Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A
| dc.contributor.author | Vagnozzi, Sunny | |
| dc.contributor.author | Roy, Rittick | |
| dc.contributor.author | Tsai, Yu-Dai | |
| dc.contributor.author | Visinelli, Luca | |
| dc.contributor.author | Afrin, Misba | |
| dc.contributor.author | Allahyari, Alireza | |
| dc.contributor.author | Bambi, Cosimo | |
| dc.date.accessioned | 2026-02-06T18:47:45Z | |
| dc.date.issued | 2023 | |
| dc.department | Doğu Akdeniz Üniversitesi | |
| dc.description.abstract | Horizon-scale images of black holes (BHs) and their shadows have opened an unprecedented window onto tests of gravity and fundamental physics in the strong-field regime. We consider a wide range of well-motivated deviations from classical general relativity (GR) BH solutions, and constrain them using the Event Horizon Telescope (EHT) observations of Sagittarius A * | |
| dc.description.sponsorship | Isaac Newton Trust; Kavli Foundation; Foundation Blanceflor Boncompagni Ludovisi, ne Bildt; Shanghai Government Scholarship (SGS); U.S. National Science Foundation (NSF) Theoretical Physics Program [PHY-1915005]; NSF [PHY-1748958]; DST-INSPIRE Fellowship, Department of Science and Technology, Government of India; SERB-DST [CRG/2021/005771]; United States-India Educational Foundation (USIEF) through a Fulbright-Nehru Postdoctoral Research Fellowship [2847/FNPDR/2022]; National Research Foundation of South Africa (NRF); National Natural Science Foundation of China (NSFC) [11973019]; Natural Science Foundation of Shanghai [22ZR1403400]; Shanghai Municipal Education Commission [2019-01-07-00-07-E00035]; Fudan University [JIH1512604] | |
| dc.description.sponsorship | We thank Richard Brito, Yifan Chen, and Naoki Tsukamoto for useful discussions. S V was partially supported by the Isaac Newton Trust and the Kavli Foundation through a Newton-Kavli Fellowship, and by a grant from the Foundation Blanceflor Boncompagni Ludovisi, nee Bildt. R R is supported by the Shanghai Government Scholarship (SGS). Y-D T is supported by U.S. National Science Foundation (NSF) Theoretical Physics Program, Grant PHY-1915005, and also in part by the NSF under Grant No. NSF PHY-1748958. M A is supported by a DST-INSPIRE Fellowship, Department of Science and Technology, Government of India. S G G is supported by SERB-DST through Project No. CRG/2021/005771. R K W acknowledges support from the United States-India Educational Foundation (USIEF) through a Fulbright-Nehru Postdoctoral Research Fellowship (Award 2847/FNPDR/2022), and from the University of KwaZulu-Natal and Prof. Sunil Maharaj through a postdoctoral fellowship of the National Research Foundation of South Africa (NRF). A OE thanks Prof. Durmus Ali Demir for hospitality at Sabanci University while this work was being conducted. A OE acknowledges the contribution of the COST Action CA18108-Quantum gravity phenomenology in the multi-messenger approach (QG-MM). C B is supported by the National Natural Science Foundation of China (NSFC) through Grant No. 11973019, the Natural Science Foundation of Shanghai through Grant No. 22ZR1403400, the Shanghai Municipal Education Commission through Grant No. 2019-01-07-00-07-E00035, and Fudan University through Grant No. JIH1512604. | |
| dc.identifier.doi | 10.1088/1361-6382/acd97b | |
| dc.identifier.issn | 0264-9381 | |
| dc.identifier.issn | 1361-6382 | |
| dc.identifier.issue | 16 | |
| dc.identifier.orcid | 0000-0002-4553-2436 | |
| dc.identifier.orcid | 0000-0002-0835-3690 | |
| dc.identifier.orcid | 0000-0003-3714-5310 | |
| dc.identifier.orcid | 0000-0002-7614-6677 | |
| dc.identifier.orcid | 0000-0003-0527-4177 | |
| dc.identifier.orcid | 0000-0002-3180-9502 | |
| dc.identifier.orcid | 0000-0003-2471-1360 | |
| dc.identifier.scopus | 2-s2.0-85164504623 | |
| dc.identifier.scopusquality | Q1 | |
| dc.identifier.uri | https://doi.org/10.1088/1361-6382/acd97b | |
| dc.identifier.uri | https://hdl.handle.net/11129/14540 | |
| dc.identifier.volume | 40 | |
| dc.identifier.wos | WOS:001033309500001 | |
| dc.identifier.wosquality | Q1 | |
| dc.indekslendigikaynak | Web of Science | |
| dc.indekslendigikaynak | Scopus | |
| dc.language.iso | en | |
| dc.publisher | Iop Publishing Ltd | |
| dc.relation.ispartof | Classical and Quantum Gravity | |
| dc.relation.publicationcategory | Makale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.snmz | KA_WoS_20260204 | |
| dc.subject | black holes | |
| dc.subject | black hole shadows | |
| dc.subject | tests of gravity | |
| dc.subject | wormholes | |
| dc.subject | naked singularities | |
| dc.title | Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A | |
| dc.type | Article |










