Effect of magnetic fields on the dynamics and gravitational wave emission of Papaloizou-Pringle instability-saturated self-gravitating accretion disks: Simulations in full GR-Reference-Cited by-同舟云学术

Effect of magnetic fields on the dynamics and gravitational wave emission of Papaloizou-Pringle instability-saturated self-gravitating accretion disks: Simulations in full GR

Published:2023-06-28 Issue:12 Volume:107 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Wessel Erik^ORCID,Paschalidis Vasileios^ORCID,Tsokaros Antonios^ORCID,Ruiz Milton^ORCID,Shapiro Stuart L.^ORCID

Funder

National Science Foundation

National Aeronautics and Space Administration

Generalitat Valenciana

Agencia Estatal de Investigación

National Centre for Supercomputing Applications

University of Illinois at Urbana-Champaign

University of Arizona

Extreme Science and Engineering Discovery Environment

UArizona Technology and Research Initiative Fund

UArizona University Information Technology Services

UArizona Office of Research, Innovation, and Impact

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.107.123031/fulltext

Reference88 articles.

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5. Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA

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