The Event Horizon General Relativistic Magnetohydrodynamic Code Comparison Project

doi:10.3847/1538-4365/ab29fd

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	The Event Horizon General Relativistic Magnetohydrodynamic Code Comparison Project
	Porth,Oliver 1,2; Chatterjee,Koushik 1; Narayan,Ramesh 3,4; Gammie,Charles F.5; Mizuno,Yosuke 2; Anninos,Peter 6; Baker,John G.7,8; Bugli,Matteo 9; Chan,Chi-kwan 10,11; Davelaar,Jordy 12
刊名	ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
	2019-08-01
卷号	243 期号:2 页码:40
关键词	black hole physics magnetic fields magnetohydrodynamics (MHD) methods: numerical relativistic processes
ISSN号	0067-0049
DOI	10.3847/1538-4365/ab29fd
产权排序	第89完成单位
文献子类	Article
英文摘要	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.
学科主题	天文学 ; 天体物理学 ; 高能天体物理学
URL标识	查看原文
出版地	TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
资助项目	National Science Foundation (NSF)[OISE-1743747] ; National Science Foundation (NSF)[AST-1816420] ; National Science Foundation (NSF)[AST-0096454] ; National Science Foundation (NSF)[AST-0352953] ; National Science Foundation (NSF)[AST-0521233] ; National Science Foundation (NSF)[AST-0705062] ; National Science Foundation (NSF)[AST-0905844] ; National Science Foundation (NSF)[AST-0922984] ; National Science Foundation (NSF)[AST-1126433] ; National Science Foundation (NSF)[AST-1140030] ; National Science Foundation (NSF)[DGE-1144085] ; NSF via XSEDE resources[TG-AST080026N] ; PRIN-MIUR project Multi-scale Simulations of High-Energy Astrophysical Plasmas[2015L5EE2Y] ; INFN-TEONGRAV initiative ; NSF PRAC award at the Blue Waters sustained-petascale computing project[1615281] ; NSF PRAC award at the Blue Waters sustained-petascale computing project[OAC-1811605] ; NSF PRAC award at the Blue Waters sustained-petascale computing project[NSF OAC-1515969] ; NSF PRAC award at the Blue Waters sustained-petascale computing project[OAC-1811228] ; Netherlands Organization for Scientific Research (NWO) VICI grant[639.043.513] ; NWO computing grant[16431] ; ERC synergy grant "BlackHoleCam: Imaging the Event Horizon of Black Holes"[610058] ; European Research Council[715368-MagBURST] ; Gauss Centre for Supercomputing e.V ; NSF[AST-1616185] ; NSF[ACI-1548562] ; NSF[DBI-0735191] ; NSF[DBI-1265383] ; NSF[DBI-1743442] ; US Department of Energy by Lawrence Livermore National Laboratory[DE-AC52-07NA27344] ; Academy of Finland[274477] ; Academy of Finland[284495] ; Academy of Finland[312496] ; European Commission Framework Programme Horizon 2020 Research and Innovation action[731016] ; John Templeton Foundation[60477] ; Comision Nacional de Investigacion Cientifica y Tecnologica (CONICYT, Chile)[PIA ACT172033] ; Comision Nacional de Investigacion Cientifica y Tecnologica (CONICYT, Chile)[Fondecyt 1171506] ; Comision Nacional de Investigacion Cientifica y Tecnologica (CONICYT, Chile)[BASAL AFB-170002] ; Comision Nacional de Investigacion Cientifica y Tecnologica (CONICYT, Chile)[ALMA-conicyt 31140007] ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[104497] ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[275201] ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[279006] ; Consejo Nacional de Ciencia y Tecnologia (CONACYT, Mexico)[281692] ; Direccion General de Asuntos del Personal Academico-Universidad Nacional Autonoma de Mexico (DGAPA-UNAM)[IN112417] ; European Research Council Synergy Grant "BlackHoleCam: Imaging the Event Horizon of Black Holes"[610058] ; Generalitat Valenciana[APOSTD/2018/177] ; Gordon and Betty Moore Foundation[GBMF-3561] ; Gordon and Betty Moore Foundation[GBMF-5278] ; Jansky Fellowship program of the National Radio Astronomy Observatory (NRAO) ; Japanese Government (Monbukagakusho: MEXT) Scholarship ; Japan Society for the Promotion of Science (JSPS)[JP17J08829] ; Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS)[QYZDJ-SSW-SLH057] ; Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS)[QYZDJ-SSW-SYS008] ; Leverhulme Trust Early Career Research Fellowship ; MEXT/JSPS KAKENHI[18KK0090] ; MEXT/JSPS