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dc.contributor.authorBacchini, F.
dc.contributor.authorZhdankin, V.
dc.contributor.authorGorbunov, E.A.
dc.contributor.authorWerner, G.R.
dc.contributor.authorArzamasskiy, L.
dc.contributor.authorBegelman, M.C.
dc.contributor.authorUzdensky, D.A.
dc.date2024
dc.date.accessioned2024-08-03T09:04:29Z
dc.date.available2024-08-03T09:04:29Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/13381
dc.descriptionWe present 3D fully kinetic shearing-box simulations of pair-plasma magnetorotational turbulence with unprecedented macro-to-microscopic scale separation. While retrieving the expected fluid behavior of the plasma at large scales, we observe a steepening of turbulent spectra at kinetic scales and substantial angular-momentum transport linked with kinetic processes. For the first time, we provide a definitive demonstration of nonthermal particle acceleration in kinetic magnetorotational turbulence agnostically of shearing-box initial conditions by means of a novel strategy exploiting synchrotron cooling.
dc.languageeng
dc.titleCollisionless Magnetorotational Turbulence in Pair Plasmas: Steady-State Dynamics, Particle Acceleration, and Radiative Cooling
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titlePhysical Review Letters
dc.source.volume113
dc.source.issue4
dc.source.pageA045202
Orfeo.peerreviewedYes
dc.identifier.doi10.1103/PhysRevLett.133.045202
dc.identifier.url


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