The event horizon general relativistic magnetohydrodynamic code comparison project

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dc.contributor.author Porth, Oliver
dc.contributor.author Chatterjee, Koushik
dc.contributor.author Narayan, Ramesh
dc.contributor.author Gammie, Charles F.
dc.contributor.author Mizuno, Yosuke
dc.contributor.author Anninos, Peter
dc.contributor.author Baker, John G.
dc.contributor.author Bugli, Matteo
dc.contributor.author Chan, Chi-kwan
dc.contributor.author Davelaar, Jordy
dc.contributor.author Del Zanna, Luca
dc.contributor.author Etienne, Zachariah B.
dc.contributor.author Fragile, P. Chris
dc.contributor.author Kelly, Bernard J.
dc.contributor.author Liska, Matthew
dc.contributor.author Markoff, Sera
dc.contributor.author McKinney, Jonathan C.
dc.contributor.author Mishra, Bhupendra
dc.contributor.author Noble, Scott C.
dc.contributor.author Olivares, Hector
dc.contributor.author Prather, Ben
dc.contributor.author Rezzolla, Luciano
dc.contributor.author Ryan, Benjamin R.
dc.contributor.author Stone, James M.
dc.contributor.author Tomei, Niccolo
dc.contributor.author White, Christopher J.
dc.contributor.author Akiyama, Kazunori
dc.contributor.author Alberdi, Antxon
dc.contributor.author Alef, Walter
dc.contributor.author Asada, Keiichi
dc.contributor.author Azulay, Rebecca
dc.contributor.author Baczko, Anne-Kathrin
dc.contributor.author Ball, David
dc.contributor.author Balokovic, Mislav
dc.contributor.author Barrett, John
dc.contributor.author Bintley, Dan
dc.contributor.author Blackburn, Lindy
dc.contributor.author Boland, Wilfred
dc.contributor.author Bouman, Katherine L.
dc.contributor.author Bower, Geoffrey C.
dc.contributor.author Bremer, Michael
dc.contributor.author Brinkerink, Christiaan D.
dc.contributor.author Brissenden, Roger
dc.contributor.author Britzen, Silke
dc.contributor.author Broderick, Avery E.
dc.contributor.author Broguiere, Dominique
dc.contributor.author Bronzwaer, Thomas
dc.contributor.author Byun, Do-Young
dc.contributor.author Carlstrom, John E.
dc.contributor.author Chael, Andrew
dc.contributor.author Chatterjee, Shami
dc.contributor.author Chen, Ming-Tang
dc.contributor.author Chen, Yongjun
dc.contributor.author Cho, Ilje
dc.contributor.author Christian, Pierre
dc.contributor.author Conway, John E.
dc.contributor.author Cordes, James M.
dc.contributor.author Crew, Geoffrey B.
dc.contributor.author Cui, Yuzhu
dc.contributor.author De Laurentis, Mariafelicia
dc.contributor.author Deane, Roger
dc.contributor.author Dempsey, Jessica
dc.contributor.author Desvignes, Gregory
dc.contributor.author Doeleman, Sheperd S.
dc.contributor.author Eatough, Ralph P.
dc.contributor.author Falcke, Heino
dc.contributor.author Fish, Vincent L.
dc.contributor.author Fomalont, Ed
dc.contributor.author Fraga-Encinas, Raquel
dc.contributor.author Freeman, William T.
dc.contributor.author Friberg, Per
dc.contributor.author Fromm, Christian M.
dc.contributor.author Gomez, Jose L.
dc.contributor.author Galison, Peter
dc.contributor.author Gammie, Charles F.
dc.contributor.author Garcia, Roberto
dc.contributor.author Gentaz, Olivier
dc.contributor.author Georgiev, Boris
dc.contributor.author Goddi, Ciriaco
dc.contributor.author Gold, Roman
dc.contributor.author Gu, Minfeng
dc.contributor.author Gurwell, Mark
dc.contributor.author Hada, Kazuhiro
dc.contributor.author Hecht, Michael H.
dc.contributor.author Hesper, Ronald
dc.contributor.author Ho, Luis C.
