Numerical relativity in spherical coordinates: A new dynamical spacetime and general relativistic MHD evolution framework for the Einstein Toolkit-Reference-Cited by-同舟云学术

Numerical relativity in spherical coordinates: A new dynamical spacetime and general relativistic MHD evolution framework for the Einstein Toolkit

Published:2020-05-05 Issue:10 Volume:101 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Mewes Vassilios^ORCID,Zlochower Yosef^ORCID,Campanelli Manuela^ORCID,Baumgarte Thomas W.^ORCID,Etienne Zachariah B.^ORCID,Armengol Federico G. Lopez^ORCID,Cipolletta Federico^ORCID

Funder

National Science Foundation

West Virginia University

National Aeronautics and Space Administration

Simons Foundation

U.S. Department of Energy

Office of Science

National Nuclear Security Administration

Ministerio de Economía y Competitividad

Bowdoin College

Exascale Computing Project

Rochester Institute of Technology

Extreme Science and Engineering Discovery Environment

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.101.104007/fulltext

Reference199 articles.

1. Observation of Gravitational Waves from a Binary Black Hole Merger

2. Properties of the Binary Black Hole Merger GW150914

3. GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence

4. GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2

5. Erratum: GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2 [Phys. Rev. Lett. 118 , 221101 (2017)]

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