KAKENHI[JP18K13594] ; MEXT/JSPS KAKENHI[JP18K03656] ; MEXT/JSPS KAKENHI[JP18H03721] ; MEXT/JSPS KAKENHI[18K03709] ; MEXT/JSPS KAKENHI[18H01245] ; MEXT/JSPS KAKENHI[25120007] ; MIT International Science and Technology Initiatives (MISTI) Funds ; Ministry of Science and Technology (MOST) of Taiwan[105-2112-M-001-025-MY3] ; Ministry of Science and Technology (MOST) of Taiwan[106-2112-M-001-011] ; Ministry of Science and Technology (MOST) of Taiwan[106-2119-M-001-027] ; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-001-017] ; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-001-020] ; Ministry of Science and Technology (MOST) of Taiwan[107-2119-M-110-005] ; National Aeronautics and Space Administration (NASA)[80NSSC17K0649] ; National Key Research and Development Program of China[2016YFA0400704] ; National Key Research and Development Program of China[2016YFA0400702] ; Natural Science Foundation of China[11573051] ; Natural Science Foundation of China[11633006] ; Natural Science Foundation of China[11650110427] ; Natural Science Foundation of China[10625314] ; Natural Science Foundation of China[11721303] ; Natural Science Foundation of China[11725312] ; National Research Foundation of Korea[NRF-2015H1A2A1033752] ; National Research Foundation of Korea[2015-R1D1A1A01056807] ; National Research Foundation of Korea[NRF-2015H1D3A1066561] ; Netherlands Organization for Scientific Research (NWO) VICI award[639.043.513] ; Spinoza Prize[SPI 78-409] ; South African Radio Astronomy Observatory (SARAO) ; Swedish Research Council[2017-00648] ; Government of Canada through the Department of Innovation, Science and Economic Development ; Province of Ontario through the Ministry of Research, Innovation and Science ; Russian Science Foundation[17-12-01029] ; Spanish Ministerio de Economia y Competitividad[AYA2015-63939-C2-1-P] ; Spanish Ministerio de Economia y Competitividad[AYA2016-80889-P] ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award[SEV-2017-0709] ; USDOE[89233218CNA000001] ; Italian Ministero dell'Istruzione Universita e Ricerca through the grant Progetti Premiali 2012-iALMA[CUP C52I13000140001] ; European Union's Horizon 2020 research and innovation programme[730562 RadioNet] ; Chandra[TM6-17006X] ; CyVerse ; Compute Ontario ; Calcul Quebec ; Compute Canada ; NWO Spinoza Prize ; [NSF PHY-1125915] ; [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]
WOS关键词	BLACK-HOLE ACCRETION ; ADVECTION-DOMINATED ACCRETION ; SGR A-ASTERISK ; GODUNOV-TYPE SCHEMES ; MAGNETOROTATIONAL INSTABILITY ; MAGNETIZED ACCRETION ; EDDINGTON ACCRETION ; GLOBAL SIMULATIONS ; NUMERICAL SCHEME ; NEUTRON-STARS
WOS研究方向	Astronomy & Astrophysics
语种	英语
出版者	IOP PUBLISHING LTD
WOS记录号	WOS:000478621800002
资助机构	National Science Foundation (NSF)[OISE-1743747, AST-1816420, AST-0096454, AST-0352953, AST-0521233, AST-0705062, AST-0905844, AST-0922984, AST-1126433, AST-1140030, DGE-1144085] ; NSF via XSEDE resources[TG-AST080026N] ; PRIN-MIUR project Multi-scale Simulations of High-Energy Astrophysical Plasmas[2015L5EE2Y] ; INFN-TEONGRAV initiative ; NSF PRAC award at the Blue Waters sustained-petascale computing project[1615281, OAC-1811605, NSF OAC-1515969, OAC-1811228] ; Netherlands Organization for Scientific Research (NWO) VICI grant[639.043.513] ; NWO computing grant[16431] ; ERC synergy grant "BlackHoleCam: Imaging the Event Horizon of Black Holes"[610058] ; European Research Council[715368-MagBURST] ; Gauss Centre for Supercomputing e.V ; NSF[AST-1616185, ACI-1548562, DBI-0735191, DBI-1265383, DBI-1743442] ; US Department of Energy by Lawrence Livermore National Laboratory[DE-AC52-07NA27344] ; Academy of Finland[274477, 284495, 312496] ; European Commission Framework Programme Horizon 2020 Research and Innovation action[731016] ; John Templeton Foundation[60477] ; Comision Nacional de Investigacion Cientifica y Tecnologica (CONICYT, Chile)[PIA ACT172033, Fondecyt 1171506, BASAL AFB-170002, ALMA-conicyt 31140007, 104497, 275201, 279006, 281692] ; Direccion General de Asuntos del Personal