dc.contributor.author Ho, Paul
dc.contributor.author Honma, Mareki
dc.contributor.author Huang, Chih-Wei L.
dc.contributor.author Huang, Lei
dc.contributor.author Hughes, David H.
dc.contributor.author Ikeda, Shiro
dc.contributor.author Inoue, Makoto
dc.contributor.author Issaoun, Sara
dc.contributor.author James, David J.
dc.contributor.author Jannuzi, Buell T.
dc.contributor.author Janssen, Michael
dc.contributor.author Jeter, Britton
dc.contributor.author Jiang, Wu
dc.contributor.author Johnson, Michael D.
dc.contributor.author Jorstad, Svetlana
dc.contributor.author Jung, Taehyun
dc.contributor.author Karami, Mansour
dc.contributor.author Karuppusamy, Ramesh
dc.contributor.author Kawashima, Tomohisa
dc.contributor.author Keating, Garrett K.
dc.contributor.author Kettenis, Mark
dc.contributor.author Kim, Jae-Young
dc.contributor.author Kim, Junhan
dc.contributor.author Kim, Jongsoo
dc.contributor.author Kino, Motoki
dc.contributor.author Koay, Jun Yi
dc.contributor.author Koch, Patrick M.
dc.contributor.author Koyama, Shoko
dc.contributor.author Kramer, Michael
dc.contributor.author Kramer, Carsten
dc.contributor.author Krichbaum, Thomas P.
dc.contributor.author Kuo, Cheng-Yu
dc.contributor.author Lauer, Tod R.
dc.contributor.author Lee, Sang-Sung
dc.contributor.author Li, Yan-Rong
dc.contributor.author Li, Zhiyuan
dc.contributor.author Lindqvist, Michael
dc.contributor.author Liu, Kuo
dc.contributor.author Liuzzo, Elisabetta
dc.contributor.author Lo, Wen-Ping
dc.contributor.author Lobanov, Andrei P.
dc.contributor.author Loinard, Laurent
dc.contributor.author Lonsdale, Colin
dc.contributor.author Lu, Ru-Sen
dc.contributor.author MacDonald, Nicholas R.
dc.contributor.author Mao, Jirong
dc.contributor.author Marrone, Daniel P.
dc.contributor.author Marscher, Alan P.
dc.contributor.author Marti-Vidal, Ivan
dc.contributor.author Matsushita, Satoki
dc.contributor.author Matthews, Lynn D.
dc.contributor.author Medeiros, Lia
dc.contributor.author Menten, Karl M.
dc.contributor.author Mizuno, Izumi
dc.contributor.author Moran, James M.
dc.contributor.author Moriyama, Kotaro
dc.contributor.author Moscibrodzka, Monika
dc.contributor.author Muller, Cornelia
dc.contributor.author Nagai, Hiroshi
dc.contributor.author Nagar, Neil M.
dc.contributor.author Nakamura, Masanori
dc.contributor.author Narayanan, Gopal
dc.contributor.author Natarajan, Iniyan
dc.contributor.author Neri, Roberto
dc.contributor.author Ni, Chunchong
dc.contributor.author Noutsos, Aristeidis
dc.contributor.author Okino, Hiroki
dc.contributor.author Oyama, Tomoaki
dc.contributor.author Ozel, Feryal
dc.contributor.author Palumbo, Daniel C.M.
dc.contributor.author Patel, Nimesh
dc.contributor.author Pen, Ue-Li
dc.contributor.author Pesce, Dominic W.
dc.contributor.author Pietu, Vincent
dc.contributor.author Plambeck, Richard
dc.contributor.author PopStefanija, Aleksandar
dc.contributor.author Preciado-Lopez, Jorge A.
dc.contributor.author Psaltis, Dimitrios
dc.contributor.author Pu, Hung-Yi
dc.contributor.author Ramakrishnan, Venkatessh
dc.contributor.author Rao, Ramprasad
dc.contributor.author Rawlings, Mark G.
dc.contributor.author Raymond, Alexander W.
