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Kim, Jae-Young
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Constraints on black-hole charges with the 2017 EHT observations of M87*

Author(s)
Kocherlakota, PrashantRezzolla, LucianoFalcke, HeinoFromm, Christian M.Kramer, MichaelMizuno, YosukeNathanail, AntoniosOlivares, HectorYounsi, ZiriAkiyama, KazunoriAlberdi, AntxonAlef, WalterAlgaba, Juan CarlosAnantua, RichardAsada, KeiichiAzulay, RebeccaBaczko, Anne-KathrinBall, DavidBalokovic, MislayBarrett, JohnBenson, Bradford A.Bintley, DanBlackburn, LindyBlundell, RaymondBoland, WilfredBouman, Katherine L.Bower, Geoffrey C.Boyce, HopeBremer, MichaelBrinkerink, Christiaan D.Brissenden, RogerBritzen, SilkeBroderick, Avery E.Broguiere, DominiqueBronzwaer, ThomasByun, Do-YoungCarlstrom, John E.Chael, AndrewChan, Chi-kwanChatterjee, ShamiChatterjee, KoushikChen, Ming-TangChen, YongjunChesler, Paul M.Cho, IljeChristian, PierreConway, John E.Cordes, James M.Crawford, Thomas M.Crew, Geoffrey B.Cruz-Osorio, AlejandroCui, YuzhuDavelaar, JordyDe Laurentis, MariafeliciaDeane, RogerDempsey, JessicaDesvignes, GregoryDoeleman, Sheperd S.Eatough, Ralph P.Farah, JosephFish, Vincent L.Fomalont, EdFraga-Encinas, RaquelFriberg, PerFord, H. AlysonFuentes, AntonioGalison, PeterGammie, Charles F.Garcia, RobertoGentaz, OlivierGeorgiev, BorisGoddi, CiriacoGold, RomanGomez, Jose L.Gomez-Ruiz, Arturo, IGu, MinfengGurwell, MarkHada, KazuhiroHaggard, DarylHecht, 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, WuJimenez-Rosales, AlejandraJohnson, Michael D.Jorstad, SvetlanaJung, TaehyunKarami, MansourKaruppusamy, RameshKawashima, TomohisaKeating, Garrett K.Kettenis, MarkKim, Dong-JinKim, Jae-YoungKim, JongsooKim, JunhanKino, MotokiKoay, Jun YiKofuji, YutaroKoch, Patrick M.Koyama, ShokoKramer, CarstenKrichbaum, Thomas P.Kuo, Cheng-YuLauer, Tod R.Lee, Sang-SungLevis, AviadLi, Yan-RongLi, ZhiyuanLindqvist, MichaelLico, RoccoLindahl, GregLiu, JunLiu, KuoLiuzzo, ElisabettaLo, Wen-PingLobanov, Andrei P.Loinard, LaurentLonsdale, ColinLu, Ru-SenMacDonald, Nicholas R.Mao, JirongMarchili, NicolaMarkoff, SeraMarrone, Daniel P.Marscher, Alan P.Marti-Vidal, IvanMatsushita, SatokiMatthews, Lynn D.Medeiros, LiaMenten, Karl M.Mizuno, IzumiMoran, James M.Moriyama, KotaroMoscibrodzka, MonikaMueller, CorneliaMusoke, GibwaMejias, Alejandro MusNagai, HiroshiNagar, Neil M.Nakamura, MasanoriNarayan, RameshNarayanan, GopalNatarajan, IniyanNeilsen, JosephNeri, RobertoNi, ChunchongNoutsos, AristeidisNowak, Michael A.Okino, HirokiOrtiz-Leon, Gisela N.Oyama, TomoakiOzel, FeryalPalumbo, Daniel C. M.Park, JonghoPatel, NimeshPen, Ue-LiPesce, Dominic W.Pietu, VincentPlambeck, RichardPopStefanija, AleksandarPorth, OliverPoetzl, Felix M.Prather, BenPreciado-Lopez, Jorge A.Psaltis, DimitriosPu, Hung-YiRamakrishnan, VenkatesshRao, RamprasadRawlings, Mark G.Raymond, Alexander W.Ricarte, AngeloRipperda, 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, ZhiqiangDes SmallSohn, Bong WonSooHoo, JasonSun, HeTazaki, FumieTetarenko, Alexandra J.Tiede, PaulTilanus, Remo P. J.Titus, MichaelToma, KenjiTorne, PabloTrent, TylerTraianou, EfthaliaTrippe, Saschavan Bemmel, Ilsevan Langevelde, Huib Janvan Rossum, Daniel R.Wagner, JanWard-Thompson, DerekWardle, JohnWeintroub, JonathanWex, NorbertWharton, RobertWielgus, MaciekWong, George N.Wu, QingwenYoon, DoosooYoung, AndreYoung, KenYuan, FengYuan, Ye-FeiZensus, J. AntonZhao, Guang-YaoZhao, Shan-Shan
Issued Date
2021-05
DOI
10.1103/PhysRevD.103.104047
URI
https://scholarworks.unist.ac.kr/handle/201301/83925
Citation
PHYSICAL REVIEW D, v.103, no.10, pp.104047
Abstract
Our understanding of strong gravity near supermassive compact objects has recently improved thanks to the measurements made by the Event Horizon Telescope (EHT). We use here the M87* shadow size to infer constraints on the physical charges of a large variety of nonrotating or rotating black holes. For example, we show that the quality of the measurements is already sufficient to rule out that M87* is a highly charged dilaton black hole. Similarly, when considering black holes with two physical and independent charges, we are able to exclude considerable regions of the space of parameters for the doubly-charged dilaton and the Sen black holes.
Publisher
AMER PHYSICAL SOC
ISSN
2470-0010
Keyword
CALIBRATIONSHADOWSGRAVITYTESTSFIELDPOLARIZATIONASTROPYMASS

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