Charged particle transport in laser-driven magnetized turbulence: understanding the intergalactic voyage of ultra-high energy cosmic rays
ORAL
Abstract
How charged particles and turbulent magnetic fields interact is key to understanding the journey of cosmic rays through space. In this talk we report on numerical simulations and laser-driven experiments at the OMEGA Laser Facility that measure the propagation of energetic particles through random magnetic fields in a turbulent plasma. We characterize their angular diffusion and recover their mean free path and associated diffusion coefficients. The OMEGA experiments we present constitute the first laboratory probe of particle diffusion through magnetized turbulence in the absence of a mean background field and complement laboratory studies of energetic particle propagation in diffuse plasmas, where there is a strong guide field. The experiments emulate the propagation of ultra-high energy cosmic rays through the intergalactic medium, critical for interpreting anisotropies in their arrival direction and for constraining the distance of their sources
*The research leading to these results has received funding from the ERC, U.S. DOE NNSA, U.S. DOE Office of Science, NSF, AWE, EPSRC, STFC, and NRF of Korea. Awards of computer time were provided by the U.S. DOE ALCC program and used resources of the ALCF at ANL. The experiments were conducted at LLE, University of Rochester.
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Presenters
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Petros Tzeferacos
- Univ of Chicago
- University of Chicago, University of Oxford