Academico-Universidad Nacional Autonoma de Mexico (DGAPA-UNAM)[IN112417] ; European Research Council Synergy Grant "BlackHoleCam: Imaging the Event Horizon of Black Holes"[610058] ; Generalitat Valenciana[APOSTD/2018/177] ; Gordon and Betty Moore Foundation[GBMF-3561, GBMF-5278] ; Jansky Fellowship program of the National Radio Astronomy Observatory (NRAO) ; Japanese Government (Monbukagakusho: MEXT) Scholarship ; Japan Society for the Promotion of Science (JSPS)[JP17J08829] ; Key Research Program of Frontier Sciences, Chinese Academy of Sciences (CAS)[QYZDJ-SSW-SLH057, QYZDJ-SSW-SYS008] ; Leverhulme Trust Early Career Research Fellowship ; MEXT/JSPS KAKENHI[18KK0090, JP18K13594, JP18K03656, JP18H03721, 18K03709, 18H01245, 25120007] ; MIT International Science and Technology Initiatives (MISTI) Funds ; 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, 107-2119-M-110-005] ; National Aeronautics and Space Administration (NASA)[80NSSC17K0649] ; National Key Research and Development Program of China[2016YFA0400704, 2016YFA0400702] ; Natural Science Foundation of China[11573051, 11633006, 11650110427, 10625314, 11721303, 11725312] ; National Research Foundation of Korea[NRF-2015H1A2A1033752, 2015-R1D1A1A01056807, NRF-2015H1D3A1066561] ; Netherlands Organization for Scientific Research (NWO) VICI award[639.043.513] ; Spinoza Prize[SPI 78-409] ; South African Radio Astronomy Observatory (SARAO) ; Swedish Research Council[2017-00648] ; Government of Canada through the Department of Innovation, Science and Economic Development ; Province of Ontario through the Ministry of Research, Innovation and Science ; Russian Science Foundation[17-12-01029] ; Spanish Ministerio de Economia y Competitividad[AYA2015-63939-C2-1-P, AYA2016-80889-P] ; State Agency for Research of the Spanish MCIU through the "Center of Excellence Severo Ochoa" award[SEV-2017-0709] ; USDOE[89233218CNA000001] ; Italian Ministero dell'Istruzione Universita e Ricerca through the grant Progetti Premiali 2012-iALMA[CUP C52I13000140001] ; European Union's Horizon 2020 research and innovation programme[730562 RadioNet] ; Chandra[TM6-17006X] ; CyVerse ; Compute Ontario ; Calcul Quebec ; Compute Canada ; NWO Spinoza Prize ; [NSF PHY-1125915] ; [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]
内容类型	期刊论文
源URL	[http://ir.ynao.ac.cn/handle/114a53/20845]
专题	云南天文台_丽江天文观测站（南方基地）云南天文台_中国科学院天体结构与演化重点实验室
作者单位	1.Anton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, 1098 XH, Amsterdam, The Netherlands; o.porth@uva.nl 2.Institut für Theoretische Physik, Goethe-Universit?t Frankfurt, Max-von-Laue-Stra?e 1, D-60438 Frankfurt am Main, Germany 3.Center for Astrophysics∣Harvard & Smithsonian, 60 Garden Street, Cambridge, MA 02138, USA 4.Black Hole Initiative at Harvard University, 20 Garden Street, Cambridge, MA 02138, USA 5.Department of Astronomy and Department of Physics, University of Illinois, Urbana, IL 61801, USA 6.Lawrence Livermore National Laboratory, Livermore, CA 94550, USA 7.Gravitational Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA 8.Joint Space-Science Institute, University of Maryland, College Park, MD 20742, USA 9.IRFU/Département d’Astrophysique, Laboratoire AIM, CEA/DRF-CNRS-Université Paris Diderot, CEA-Saclay F-91191, France 10.Steward Observatory and Department of Astronomy, University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721, USA
推荐引用方式 GB/T 7714	Porth,Oliver,Chatterjee,Koushik,Narayan,Ramesh,et al. The Event Horizon General Relativistic Magnetohydrodynamic Code Comparison Project[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2019,243(2):40.
APA	Porth,Oliver.,Chatterjee,Koushik.,Narayan,Ramesh.,Gammie,Charles F..,Mizuno,Yosuke.,...&Zhu,Ziyan.(2019).The Event Horizon General Relativistic Magnetohydrodynamic Code Comparison Project.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,243(2),40.
MLA	Porth,Oliver,et al."The Event Horizon General Relativistic Magnetohydrodynamic Code Comparison Project".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 243.2(2019):40.