, K and Wiebusch, CH and Wille, L and Williams, DR and Wills, L. and Wolf, M and Wood, TR and Woolsey, E and Woschnagg, K and Wren, S and Xu, DL and Xu, XW and Xu, Y and Yanez, JP and Yodh, G and Yoshida, S and Zoll, M}},
  issn         = {{0954-3899}},
  journal      = {{JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS}},
  keywords     = {{neutrino oscillations,atmospheric neutrinos,IceCube Neutrino Observatory,PINGU,ATMOSPHERIC NEUTRINOS,SUPERNOVA DETECTION,OSCILLATIONS,ICECUBE,SYSTEM,MATTER,KM3NET}},
  language     = {{eng}},
  number       = {{5}},
  pages        = {{19}},
  title        = {{PINGU : a vision for neutrino and particle physics at the South Pole}},
  url          = {{http://dx.doi.org/10.1088/1361-6471/44/5/054006}},
  volume       = {{44}},
  year         = {{2017}},
}
Altmetric
View in Altmetric
Web of Science
Times cited: