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dc.contributor.authorJorge, R.
dc.contributor.authorRicci, P.
dc.contributor.authorGomes Loureiro, Nuno F
dc.date.accessioned2018-10-25T14:50:47Z
dc.date.available2018-10-25T14:50:47Z
dc.date.issued2018-10
dc.date.submitted2018-09
dc.identifier.issn0031-9007
dc.identifier.issn1079-7114
dc.identifier.urihttp://hdl.handle.net/1721.1/118765
dc.description.abstractA numerically efficient framework that takes into account the effect of the Coulomb collision operator at arbitrary collisionalities is introduced. Such a model is based on the expansion of the distribution function on a Hermite-Laguerre polynomial basis to study the effects of collisions on magnetized plasma instabilities at arbitrary mean-free path. Focusing on the drift-wave instability, we show that our framework allows retrieving established collisional and collisionless limits. At the intermediate collisionalities relevant for present and future magnetic nuclear fusion devices, deviations with respect to collision operators used in state-of-the-art turbulence simulation codes show the need for retaining the full Coulomb operator in order to obtain both the correct instability growth rate and eigenmode spectrum, which, for example, may significantly impact quantitative predictions of transport. The exponential convergence of the spectral representation that we propose makes the representation of the velocity space dependence, including the full collision operator, more efficient than standard finite difference methods.en_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevLett.121.165001en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceAmerican Physical Societyen_US
dc.titleTheory of the Drift-Wave Instability at Arbitrary Collisionalityen_US
dc.typeArticleen_US
dc.identifier.citationJorge, R., et al. “Theory of the Drift-Wave Instability at Arbitrary Collisionality.” Physical Review Letters, vol. 121, no. 16, Oct. 2018. © 2018 American Physical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Laboratory for Nuclear Scienceen_US
dc.contributor.departmentMassachusetts Institute of Technology. Plasma Science and Fusion Centeren_US
dc.contributor.mitauthorGomes Loureiro, Nuno F
dc.relation.journalPhysical Review Lettersen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2018-10-19T18:01:18Z
dc.language.rfc3066en
dc.rights.holderAmerican Physical Society
dspace.orderedauthorsJorge, R.; Ricci, P.; Loureiro, N. F.en_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0001-9755-6563
mit.licensePUBLISHER_POLICYen_US


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