Collisionless Magnetorotational Turbulence in Pair Plasmas: Steady-State Dynamics, Particle Acceleration, and Radiative Cooling
dc.contributor.author | Bacchini, F. | |
dc.contributor.author | Zhdankin, V. | |
dc.contributor.author | Gorbunov, E.A. | |
dc.contributor.author | Werner, G.R. | |
dc.contributor.author | Arzamasskiy, L. | |
dc.contributor.author | Begelman, M.C. | |
dc.contributor.author | Uzdensky, D.A. | |
dc.date | 2024 | |
dc.date.accessioned | 2024-08-03T09:04:29Z | |
dc.date.available | 2024-08-03T09:04:29Z | |
dc.identifier.uri | https://orfeo.belnet.be/handle/internal/13381 | |
dc.description | We 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.language | eng | |
dc.title | Collisionless Magnetorotational Turbulence in Pair Plasmas: Steady-State Dynamics, Particle Acceleration, and Radiative Cooling | |
dc.type | Article | |
dc.subject.frascati | Physical sciences | |
dc.audience | Scientific | |
dc.source.title | Physical Review Letters | |
dc.source.volume | 113 | |
dc.source.issue | 4 | |
dc.source.page | A045202 | |
Orfeo.peerreviewed | Yes | |
dc.identifier.doi | 10.1103/PhysRevLett.133.045202 | |
dc.identifier.url |