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Record W2937696600 · doi:10.3847/1538-4365/ab29fd

The Event Horizon General Relativistic Magnetohydrodynamic Code Comparison Project

2019· article· en· W2937696600 on OpenAlexafffund
Oliver Porth, Koushik Chatterjee, Ramesh Narayan, Charles F. Gammie, Yosuke Mizuno, Peter Anninos, John G. Baker, Matteo Bugli, Chi‐kwan Chan, Jordy Davelaar, L. Del Zanna, Z. B. Etienne, P. Chris Fragile, Bernard Kelly, Matthew Liska, Sera Markoff, Jonathan C. McKinney, Bhupendra Mishra, Scott C. Noble, Héctor Olivares, Ben Prather, Luciano Rezzolla, Benjamin R. Ryan, James M. Stone, Niccolò Tomei, Christopher J. White, Ziri Younsi, Kazunori Akiyama, A. Alberdi, W. Alef, Keiichi Asada, Rebecca Azulay, Anne-Kathrin Baczko, David Ball, Mislav Baloković, John Barrett, Dan Bintley, Lindy Blackburn, W. Boland, Katherine L. Bouman, Geoffrey C. Bower, Michael Bremer, Christiaan D. Brinkerink, Roger Brissenden, S. Britzen, Avery E. Broderick, Dominique Broguière, Thomas Bronzwaer, Do‐Young Byun, J. E. Carlstrom, Andrew Chael, Shami Chatterjee, Ming‐Tang Chen, Yongjun 军 Chen 陈永, Ilje Cho, Pierre Christian, J. E. Conway, J. M. Cordes, G. Crew, Yuzhu Cui, Mariafelicia De Laurentis, Roger Deane, Jessica Dempsey, G. Desvignes, Sheperd S. Doeleman, Ralph P. Eatough, H. Falcke, Vincent L. Fish, Ed Fomalont, Raquel Fraga-Encinas, Bill Freeman, Per Friberg, Christian M. Fromm, José L. Gómez, Peter Galison, Roberto García, Olivier Gentaz, Boris Georgiev, C. Goddi, Roman Gold, Minfeng Gu, Mark Gurwell, Kazuhiro Hada, M. H. Hecht, Ronald Hesper, Luis C. Ho, Paul T. P. Ho, Mareki Honma, Lei 磊 Huang 黄, D. H. Hughes, Shiro Ikeda, Makoto Inoue, Sara Issaoun, D. J. James, Buell T. Jannuzi, Michaël Janssen, Britton Jeter, Wu Jiang, Michael D. Johnson, Svetlana G. Jorstad, Taehyun Jung, Mansour Karami, R. Karuppusamy, Tomohisa Kawashima, Garrett K. Keating, Mark Kettenis, Jae-Young Kim, Junhan Kim, Jongsoo Kim, Motoki Kino, Jun Yi Koay, Patrick M. Koch, Shoko Koyama, C. Krämer, T. P. Krichbaum, Cheng‐Yu Kuo, Tod R. Lauer, Sang-Sung Lee, Yanrong Li, M. Lindqvist, Kuo Liu, Elisabetta Liuzzo, Wen-Ping Lo, A. P. Lobanov, Laurent Loinard, C. J. Lonsdale, Ru-Sen Lu, Nicholas R. MacDonald, Daniel P. Marrone, Alan P. Marscher, I. Martí‐Vidal, Satoki Matsushita, Lynn D. Matthews, Lia Medeiros, K. M. Menten, Izumi Mizuno, J. M. Moran, Kotaro Moriyama, Monika Mościbrodzka, Cornelia Müller, Hiroshi Nagai, Neil M. Nagar, Masanori Nakamura, Gopal Narayanan, Iniyan Natarajan, R. Neri, Chunchong Ni, A. Noutsos, Hiroki Okino, Tomoaki Oyama, Feryal Özel, Daniel C. M. Palumbo, Nimesh Patel, Ue‐Li Pen, Dominic W. Pesce, Vincent Piétu, R. L. Plambeck, Aleksandar PopStefanija, Jorge A. Preciado-López, Dimitrios Psaltis, Hung-Yi Pu, Venkatessh Ramakrishnan, Ramprasad Rao, Mark G. Rawlings, Alexander W. Raymond, Bart Ripperda, Freek Roelofs, A. E. E. Rogers, E. Ros, Mel Rose, Arash Roshanineshat, Helge Rottmann, A. L. Roy, Chet Ruszczyk, K. L. J. Rygl, Salvador Sánchez, David Sánchez-Argüelles, Mahito Sasada, T. Savolainen, F. Peter Schloerb, K. Schüster, Lijing Shao, Zhi-Qiang Shen, Des Small, Bong Won Sohn, Jason Soohoo, Fumie Tazaki, Paul Tiede, R. P. J. Tilanus, Kenji Toma, Pablo Torné, Tyler Trent, Sascha Trippe, Shuichiro Tsuda, Ilse van Bemmel, Huib Jan van Langevelde, Daniel R. van Rossum, Jan Wagner, J. F. C. Wardle, Jonathan Weintroub, Norbert Wex, Robert Wharton, Maciek Wielgus, George N. Wong, Ken Young, André Young, J. A. Zensus, Guang-Yao Zhao, Shan-Shan Zhao, Ziyan Zhu

