MétaCan
Menu
Back to cohort
Record W1759977769 · doi:10.3204/pubdb-2017-09959

IceCube-Gen2: A Vision for the Future of Neutrino Astronomy in Antarctica

2014· article· en· W1759977769 on OpenAlex
M. G. Aartsen, M. Ackermann, J. Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, D. Altmann, T. Anderson, G. Anton, C. Argüelles, T. C. Arlen, J. Auffenberg, Spencer Axani, X. Bai, I. Bartos, S. W. Barwick, V. Baum, R. Bay, J. J. Beatty, J. Becker Tjus, K.-H. Becker, S. BenZvi, P. Berghaus, D. Berley, E. Bernardini, A. Bernhard, D. Z. Besson, G. Binder, D. Bindig, M. Bissok, E. Blaufuss, J. Blumenthal, D. J. Boersma, Christoph Böhm, F. Bos, D. Bose, S. Böser, O. Botner, L. Brayeur, H.-P. Bretz, A. M. Brown, N. Buzinsky, J. Casey, M. Casier, E. Cheung, D. Chirkin, A. Christov, B. Christy, K. Clark, Lew Classen, F. Clevermann, S. Coenders, G. H. Collin, J. M. Conrad, D. F. Cowen, A. H. Cruz Silva, J. Daughhetee, J. C. Davis, M. Day, J. P. A. M. de André, C. De Clercq, S. De Ridder, P. Desiati, K. D. de Vries, T. DeYoung, M. Dunkman, R. Eagan, B. Eberhardt, Thomas Ehrhardt, B. Eichmann, J. Eisch, S. Euler, John Evans, P. A. Evenson, O. Fadiran, A. R. Fazely, Anatoli Fedynitch, J. Feintzeig, J. Felde, K. Filimonov, C. Finley, T. Fischer-Wasels, S. Flis, K. Frantzen, T. Fuchs, T. K. Gaisser, R. Gaïor, J. S. Gallagher, L. Gerhardt, D. Gier, L. Gladstone, T. Glüsenkamp, A. Goldschmidt, G. Golup, J. G. González, J. A. Goodman, D. Góra, D. Grant, P. Gretskov, J. C. Groh, C. Ha, Christian Haack, A. Haj Ismail, P. Hallen, A. Hallgren, F. Halzen, K. Hanson, J. Haugen, D. Hebecker, D. Heereman, D. Heinen, K. Helbing, R. Hellauer, D. Hellwig, S. Hickford, J. Hignight, G. C. Hill, K. D. Hoffman, R. Hoffmann, A. Homeier, K. Hoshina, F. Huang, W. Huelsnitz, P. O. Hulth, K. Hultqvist, A. Ishihara, E. Jacobi, J. Jacobsen, G. S. Japaridze, K. Jero, O. Jlelati, B. J. P. Jones, M. Jurković, O. Kalekin, A. Kappes, T. Karg, A. Karle, T. Katori, U. Katz, M. Kauer, A. Keivani, J. L. Kelley, Ali Kheirandish, J. Kiryluk, J. Kläs, J.-H. Köhne, G. Kohnen, H. Kolanoski, A. Koob, L. Köpke, Claudio Kopper, S. Kopper, D. J. Koskinen, M. Kowalski, C. B. Krauss, A. Kriesten, K. Krings, G. Kroll, M. Kroll, J. Kunnen, N. Kurahashi, T. Kuwabara, M. Labare, J. L. Lanfranchi, D. Larsen, M. J. Larson, M. Lesiak-Bzdak, M. Leuermann, J. M. LoSecco, J. Lünemann, J. Madsen, G. Maggi, K. B. M. Mahn, Szabolcs Márka, Z. Márka, R. Maruyama, K. Mase, H. S. Matis, R. Maunu, Frank McNally, K. Meagher, M. Medici, A. Meli, T. Meures, S. Miarecki, E. Middell, E. Middlemas, N. Milke, J. Miller, L. Mohrmann, T. Montaruli, R. W. Moore, R. Morse, R. Nahnhauer, Uwe Naumann, Hans Niederhausen, S. C. Nowicki, D. R. Nygren, A. Obertacke, S. Odrowski, A. Olivas, A. Omairat, A. O’Murchadha, T. Palczewski, L. Paul, Ö. Penek, Joshua Pepper, C. Pfendner, D. Pieloth, E. Pinat, J. L. Pinfold, J. Posselt, P. B. Price, G. T. Przybylski, J. Pütz, M. Quinnan, L. Rädel, M. Rameez, K. Rawlins, P. Redl, Ian Rees, R. Reimann, M. Relich, E. Resconi, W. Rhode, M. Richman, Benedikt Riedel, S. Robertson, J. P. Rodrigues, Martin Rongen, C. Rott, T. Ruhe, B. Ruzybayev, D. Ryckbosch, S. M. Saba, H. G. Sander, J. Sandroos, P. Sandstrom, M. Santander, S. Sarkar, K. Schatto, F. Scheriau, T. Schmidt, M. Schmitz, S. Schoenen, S. Schöneberg, A. Schönwald, A. Schukraft, L. Schulte, O. Schulz, D. Seckel, Y. Sestayo, S. Seunarine, M. H. Shaevitz, R. Shanidze, M. W. E. Smith, D. Soldin, S. Söldner‐Rembold, G. M. Spiczak, C. Spiering, M. Stamatikos, Todor Stanev, N. A. Stanisha, A. Stasik, T. Stezelberger, R. G. Stokstad, E. A. Strahler, L. R. Strom, N. L. Strotjohann, G. W. Sullivan, H. Taavola, I. Taboada, A. Taketa, A. Tamburro, Hiroki Tanaka, A. Tepe, S. Ter–Antonyan, A. Terliuk, andić, S. Tilav, P. A. Toale, M. N. Tobin, D. Tosi, M. Tselengidou, E. Unger, M. Usner, S. Vallecorsa, N. van Eijndhoven, J. Vandenbroucke, J. V. Santen, S. Vanheule, M. Vehring, M. Vöge, M. Vraeghe, C. Walck, M. Wallraff, Ch. Weaver, M. Wellons, Chris Wendt, S. Westerhoff, B. J. Whelan, N. Whitehorn, C. Wichary, K. Wiebe, C. H. Wiebusch, D. R. Williams, H. Wissing, M. Wolf, T. R. Wood, K. Woschnagg, Steven Wren, D. L. Xu, X. W. Xu, Y. Xu, G. Yodh, S. Yoshida, P. Zarzhitsky, J. Ziemann, M. Zoll