dc.contributor.author Ripperda, Bart
dc.contributor.author Roelofs, Freek
dc.contributor.author Rogers, Alan
dc.contributor.author Ros, Eduardo
dc.contributor.author Rose, Mel
dc.contributor.author Roshanineshat, Arash
dc.contributor.author Rottmann, Helge
dc.contributor.author Roy, Alan L.
dc.contributor.author Ruszczyk, Chet
dc.contributor.author Rygl, Kazi L.J.
dc.contributor.author Sanchez, Salvador
dc.contributor.author Sanchez-Arguelles, David
dc.contributor.author Sasada, Mahito
dc.contributor.author Savolainen, Tuomas
dc.contributor.author Schloerb, F. Peter
dc.contributor.author Schuster, Karl-Friedrich
dc.contributor.author Shao, Lijing
dc.contributor.author Shen, Zhiqiang
dc.contributor.author Small, Des
dc.contributor.author Sohn, Bong Won
dc.contributor.author SooHoo, Jason
dc.contributor.author Tazaki, Fumie
dc.contributor.author Tiede, Paul
dc.contributor.author Tilanus, Remo P.J.
dc.contributor.author Titus, Michael
dc.contributor.author Toma, Kenji
dc.contributor.author Torne, Pablo
dc.contributor.author Trent, Tyler
dc.contributor.author Trippe, Sascha
dc.contributor.author Tsuda, Shuichiro
dc.contributor.author Van Bemmel, Ilse
dc.contributor.author Van Langevelde, Huib Jan
dc.contributor.author Van Rossum, Daniel R.
dc.contributor.author Wagner, Jan
dc.contributor.author Wardle, John
dc.contributor.author Weintroub, Jonathan
dc.contributor.author Wex, Norbert
dc.contributor.author Wharton, Robert
dc.contributor.author Wielgus, Maciek
dc.contributor.author Wong, George N.
dc.contributor.author Wu, Qingwen
dc.contributor.author Young, Ken
dc.contributor.author Young, Andre
dc.contributor.author Yuan, Feng
dc.contributor.author Yuan, Ye-Fei
dc.contributor.author Zensus, J. Anton
dc.contributor.author Zhao, Guangyao
dc.contributor.author Zhao, Shan-Shan
dc.contributor.author Zhu, Ziyan
dc.date.accessioned 2020-12-03T05:05:03Z
dc.date.available 2020-12-03T05:05:03Z
dc.date.issued 2019-08
dc.description.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. en_ZA
dc.description.department Physics en_ZA
dc.description.librarian am2020 en_ZA
dc.description.sponsorship R.N. thanks the National Science Foundation (NSF; grants OISE-1743747, AST-1816420) and acknowledges computational support from the NSF via XSEDE resources (grant TG-AST080026N). L.D.Z. acknowledges support from the PRIN-MIUR project Multi-scale Simulations of High-Energy Astrophysical Plasmas (Prot. 2015L5EE2Y) and from the INFN—TEONGRAV initiative. C.J.W. made use of the Extreme Science and Engineering Discovery Environment (XSEDE) Comet at the San Diego Supercomputer Center through allocation AST170012. The H-AMR high-resolution simulation was made possible by NSF PRAC award Nos. 1615281 and OAC-1811605 at the Blue Waters sustainedpetascale computing project and supported in part under grant No. NSF PHY-1125915 (PI A. Tchekhovskoy). K.C. and S.M. are supported by the Netherlands Organization for Scientific Research (NWO) VICI grant (No. 639.043.513); M.L. is supported by the NWO Spinoza Prize (PI M.B.M. van der Klis). The HARM-Noble simulations were made possible by NSF PRAC award No. NSF OAC-1515969, OAC-1811228 at the Blue Waters sustained-petascale computing project, and supported in part under grant No. NSF PHY-1125915. The BHAC CKS-GRMHD simulations were performed on the Dutch National Supercomputing cluster Cartesius and are funded by the NWO computing grant 16431. S.C.N. was supported by an appointment to the NASA Postdoctoral Program at the Goddard Space Flight Center administered by USRA through a contract with NASA. Y.M., H.O., O.P., and L.R. acknowledge support from the ERC synergy grant “BlackHoleCam: Imaging the Event Horizon of Black Holes” (grant No. 610058). M.B. acknowledges support from the European Research Council (grant No. 715368—MagBURST) and from the Gauss