Author Correction: Fundamental physics opportunities with the next-generation Event Horizon Telescope

After this article was published, the Authors requested to change the title and abstract back to their original submission, since the removal of mention of the ngEHT project from the title and abstract during revisions does not accurately convey nor reflect the fact that this work was initiated and undertaken as part of the ngEHT project. The changes made following suggestions by a reviewer had not been approved by all authors/project director. Instead of “Fundamental physics opportunities with future ground-based mm/sub-mm VLBI arrays” the title should read “Fundamental physics opportunities with the next-generation Event Horizon Telescope”. The running title should be changed from “Fundamental physics opportunities with future ground…” to “Fundamental physics opportunities with the ngEHT”. Also, the current Abstract “The Event Horizon Telescope (EHT) Collaboration recently published the first images of the supermassive black holes in the cores of the Messier 87 and Milky Way galaxies. These observations have provided a new means to study supermassive black holes and probe physical processes occurring in the strong-field regime. We review the prospects of future observations and theoretical studies of supermassive black hole systems. Current ground-based very-long-baseline interferometry (VLBI) arrays like the EHT and proposed future extensions like the next-generation Event Horizon Telescope will greatly enhance the capabilities of black-hole imaging interferometry. These enhancements will open up several previously inaccessible avenues of investigation, thereby providing important new insights into the properties of supermassive black holes and their environments. This review describes the current state of knowledge for five key science cases, summarising the unique challenges and opportunities for fundamental physics investigations that future mm/sub-mm VLBI developments will enable” should be changed to “The Event Horizon Telescope (EHT) Collaboration recently published the first images of the supermassive black holes in the cores of the Messier 87 and Milky Way galaxies. These observations have provided a new means to study supermassive black holes and probe physical processes occurring in the strong-field regime. We review the prospects of future observations and theoretical studies of supermassive black hole systems with the next-generation Event Horizon Telescope (ngEHT) project, which will greatly enhance the capabilities of the existing EHT array. These enhancements will open up several previously inaccessible avenues of investigation, thereby providing important new insights into the properties of supermassive black holes and their environments. This review describes the current state of knowledge for five key science cases, summarising the unique challenges and opportunities for fundamental physics investigations that the ngEHT will enable”. The Original Article has been corrected.

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Publication Details

Journal
Living Reviews in Relativity
Published
2025-09-22
DOI
https://doi.org/10.1007/s41114-025-00062-3
Citations
1
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
1.87
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Author Correction: Fundamental physics opportunities with the next-generation Event Horizon Telescope

Sushant G. Ghosh, S. Britzen, Aditya Tamar, Saurabh Kumar et al.
1 citations
Living Reviews in Relativity
Dark Matter and Cosmic Phenomena
1.87
article

Author Correction: Fundamental physics opportunities with the next-generation Event Horizon Telescope

Sushant G. Ghosh, S. Britzen, Aditya Tamar, Saurabh Kumar, Dominic W. Pesce, Roman Gold, Astrid Eichhorn, Christian M. Fromm, Shammi Tahura, Avery E. Broderick, Priyamvada Natarajan, Yun Fang, Héctor Olivares, Leonid Gurvits, Paul Tiede, Sheperd S. Doeleman, Prashant Kocherlakota, Janice Houston, K. Yakut, Surjeet Rajendran, Peter Galison, Michael D. Johnson, Raúl Carballo-Rubio, Andrew Chael, Shahar Hadar, Lijing Shao, Ziri Younsi, Vítor Cardoso, Richard Brito, Maciek Wielgus, Xiao Xue, Peter B. Denton, T. M. Eubanks, Luca Visinelli, Hooman Davoudiasl, Koushik Chatterjee, A. Foschi, Lindy Blackburn, Pedro V. P. Cunha, Rittick Roy, Huan Yang, Daniel C. M. Palumbo, Dimitry Ayzenberg, Aaron Held, Yifan Chen, Frédéric E. Vincent, Zhiren Wang, Yichao Hu
article en
1 citations

