by Sheperd Doeleman, Kazunori Akiyama, Lindy Blackburn, Katherine L. Bouman, Geoffrey C. Bower, Avery E. Broderick, Andrew Chael, Vincent L. Fish, Michael D. Johnson, Colin J. Lonsdale, Thomas P. Krichbaum, Daniel Palumbo, Dominic W. Pesce, Alexander W. Raymond, Jonathan Weintroub, and Maciek Wielgus
Published onMay 31, 2019
Black Hole Physics on Horizon Scales
·
Abstract
High-resolution imaging of supermassive black holes can test general relativity and elucidate processes of accretion/jet formation on scales of the event horizon. Enhancements achievable within the decade would provide high-fidelity, time-resolved observations of Sgr A*, M87, and other black holes, enabling breakthroughs in black hole astrophysics.
The full text of this article is only available in PDF format:
Creative Commons Attribution 4.0 International License (CC-BY 4.0)