Bibliographic record

VenueThe Astrophysical Journal Supplement Series · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsCanadian Institute for Theoretical AstrophysicsCanadian Institute for Advanced ResearchUniversity of TorontoPerimeter InstituteUniversity of Waterloo
FundersLos Alamos National LaboratoryOffice of International Science and EngineeringNational Key Research and Development Program of ChinaConsejo Nacional de Ciencia y TecnologíaDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoJapan Society for the Promotion of ScienceLeibniz-GemeinschaftChina Scholarship CouncilJohn Templeton FoundationMinistry of Education, Culture, Sports, Science and TechnologyMinisterio de Economía y CompetitividadNatural Sciences and Engineering Research Council of CanadaNational Nuclear Security AdministrationInstitut Périmètre de physique théoriqueRecruitment Program of Global ExpertsUniversidad Nacional Autónoma de MéxicoLeibniz-RechenzentrumNational Natural Science Foundation of ChinaNational Research Foundation of KoreaGovernment of CanadaNational Institutes of Natural SciencesMinisterio de Ciencia, Innovación y UniversidadesNuclear Safety and Security CommissionComisión Nacional de Investigación Científica y TecnológicaGoddard Space Flight CenterGordon and Betty Moore FoundationMinistero dell’Istruzione, dell’Università e della RicercaGeneralitat ValencianaAcademy of FinlandMax-Planck-GesellschaftLawrence Livermore National LaboratoryChinese Academy of SciencesNederlandse Organisatie voor Wetenschappelijk OnderzoekInstituto de Astrofísica de AndalucíaHarvard UniversityGauss Centre for SupercomputingToray Science FoundationNational Research FoundationVetenskapsrådetU.S. Department of EnergyLeverhulme TrustEuropean CommissionNational Radio Astronomy ObservatoryCompute CanadaUniversities Space Research AssociationInternational Max Planck Research School for Environmental, Cellular and Molecular MicrobiologyNational Science FoundationAcademia SinicaIstituto Nazionale di Fisica NucleareDepartment of Science and Technology, Ministry of Science and Technology, IndiaRussian Science FoundationNational Aeronautics and Space Administration
KeywordsPhysicsEvent horizonMagnetorotational instabilityMagnetohydrodynamic driveGeneral relativityNeutron starAstrophysicsBlack hole (networking)Event (particle physics)MagnetohydrodynamicsTheoretical physicsComputer scienceMagnetic fieldComputer security

Abstract

fetched live from OpenAlex

Abstract Recent developments in compact object astrophysics, especially the discovery of merging neutron stars by LIGO, the imaging of the black hole in M87 by the Event Horizon Telescope, and high- precision astrometry of the Galactic Center at close to the event horizon scale by the GRAVITY experiment motivate the development of numerical source models that solve the equations of general relativistic magnetohydrodynamics (GRMHD). Here we compare GRMHD solutions for the evolution of a magnetized accretion flow where turbulence is promoted by the magnetorotational instability from a set of nine GRMHD codes: Athena++ , BHAC , Cosmos++ , ECHO , H-AMR , iharm3D , HARM-Noble , IllinoisGRMHD , and KORAL . Agreement among the codes improves as resolution increases, as measured by a consistently applied, specially developed set of code performance metrics. We conclude that the community of GRMHD codes is mature, capable, and consistent on these test problems.

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.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.004
metaresearch head score (Gemma)0.007
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.008
Threshold uncertainty score0.020

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0040.007
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0010.002
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0030.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0060.002

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 head0.011
GPT teacher head0.264
Teacher spread0.253 · 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

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations340
Published2019
Admission routes2
Has abstractyes

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