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Kim, Jae-Young
Observational Astrophysics Lab
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The Event Horizon General Relativistic Magnetohydrodynamic Code Comparison Project

Author(s)
Porth, OliverChatterjee, KoushikNarayan, RameshGammie, Charles F.Mizuno, YosukeAnninos, PeterBaker, John G.Bugli, MatteoChan, Chi-kwanDavelaar, JordyDel Zanna, LucaEtienne, Zachariah B.Fragile, P. ChrisKelly, Bernard J.Liska, MatthewMarkoff, SeraMcKinney, Jonathan C.Mishra, BhupendraNoble, Scott C.Olivares, HectorPrather, BenRezzolla, LucianoRyan, Benjamin R.Stone, James M.Tomei, NiccoloWhite, Christopher J.Younsi, ZiriAkiyama, KazunoriAlberdi, AntxonAlef, WalterAsada, KeiichiAzulay, RebeccaBaczko, Anne-KathrinBall, DavidBalokovic, MislavBarrett, JohnBintley, DanBlackburn, LindyBoland, WilfredBouman, Katherine L.Bower, Geoffrey C.Bremer, MichaelBrinkerink, Christiaan D.Brissenden, RogerBritzen, SilkeBroderick, Avery E.Broguiere, DominiqueBronzwaer, ThomasByun, Do-YoungCarlstrom, John E.Chael, AndrewChatterjee, ShamiChen, Ming-TangChen, YongjunCho, IljeChristian, PierreConway, John E.Cordes, James M.Crew, Geoffrey B.Cui, YuzhuDe Laurentis, MariafeliciaDeane, RogerDempsey, JessicaDesvignes, GregoryDoeleman, Sheperd S.Eatough, Ralph P.Falcke, HeinoFish, Vincent L.Fomalont, EdFraga-Encinas, RaquelFreeman, BillFriberg, PerFromm, Christian M.Gomez, Jose L.Galison, PeterGarcia, RobertoGentaz, OlivierGeorgiev, BorisGoddi, CiriacoGold, RomanGu, MinfengGurwell, MarkHada, KazuhiroHecht, Michael H.Hesper, RonaldHo, Luis C.Ho, PaulHonma, MarekiHuang, Chih-Wei L.Huang, LeiHughes, David H.Ikeda, ShiroInoue, MakotoIssaoun, SaraJames, David J.Jannuzi, Buell T.Janssen, MichaelJeter, BrittonJiang, WuJohnson, Michael D.Jorstad, SvetlanaJung, TaehyunKarami, MansourKaruppusamy, RameshKawashima, TomohisaKeating, Garrett K.Kettenis, MarkKim, Jae-YoungKim, JunhanKim, JongsooKino, MotokiKoay, Jun YiPatrick, M. KochKoyama, ShokoKramer, MichaelKramer, CarstenKrichbaum, Thomas P.Kuo, Cheng-YuLauer, Tod R.Lee, Sang-SungLi, Yan-RongLi, ZhiyuanLindqvist, MichaelLiu, KuoLiuzzo, ElisabettaLo, Wen-PingLobanov, Andrei P.Loinard, LaurentLonsdale, ColinLu, Ru-SenMacDonald, Nicholas R.Mao, JirongMarrone, Daniel P.Marscher, Alan P.Marti-Vidal, IvanMatsushita, SatokiMatthews, Lynn D.Medeiros, LiaMenten, Karl M.Mizuno, IzumiMoran, James M.Moriyama, KotaroMoscibrodzka, MonikaMueller, CorneliaNagai, HiroshiNagar, Neil M.Nakamura, MasanoriNarayanan, GopalNatarajan, IniyanNeri, RobertoNi, ChunchongNoutsos, AristeidisOkino, HirokiOyama, TomoakiOzel, FeryalPalumbo, Daniel C. M.Patel, NimeshPen, Ue-LiPesce, Dominic W.Pietu, VincentPlambeck, RichardPopStefanija, AleksandarPreciado-Lopez, Jorge A.Psaltis, DimitriosPu, Hung-YiRamakrishnan, VenkatesshRao, RamprasadRawlings, Mark G.Raymond, Alexander W.Ripperda, BartRoelofs, FreekRogers, AlanRos, EduardoRose, MelRoshanineshat, ArashRottmann, HelgeRoy, Alan L.Ruszczyk, ChetRygl, Kazi L. J.Sanchez, SalvadorSanchez-Arguelles, DavidSasada, MahitoSavolainen, TuomasSchloerb, F. PeterSchuster, Karl-FriedrichShao, LijingShen, ZhiqiangSmall, DesSohn, Bong WonSooHoo, JasonTazaki, FumieTiede, PaulTilanus, Remo P. J.Titus, MichaelToma, KenjiTorne, PabloTrent, TylerTrippe, SaschaTsuda, Shuichirovan Bemmel, Ilsevan Langevelde, Huib Janvan Rossum, Daniel R.Wagner, JanWardle, JohnWeintroub, JonathanWex, NorbertWharton, RobertWielgus, MaciekWong, George N.Wu, QingwenYoung, KenYoung, AndreYuan, FengYuan, Ye-FeiZensus, J. AntonZhao, GuangyaoZhao, Shan-ShanZhu, Ziyan
Issued Date
2019-08
DOI
10.3847/1538-4365/ab29fd
URI
https://scholarworks.unist.ac.kr/handle/201301/83928
Citation
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, v.243, no.2, pp.26
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.
Publisher
IOP Publishing Ltd
ISSN
0067-0049
Keyword (Author)
black hole physicsmagnetic fieldsmagnetohydrodynamics (MHD)methods: numericalrelativistic processes
Keyword
BLACK-HOLE ACCRETIONADVECTION-DOMINATED ACCRETIONSGR A-ASTERISKGODUNOV-TYPE SCHEMESMAGNETOROTATIONAL INSTABILITYMAGNETIZED ACCRETIONEDDINGTON ACCRETIONGLOBAL SIMULATIONSNUMERICAL SCHEMENEUTRON-STARS

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