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Gravitational Test beyond the First Post-Newtonian Order with the Shadow of the M87 Black Hole

2020· article· en· W3091374297 on OpenAlexafffund
Dimitrios Psaltis, Lia Medeiros, Pierre Christian, Feryal Özel, Kazunori Akiyama, W. Alef, Keiichi Asada, Rebecca Azulay, David Ball, Mislav Baloković, John Barrett, Dan Bintley, Lindy Blackburn, W. Boland, Geoffrey C. Bower, Michael Bremer, Christiaan D. Brinkerink, Roger Brissenden, S. Britzen, Dominique Broguière, Thomas Bronzwaer, Do‐Young Byun, J. E. Carlstrom, Andrew Chael, Chi‐kwan Chan, Shami Chatterjee, Koushik Chatterjee, Ming‐Tang Chen, Xiaopeng Cheng, Ilje Cho, J. E. Conway, J. M. Cordes, G. Crew, Yuzhu Cui, Jordy Davelaar, Mariafelicia De Laurentis, Roger Deane, Jessica Dempsey, G. Desvignes, Jason Dexter, Ralph P. Eatough, H. Falcke, Vincent L. Fish, Ed Fomalont, Raquel Fraga-Encinas, Per Friberg, Christian M. Fromm, Charles F. Gammie, Roberto García, Olivier Gentaz, C. Goddi, José L. Gómez, Minfeng Gu, Mark Gurwell, Kazuhiro Hada, Ronald Hesper, Luis C. Ho, Paul T. P. Ho, Mareki Honma, Lei Huang, D. H. Hughes, Makoto Inoue, Sara Issaoun, D. J. James, Buell T. Jannuzi, Michaël Janssen, Alejandra Jiménez-Rosales, 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, M. Krämer, C. Krämer, T. P. Krichbaum, Cheng‐Yu Kuo, Tod R. Lauer, Sang-Sung Lee, Yanrong Li, M. Lindqvist, Rocco Lico, Kuo Liu, Elisabetta Liuzzo, Wen-Ping Lo, A. P. Lobanov, C. J. Lonsdale, Ru-Sen Lu, J. Mao, Sera Markoff, Daniel P. Marrone, Alan P. Marscher, I. Martí‐Vidal, Satoki Matsushita, Yosuke Mizuno, Izumi Mizuno, J. M. Moran, Kotaro Moriyama, Monika Mościbrodzka, Cornelia Müller, Alejandro Mus, Hiroshi Nagai, Neil M. Nagar, Ramesh Narayan, Gopal Narayanan, Iniyan Natarajan, R. Neri, A. Noutsos, Hiroki Okino, Héctor Olivares, Tomoaki Oyama, Daniel C. M. Palumbo, Jongho Park, Nimesh Patel, Ue‐Li Pen, Vincent Piétu, R. L. Plambeck, Aleksandar PopStefanija, Ben Prather, Jorge A. Preciado-López, 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, Benjamin R. Ryan, K. L. J. Rygl, David Sánchez-Argüelles, Mahito Sasada, T. Savolainen, F. Peter Schloerb, K. Schüster, Lijing Shao, Zhiqiang Shen, Des Small, Bong Won Sohn, Jason Soohoo, Fumie Tazaki, R. P. J. Tilanus, Michael S. Titus, Pablo Torné, Tyler Trent, Efthalia Traianou, Sascha Trippe, Huib Jan van Langevelde, Daniel R. van Rossum, Jan Wagner, J. F. C. Wardle, D. Ward–Thompson, Jonathan Weintroub, Norbert Wex, Robert Wharton, Maciek Wielgus, George N. Wong, Qingwen Wu, Doosoo Yoon, André Young, Ken Young, Ziri Younsi, Feng Yuan, Ye-Fei Yuan, Shan-Shan Zhao