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

fundA Canadian funder is recorded on the work.
no affNo Canadian affiliation: this work is invisible to an affiliation-only frame.
No Canadian affiliation. An affiliation-only frame, the usual design, would never have seen this work. It is one of the works that make the case for inverting the frame.

Bibliographic record

VenueResearch Explorer (The University of Manchester) · 2014
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsnot available
FundersOffice of Polar ProgramsBundesministerium für Bildung und ForschungMarsden FundJapan Society for the Promotion of ScienceU.S. Department of EnergyVetenskapsrådetDivision of Polar ProgramsNatural Sciences and Engineering Research Council of CanadaKnut och Alice Wallenbergs StiftelseNational Research Foundation of KoreaFonds Wetenschappelijk OnderzoekNational Science FoundationBelgian Federal Science Policy OfficeDeutsche ForschungsgemeinschaftNational Research FoundationWestern Canada Research GridVlaamse regeringUniversity of OxfordCompute CanadaFonds De La Recherche Scientifique - FNRSPolarforskningssekretariatetHelmholtz Alliance for Astroparticle PhysicsDanmarks GrundforskningsfondColumbia UniversitySchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
KeywordsAstrobiologyAstronomyNeutrinoPhysicsParticle physics

Abstract

fetched live from OpenAlex

The recent observation by the IceCube neutrino observatory of an astrophysical flux of neutrinos represents the 'first light' in the nascent field of neutrino astronomy. The observed diffuse neutrino flux seems to suggest a much larger level of hadronic activity in the non-thermal universe than previously thought and suggests a rich discovery potential for a larger neutrino observatory. This document presents a vision for an substantial expansion of the current IceCube detector, IceCube-Gen2, including the aim of instrumenting a $10\,\mathrm{km}^3$ volume of clear glacial ice at the South Pole to deliver substantial increases in the astrophysical neutrino sample for all flavors. A detector of this size would have a rich physics program with the goal to resolve the sources of these astrophysical neutrinos, discover GZK neutrinos, and be a leading observatory in future multi-messenger astronomy programs.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Other design · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.728
Threshold uncertainty score0.295

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0010.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.025
GPT teacher head0.267
Teacher spread0.242 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it