Self-diffusion in two-dimensional quasi-magnetized rotating dusty plasmas

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dc.contributor.authorHartmann, Peter
dc.contributor.authorReyes, J. C.
dc.contributor.authorKostadinova, Eva Georgieva, 1992-
dc.contributor.authorMatthews, Lorin Swint.
dc.contributor.authorHyde, Truell Wayne.
dc.contributor.authorDzhumagulova, K. N.
dc.contributor.authorMasheyeva, R. U.
dc.contributor.authorRamazanov, T. S.
dc.contributor.authorOtt, T.
dc.contributor.authorkahlert, H.
dc.contributor.authorBonitz, M.
dc.contributor.authorKorolov, I.
dc.contributor.authorDonko, Zoltan
dc.date.accessioned2019-07-16T14:47:06Z
dc.date.available2019-07-16T14:47:06Z
dc.date.issued2019-01-10
dc.description.abstractThe self-diffusion phenomenon in a two-dimensional dusty plasma at extremely strong (effective) magnetic fields is studied experimentally and by means of molecular dynamics simulations. In the experiment the high magnetic field is introduced by rotating the particle cloud and observing the particle trajectories in a corotating frame, which allows reaching effective magnetic fields up to 3000 T. The experimental results confirm the predictions of the simulations: (i) superdiffusive behavior is found at intermediate timescales and (ii) the dependence of the self-diffusion coefficient on the magnetic field is well reproduced.en_US
dc.description.keywordsself-diffusionen_US
dc.description.keywordsmagnetized plasmaen_US
dc.description.keywordsdusty plasmaen_US
dc.identifier.citationPhysical Review E, 99, 013203, January 10, 2019.en_US
dc.identifier.doi10.1103/PhysRevE.99.013203
dc.identifier.urihttps://hdl.handle.net/2104/10640
dc.language.isoenen
dc.publisherPhysical Review Een_US
dc.titleSelf-diffusion in two-dimensional quasi-magnetized rotating dusty plasmasen_US
dc.typeArticleen

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