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dc.contributor.authorDewberry, Janosz Wen
dc.contributor.authorLatter, Henriken
dc.contributor.authorOgilvie, Gordonen
dc.contributor.authorFromang, Sebastianen
dc.date.accessioned2020-08-05T12:24:33Z
dc.date.available2020-08-05T12:24:33Z
dc.identifier.issn0035-8711
dc.identifier.urihttps://www.repository.cam.ac.uk/handle/1810/308792
dc.description.abstractHigh-frequency quasi-periodic oscillations (HFQPOs) observed in the emission of black-hole X-ray binary systems promise insight into strongly curved spacetime. `Discoseismic' oscillations with frequencies set by the intrinsic properties of the central black hole, in particular `trapped inertial waves' (r-modes), offer an attractive explanation for HFQPOs. To produce an observable signature, however, such oscillations must be excited to sufficiently large amplitudes. Turbulence driven by the magnetorotational instability (MRI) fails to provide the necessary amplification, but r-modes may still be excited via interaction with accretion disc warps or eccentricities. We present 3D global hydrodynamic simulations of relativistic accretion discs, which demonstrate for the first time the excitation of trapped inertial waves by an imposed eccentricity in the flow. While the r-modes' saturated state depends on the vertical boundary conditions used in our unstratified, cylindrical framework, their excitation is unambiguous in all runs with eccentricity >0.005 near the ISCO. These simulations provide a proof of concept, demonstrating the robustness of trapped inertial wave excitation in a non-magnetized context. In a companion paper, we explore the competition between this excitation, and damping by magnetohydrodynamic turbulence.
dc.publisherOxford University Press
dc.rightsAll rights reserved
dc.titleHFQPOs and discoseismic mode excitation in eccentric, relativistic discs. I. Hydrodynamic simulations.en
dc.typeArticle
prism.publicationNameMonthly Notices of the Royal Astronomical Societyen
dc.identifier.doi10.17863/CAM.55880
dcterms.dateAccepted2020-03-26en
rioxxterms.versionofrecord10.1093/mnras/staa1897en
rioxxterms.versionVoR
rioxxterms.licenseref.urihttp://www.rioxx.net/licenses/all-rights-reserveden
rioxxterms.licenseref.startdate2020-03-26en
dc.contributor.orcidOgilvie, Gordon [0000-0002-7756-1944]
dc.identifier.eissn1365-2966
rioxxterms.typeJournal Article/Reviewen
pubs.funder-project-idSTFC (ST/P000673/1)
cam.issuedOnline2020-07-08en
dc.identifier.urlhttp://dx.doi.org/10.1093/mnras/staa1897en


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