Centre for Supercomputing e.V. (www. Gauss-centre.eu) for funding this project by providing computing time on the GCS Supercomputer SuperMUC at Leibniz Supercomputing Centre (www.lrz.de). P.C.F. was supported by NSF grant AST-1616185 and used resources from the Extreme Science and Engineering Discovery Environment (XSEDE), which is supported by NSF grant No. ACI-1548562. Work by P.A. was performed in part under the auspices of the US Department of Energy by Lawrence Livermore National Laboratory under contract DE-AC52- 07NA27344. The authors of the present paper further thank the following organizations and programs: the Academy of Finland (projects 274477, 284495, 312496); the Advanced European Network of E-infrastructures for Astronomy with the SKA (AENEAS) project, supported by the European Commission Framework Programme Horizon 2020 Research and Innovation action under grant agreement 731016; the Alexander von Humboldt Stiftung; the Black Hole Initiative at Harvard University, through a grant (60477) from the John Templeton Foundation; the China Scholarship Council; Comisión Nacional de Investigación Científica y Tecnológica (CONICYT, Chile, via PIA ACT172033, Fondecyt 1171506, BASAL AFB-170002, ALMA-conicyt 31140007); Consejo Nacional de Ciencia y Tecnología (CONACYT, Mexico, projects 104497, 275201, 279006, 281692); the Delaney Family via the Delaney Family John A. Wheeler Chair at Perimeter Institute; Dirección General de Asuntos del Personal Académico-Universidad Nacional Autónoma de México (DGAPA-UNAM, project IN112417); the European Research Council Synergy Grant “BlackHoleCam: Imaging the Event Horizon of Black Holes” (grant 610058); the Generalitat Valenciana postdoctoral grant APOSTD/2018/177; the Gordon and Betty Moore Foundation (grants GBMF-3561, GBMF-5278); the Istituto Nazionale di Fisica Nucleare (INFN) sezione di Napoli, iniziative specifiche TEONGRAV; the International Max Planck Research School for Astronomy and Astrophysics at the Universities of Bonn and Cologne; the Jansky Fellowship program of the National Radio Astronomy Observatory (NRAO); the Japanese Government (Monbukagakusho: MEXT) Scholarship; the Japan Society for the Promotion of Science (JSPS) Grant-in-Aid for JSPS Research Fellowship (JP17J08829); the Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS, grants QYZDJ-SSW-SLH057, QYZDJ-SSW-SYS008); the Leverhulme Trust Early Career Research Fellowship; the Max-Planck-Gesellschaft (MPG); the Max Planck Partner Group of the MPG and the CAS; the MEXT/JSPS KAKENHI (grants 18KK0090, JP18K13594, JP18K03656, JP18H03721, 18K03709, 18H01245, 25120007); the MIT International Science and Technology Initiatives (MISTI) Funds; the Ministry of Science and Technology (MOST) of Taiwan (105-2112-M- 001-025-MY3, 106-2112-M-001-011, 106-2119-M-001-027, 107-2119-M-001-017, 107-2119-M-001-020, and 107-2119-M- 110-005); the National Aeronautics and Space Administration (NASA, Fermi Guest Investigator grant 80NSSC17K0649); the National Institute of Natural Sciences (NINS) of Japan; the National Key Research and Development Program of China (grant 2016YFA0400704, 2016YFA0400702); the National Science Foundation (NSF, grants AST-0096454, AST-0352953, AST-0521233, AST-0705062, AST-0905844, AST-0922984, AST-1126433, AST-1140030, DGE-1144085, AST-1207704, AST-1207730, AST-1207752, MRI-1228509, OPP-1248097, AST-1310896, AST-1312651, AST-1337663, AST-1440254, AST-1555365, AST-1715061, AST-1615796, AST-1716327, OISE-1743747, AST-1816420); the Natural Science Foundation of China (grants 11573051, 11633006, 11650110427, 10625314, 11721303, 11725312); the Natural Sciences and Engineering Research Council of Canada (NSERC, including a Discovery Grant and the NSERC Alexander Graham Bell Canada Graduate Scholarships Doctoral Program); the National Youth Thousand