Abstract

After this article was published, the Authors requested to change the title and abstract back to their original submission, since the removal of mention of the ngEHT project from the title and abstract during revisions does not accurately convey nor reflect the fact that this work was initiated and undertaken as part of the ngEHT project. The changes made following suggestions by a reviewer had not been approved by all authors/project director. Instead of “Fundamental physics opportunities with future ground-based mm/sub-mm VLBI arrays” the title should read “Fundamental physics opportunities with the next-generation Event Horizon Telescope”. The running title should be changed from “Fundamental physics opportunities with future ground…” to “Fundamental physics opportunities with the ngEHT”. Also, the current Abstract “The Event Horizon Telescope (EHT) Collaboration recently published the first images of the supermassive black holes in the cores of the Messier 87 and Milky Way galaxies. These observations have provided a new means to study supermassive black holes and probe physical processes occurring in the strong-field regime. We review the prospects of future observations and theoretical studies of supermassive black hole systems. Current ground-based very-long-baseline interferometry (VLBI) arrays like the EHT and proposed future extensions like the next-generation Event Horizon Telescope will greatly enhance the capabilities of black-hole imaging interferometry. These enhancements will open up several previously inaccessible avenues of investigation, thereby providing important new insights into the properties of supermassive black holes and their environments. This review describes the current state of knowledge for five key science cases, summarising the unique challenges and opportunities for fundamental physics investigations that future mm/sub-mm VLBI developments will enable” should be changed to “The Event Horizon Telescope (EHT) Collaboration recently published the first images of the supermassive black holes in the cores of the Messier 87 and Milky Way galaxies. These observations have provided a new means to study supermassive black holes and probe physical processes occurring in the strong-field regime. We review the prospects of future observations and theoretical studies of supermassive black hole systems with the next-generation Event Horizon Telescope (ngEHT) project, which will greatly enhance the capabilities of the existing EHT array. These enhancements will open up several previously inaccessible avenues of investigation, thereby providing important new insights into the properties of supermassive black holes and their environments. This review describes the current state of knowledge for five key science cases, summarising the unique challenges and opportunities for fundamental physics investigations that the ngEHT will enable”. The Original Article has been corrected.

Living Reviews in RelativityVol. 28(1)
University of Central Florida (US), Oranim Academic College of Education (IL), Ningbo University (CN), Goethe University Frankfurt (DE), National Institute of Technology Karnataka (IN), Instituto de Engenharia de Sistemas e Computadores Investigação e Desenvolvimento (PT), University of Iowa (US), Centre National de la Recherche Scientifique (FR), Woodwell Climate Research Center (US), University of Salerno (IT), Harvard University (US), Johns Hopkins University (US), University of Waterloo (CA), Universität Hamburg (DE), Istituto Nazionale di Fisica Nucleare (IT), Délégation Paris 7 (FR), University of Southern Denmark (DK), Perimeter Institute (CA), Chinese Academy of Sciences (CN), Brookhaven National Laboratory (US), Princeton University (US), Peking University (CN), Université Paris Cité (FR), Heidelberg University (DE), University of Würzburg (DE), Université Paris Sciences et Lettres (FR), Princeton Plasma Physics Laboratory (US), Observatoire de Paris (FR), Harvard University Press (US), Deutsches Elektronen-Synchrotron DESY (DE), École Normale Supérieure - PSL (FR), Yale University (US), Sorbonne Université (FR), Ege University (TR), Sorbonne Paris Cité (FR), École Normale Supérieure (BI), Kavli Institute for Theoretical Sciences (CN), Center for Astrophysics Harvard & Smithsonian (US), North Carolina Space Grant Consortium (US), Niels Brock (DK), Astronomy and Space (AU), Max Planck Institute for Radio Astronomy (DE), Instituto de Astrofísica de Andalucía (ES), National Astronomical Observatories (CN), University College London (GB), Jamia Millia Islamia (IN), University of Aveiro (PT), University of Maryland, College Park (US), Heidelberg Institute for Theoretical Studies (DE), University of Guelph (CA), Joint Institute for VLBI ERIC (NL), University of Tübingen (DE), University of Amsterdam (NL), University of Haifa (IL), University of KwaZulu-Natal (ZA), Delft University of Technology (NL), Tsinghua University (CN)
Openalex Percentile: Top 12%
Dark Matter and Cosmic Phenomena
1.87
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