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Article: The Physics of Accretion Discs, Winds and Jets in Tidal Disruption Events

TitleThe Physics of Accretion Discs, Winds and Jets in Tidal Disruption Events
Authors
Dai, JLLodato, GCheng, R
KeywordsAccretion, accretion discs
Black hole physics
Galaxies: jets
Galaxies: nuclei
Gravitation
Issue Date2021
PublisherSpringer Netherlands. The Journal's web site is located at https://www.springer.com/journal/11214
Citation
Space Science Reviews, 2021, v. 217 n. 1, p. article no. 12 How to Cite?
DOI: http://dx.doi.org/10.1007/s11214-020-00747-x
AbstractAccretion onto black holes is an efficient mechanism in converting the gas mass-energy into energetic outputs as radiation, wind and jet. Tidal disruption events, in which stars are tidally torn apart and then accreted onto supermassive black holes, offer unique opportunities of studying the accretion physics as well as the wind and jet launching physics across different accretion regimes. In this review, we systematically describe and discuss the models that have been developed to study the accretion flows and jets in tidal disruption events. A good knowledge of these physics is not only needed for understanding the emissions of the observed events, but also crucial for probing the general relativistic space-time around black holes and the demographics of supermassive black holes via tidal disruption events.
Persistent Identifierhttp://hdl.handle.net/10722/296388
ISSN
0038-6308
2021 Impact Factor: 8.943
2020 SCImago Journal Rankings: 2.474
ISI Accession Number ID
WOS:000610552400002

 

DC FieldValueLanguage
dc.contributor.authorDai, JL-
dc.contributor.authorLodato, G-
dc.contributor.authorCheng, R-
dc.date.accessioned2021-02-22T04:54:35Z-
dc.date.available2021-02-22T04:54:35Z-
dc.date.issued2021-
dc.identifier.citationSpace Science Reviews, 2021, v. 217 n. 1, p. article no. 12-
dc.identifier.issn0038-6308-
dc.identifier.urihttp://hdl.handle.net/10722/296388-
dc.description.abstractAccretion onto black holes is an efficient mechanism in converting the gas mass-energy into energetic outputs as radiation, wind and jet. Tidal disruption events, in which stars are tidally torn apart and then accreted onto supermassive black holes, offer unique opportunities of studying the accretion physics as well as the wind and jet launching physics across different accretion regimes. In this review, we systematically describe and discuss the models that have been developed to study the accretion flows and jets in tidal disruption events. A good knowledge of these physics is not only needed for understanding the emissions of the observed events, but also crucial for probing the general relativistic space-time around black holes and the demographics of supermassive black holes via tidal disruption events.-
dc.languageeng-
dc.publisherSpringer Netherlands. The Journal's web site is located at https://www.springer.com/journal/11214-
dc.relation.ispartofSpace Science Reviews-
dc.rightsAccepted Manuscript (AAM) This is a post-peer-review, pre-copyedit version of an article published in [insert journal title]. The final authenticated version is available online at: https://doi.org/[insert DOI]-
dc.subjectAccretion, accretion discs-
dc.subjectBlack hole physics-
dc.subjectGalaxies: jets-
dc.subjectGalaxies: nuclei-
dc.subjectGravitation-
dc.titleThe Physics of Accretion Discs, Winds and Jets in Tidal Disruption Events-
dc.typeArticle-
dc.identifier.emailDai, JL: lixindai@hku.hk-
dc.identifier.authorityDai, JL=rp02540-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1007/s11214-020-00747-x-
dc.identifier.scopuseid_2-s2.0-85099339784-
dc.identifier.hkuros321402-
dc.identifier.volume217-
dc.identifier.issue1-
dc.identifier.spagearticle no. 12-
dc.identifier.epagearticle no. 12-
dc.identifier.isiWOS:000610552400002-
dc.publisher.placeNetherlands-

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