Talents Program of China; the National Research Foundation of Korea (the Global PhD Fellowship Grant: grants NRF- 2015H1A2A1033752, 2015-R1D1A1A01056807, the Korea Research Fellowship Program: NRF-2015H1D3A1066561); the Netherlands Organization for Scientific Research (NWO) VICI award (grant 639.043.513) and Spinoza Prize SPI 78-409; the New Scientific Frontiers with Precision Radio Interferometry Fellowship awarded by the South African Radio Astronomy Observatory (SARAO), which is a facility of the National Research Foundation (NRF), an agency of the Department of Science and Technology (DST) of South Africa; the Onsala Space Observatory (OSO) national infrastructure, for the provisioning of its facilities/observational support (OSO receives funding through the Swedish Research Council under grant 2017-00648); the Perimeter Institute for Theoretical Physics (research at Perimeter Institute is supported by the Government of Canada through the Department of Innovation, Science and Economic Development, and by the Province of Ontario through the Ministry of Research, Innovation and Science); the Russian Science Foundation (grant 17-12-01029); the Spanish Ministerio de Economía y Competitividad (grants AYA2015-63939-C2-1-P, AYA2016-80889-P); the State Agency for Research of the Spanish MCIU through the “Center of Excellence Severo Ochoa” award for the Instituto de Astrofísica de Andalucía (SEV-2017-0709); the Toray Science Foundation; the US Department of Energy (USDOE) through the Los Alamos National Laboratory (operated by Triad National Security, LLC, for the National Nuclear Security Administration of the USDOE (Contract 89233218CNA000001)); the Italian Ministero dell’Istruzione Università e Ricerca through the grant Progetti Premiali 2012-iALMA (CUP C52I13000140001); the European Union’s Horizon 2020 research and innovation programme under grant agreement No. 730562 RadioNet; ALMA North America Development Fund; the Academia Sinica; and Chandra TM6-17006X. This work used the Extreme Science and Engineering Discovery Environment (XSEDE), supported by NSF grant ACI-1548562, and CyVerse, supported by NSF grants DBI-0735191, DBI-1265383, and DBI-1743442. XSEDE Stampede2 resource at TACC was allocated through TG-AST170024 and TG-AST080026N. XSEDE JetStream resource at PTI and TACC was allocated through AST170028. The simulations were performed in part on the SuperMUC cluster at the LRZ in Garching, on the LOEWE cluster in CSC in Frankfurt, and on the HazelHen cluster at the HLRS in Stuttgart. This research was enabled in part by support provided by Compute Ontario (http://computeontario.ca), Calcul Quebec (http://www.calculquebec.ca), and Compute Canada (http:// www.computecanada.ca). en_ZA
dc.description.uri http://iopscience.iop.org/0067-0049 en_ZA
dc.identifier.citation Porth, O., Chatterjee, K., Narayan, R. et al. 2019, 'The event horizon general relativistic magnetohydrodynamic code comparison project', Astrophysical Journal Supplement, vol. 243, no. 26, pp. 1-40. en_ZA
dc.identifier.issn 0067-0049 (print)
dc.identifier.issn 1538-4365 (online)
dc.identifier.other 10.3847/1538-4365/ab29fd
dc.identifier.uri http://hdl.handle.net/2263/77248
dc.language.iso en en_ZA
dc.publisher IOP Publishing en_ZA
dc.rights © 2019. The American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. en_ZA
dc.subject Black hole physics en_ZA
dc.subject Magnetic fields en_ZA
dc.subject Magnetohydrodynamics (MHD) en_ZA
dc.subject Methods: numerical en_ZA
dc.subject Relativistic processes en_ZA
dc.subject Event Horizon Telescope (EHT) en_ZA
dc.subject General relativistic magnetohydrodynamics (GRMHD) en_ZA
dc.title The event horizon general relativistic magnetohydrodynamic code comparison project en_ZA
dc.type Article en_ZA


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