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dc.contributor.authorGorbunov, E.A.
dc.contributor.authorGrošelj, D.
dc.contributor.authorBacchini, F.
dc.date2025
dc.date.accessioned2025-11-04T13:44:13Z
dc.date.available2025-11-04T13:44:13Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/14387
dc.descriptionWe study particle acceleration in strongly turbulent pair plasmas using novel 3D particle-in-cell simulations, featuring particle injection from an external heat bath and diffusive escape. We demonstrate the formation of steady-state, nonthermal particle distributions with maximum energies reaching the Hillas limit. The steady state is characterized by the equilibration of plasma kinetic and magnetic pressures, which imposes upper limits on the acceleration rate. With growing cold plasma magnetization 𝜎0, nonthermal power-law spectra become harder, and the fraction of energy channeled into escaping cosmic rays increases. At 𝜎0 ≳1, the escaping cosmic rays amount to more than 50% of the dissipated energy. Our method allows for kinetic studies of particle acceleration under steady-state conditions, with applications to a variety of astrophysical systems.
dc.languageeng
dc.titleLeaking Outside the Box: Kinetic Turbulence with Cosmic-Ray Escape
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeCosmic ray acceleration
dc.subject.freeCosmic ray sources
dc.subject.freeElectron-positron plasmas
dc.subject.freeIntergalactic medium
dc.subject.freeMagnetized plasma
dc.subject.freeRelativistic plasmas
dc.subject.freeAstrophysical electromagnetic fields
dc.subject.freeAstrophysical & cosmological simulations
dc.subject.freeFirst-principles calculations in plasma physics
dc.subject.freeFokker-Planck & Vlasov model
dc.subject.freeNumerical relativity
dc.subject.freeParticle-in-cell methods
dc.subject.freePlasma kinetic theory
dc.source.titlePhysical Review Letters
dc.source.volume135
dc.source.issue6
dc.source.pageA065201
Orfeo.peerreviewedYes
dc.identifier.doi10.1103/3777-z37m
dc.identifier.url


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