Bibliographic record

VenuePhysical Review Letters · 2020
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 ChinaFondo Nacional de Desarrollo Científico, Tecnológico y de Innovación TecnológicaInstituto Nazionale di Fisica NucleareComisión Nacional de Investigación Científica y TecnológicaJapan Society for the Promotion of ScienceScience and Technology Facilities CouncilNational Nuclear Security AdministrationToray Science FoundationInstitut Périmètre de physique théoriqueIstituto Nazionale di Fisica NucleareJunta de AndalucíaRecruitment Program of Global ExpertsRussian Science FoundationNational Astronomical Observatory of JapanUniversidad Nacional Autónoma de MéxicoAcademy of FinlandMax-Planck-GesellschaftCentre National de la Recherche ScientifiqueMinistry of Science and Technology, TaiwanNational Natural Science Foundation of ChinaNational Research Foundation of KoreaMinisterio de Ciencia, Innovación y UniversidadesNuclear Safety and Security CommissionOntario Ministry of Research, Innovation and ScienceH2020 European Research CouncilGordon and Betty Moore FoundationMinistero dell’Istruzione, dell’Università e della RicercaGeneralitat ValencianaNatural Sciences and Engineering Research Council of CanadaChina Scholarship CouncilMinistry of Education, Culture, Sports, Science and TechnologyJohn Templeton FoundationEuropean Southern ObservatoryMinisterio de Economía y CompetitividadInstituto de Astrofísica de AndalucíaConsejería de Economía, Innovación, Ciencia y Empleo, Junta de AndalucíaNederlandse Organisatie voor Wetenschappelijk OnderzoekChinese Academy of SciencesAcademia SinicaDepartment of Science and Technology, Ministry of Science and Technology, IndiaDepartment of Science and Technology, Republic of South AfricaMinistero dello Sviluppo EconomicoKorea Astronomy and Space Science InstituteAssociated UniversitiesSpace Telescope Science InstituteInnovation, Science and Economic Development CanadaNational Research FoundationIndonesia Toray Science FoundationDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoConsejo Nacional de Ciencia y TecnologíaConsejo Superior de Investigaciones CientíficasUniversity of ChicagoHorizon 2020 Framework ProgrammeVetenskapsrådetInternational Max Planck Research School for Environmental, Cellular and Molecular MicrobiologySmithsonian InstitutionU.S. Department of EnergyKavli FoundationLeverhulme TrustEuropean CommissionNational Radio Astronomy ObservatoryHarvard UniversityUniversity of ArizonaMassachusetts Institute of TechnologyNational Institutes of Natural SciencesGovernment of CanadaNational Aeronautics and Space AdministrationAlexander von Humboldt-StiftungCompute CanadaNational Science Foundation
KeywordsPhysicsBlack hole (networking)Shadow (psychology)Event horizonRotating black holeMetric (unit)AstrophysicsField (mathematics)Gravitational waveGravitational fieldHorizonClassical mechanicsEvent (particle physics)Astronomy

Abstract

fetched live from OpenAlex

We present measurements of the properties of the central radio source in M87 using Event Horizon Telescope data obtained during the 2017 campaign. We develop and fit geometric crescent models (asymmetric rings with interior brightness depressions) using two independent sampling algorithms that consider distinct representations of the visibility data. We show that the crescent family of models is statistically preferred over other comparably complex geometric models that we explore. We calibrate the geometric model parameters using general relativistic magnetohydrodynamic (GRMHD) models of the emission region and estimate physical properties of the source. We further fit images generated from GRMHD models directly to the data. We compare the derived emission region and black hole parameters from these analyses with those recovered from reconstructed images. There is a remarkable consistency among all methods and data sets. We find that >50% of the total flux at arcsecond scales comes from near the horizon, and that the emission is dramatically suppressed interior to this region by a factor >10, providing direct evidence of the predicted shadow of a black hole. Across all methods, we measure a crescent diameter of 423 as and constrain its fractional width to be <0.5. Associating the crescent feature with the emission surrounding the black hole shadow, we infer an angular gravitational radius of GM/Dc 2 =3.80.4 as. Folding in a distance measurement of -+ 16.8 Mpc 0.7 0.8 gives a black hole mass of = | | M M 6.5 0.2 0.7 10 stat sys 9

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)0.001
metaresearch head score (Gemma)0.004
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.006
Threshold uncertainty score0.012

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.004
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.001
Scholarly communication0.0010.000
Open science0.0000.001
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 head0.011
GPT teacher head0.231
Teacher spread0.221 · 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 designObservational
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".

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Citations330
Published2020
Admission routes2
Has abstractyes

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