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Measuring Small-scale Turbulence in Supernova Remnants with Jitter Radiation
Emily Simon, Damiano Caprioli, Niccolò Bucciantini +2
Hard X-ray emission from Cas A has been attributed to jitter radiation, implying magnetic turbulence on scales near or below the ion Larmor radius. We propose these fields arise fr…
Detecting Neutrino Emission from Supernova Remnants: A Theoretically Motivated Target Catalog
Emily Simon, Rebecca Diesing, Damiano Caprioli +1
Galactic supernova remnants (SNRs) are thought to accelerate cosmic rays (CRs) to several PeV energies, but this has yet to be confirmed as general behavior. Although several sourc…
A "Faux-Shock" Method for Hybrid Simulations of Astrophysical Shocks
Emily R. Simon, Damiano Caprioli, Colby C. Haggerty +1
We demonstrate a novel setup for hybrid particle-in-cell simulations designed to isolate the physics of the shock precursor over long time periods for significantly lower computati…
Maximum energy achievable in supernova remnants: self-consistent simulations
Emily Simon, Damiano Caprioli, Colby Haggerty +1
It has been long believed that oblique and quasi-perpendicular configurations in supernova remnants (SNRs) were inefficient at injecting ions into diffusive shock acceleration (DSA…