Relativistic Aspects of Accreting Supermassive Black Hole Binaries in Their Natural Habitat: A Review

In this review a summary is given on recent theoretical work, on understanding accreting supermassive black hole binaries in the gravitational wave (GW)-driven regime. A particular focus is given to theoretical predictions of properties of disks and jets in these systems during the gravitational wav...

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Main Author: Roman Gold
Format: Article
Language:English
Published: MDPI AG 2019-05-01
Series:Galaxies
Subjects:
Online Access:https://www.mdpi.com/2075-4434/7/2/63
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author Roman Gold
author_facet Roman Gold
author_sort Roman Gold
collection DOAJ
description In this review a summary is given on recent theoretical work, on understanding accreting supermassive black hole binaries in the gravitational wave (GW)-driven regime. A particular focus is given to theoretical predictions of properties of disks and jets in these systems during the gravitational wave driven phase. Since a previous review by Schnittman 2013, which focussed on Newtonian aspects of the problem, various relativistic aspects have been studied. In this review we provide an update on these relativistic aspects. Further, a perspective is given on recent observational developments that have seen a surge in the number of proposed supermassive black hole binary candidates. The prospect of bringing theoretical and observational efforts closer together makes this an exciting field of research for years to come.
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spelling doaj.art-2ab4ef1e50354ff097686aa14e2e762c2022-12-22T01:32:12ZengMDPI AGGalaxies2075-44342019-05-01726310.3390/galaxies7020063galaxies7020063Relativistic Aspects of Accreting Supermassive Black Hole Binaries in Their Natural Habitat: A ReviewRoman Gold0Institute for Theoretical Physics, Johann Wolfgang Goethe-Universität Max-von-Laue-Str. 1, 60438 Frankfurt am Main, GermanyIn this review a summary is given on recent theoretical work, on understanding accreting supermassive black hole binaries in the gravitational wave (GW)-driven regime. A particular focus is given to theoretical predictions of properties of disks and jets in these systems during the gravitational wave driven phase. Since a previous review by Schnittman 2013, which focussed on Newtonian aspects of the problem, various relativistic aspects have been studied. In this review we provide an update on these relativistic aspects. Further, a perspective is given on recent observational developments that have seen a surge in the number of proposed supermassive black hole binary candidates. The prospect of bringing theoretical and observational efforts closer together makes this an exciting field of research for years to come.https://www.mdpi.com/2075-4434/7/2/63GRMHDnumerical relativityrelativistic astrophysicsjetshigh energy astrophysics
spellingShingle Roman Gold
Relativistic Aspects of Accreting Supermassive Black Hole Binaries in Their Natural Habitat: A Review
Galaxies
GRMHD
numerical relativity
relativistic astrophysics
jets
high energy astrophysics
title Relativistic Aspects of Accreting Supermassive Black Hole Binaries in Their Natural Habitat: A Review
title_full Relativistic Aspects of Accreting Supermassive Black Hole Binaries in Their Natural Habitat: A Review
title_fullStr Relativistic Aspects of Accreting Supermassive Black Hole Binaries in Their Natural Habitat: A Review
title_full_unstemmed Relativistic Aspects of Accreting Supermassive Black Hole Binaries in Their Natural Habitat: A Review
title_short Relativistic Aspects of Accreting Supermassive Black Hole Binaries in Their Natural Habitat: A Review
title_sort relativistic aspects of accreting supermassive black hole binaries in their natural habitat a review
topic GRMHD
numerical relativity
relativistic astrophysics
jets
high energy astrophysics
url https://www.mdpi.com/2075-4434/7/2/63
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