Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
Constraints on black-hole charges with the 2017 EHT observations of M87∗. / EHT collaboration.
в: Physical Review D, Том 103, № 10, 104047, 20.05.2021.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - Constraints on black-hole charges with the 2017 EHT observations of M87∗
AU - (EHT Collaboration)
AU - Kocherlakota, Prashant
AU - Rezzolla, Luciano
AU - Falcke, Heino
AU - Fromm, Christian M.
AU - Kramer, Michael
AU - Mizuno, Yosuke
AU - Nathanail, Antonios
AU - Olivares, Héctor
AU - Younsi, Ziri
AU - Akiyama, Kazunori
AU - Alberdi, Antxon
AU - Alef, Walter
AU - Algaba, Juan Carlos
AU - Anantua, Richard
AU - Asada, Keiichi
AU - Azulay, Rebecca
AU - Baczko, Anne Kathrin
AU - Ball, David
AU - Baloković, Mislav
AU - Barrett, John
AU - Benson, Bradford A.
AU - Bintley, Dan
AU - Blackburn, Lindy
AU - Blundell, Raymond
AU - Boland, Wilfred
AU - Bouman, Katherine L.
AU - Bower, Geoffrey C.
AU - Boyce, Hope
AU - Bremer, Michael
AU - Brinkerink, Christiaan D.
AU - Brissenden, Roger
AU - Britzen, Silke
AU - Broderick, Avery E.
AU - Broguiere, Dominique
AU - Bronzwaer, Thomas
AU - Byun, Do Young
AU - Carlstrom, John E.
AU - Chael, Andrew
AU - Chan, Chi Kwan
AU - Chatterjee, Shami
AU - Chatterjee, Koushik
AU - Chen, Ming Tang
AU - Chen, Yongjun
AU - Chesler, Paul M.
AU - Cho, Ilje
AU - Christian, Pierre
AU - Conway, John E.
AU - Cordes, James M.
AU - Crawford, Thomas M.
AU - Jorstad, Svetlana
N1 - Publisher Copyright: © 2021 authors. Published by the American Physical Society.
PY - 2021/5/20
Y1 - 2021/5/20
N2 - 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.
AB - 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.
KW - CALIBRATION
KW - SHADOWS
KW - GRAVITY
KW - TESTS
KW - FIELD
KW - POLARIZATION
KW - ASTROPY
KW - MASS
UR - http://www.scopus.com/inward/record.url?scp=85107031687&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.103.104047
DO - 10.1103/PhysRevD.103.104047
M3 - Article
AN - SCOPUS:85107031687
VL - 103
JO - Physical review D
JF - Physical review D
SN - 2470-0010
IS - 10
M1 - 104047
ER -
ID: 86508646