Self-generated magnetic turbulence in cosmic filaments suppresses low-rigidity UHECR escape for cluster-scale sources, photodisintegrates heavy nuclei into secondary protons below the ankle, and yields neutrino and gamma-ray fluxes compatible with or constrained by current limits.
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3 Pith papers cite this work. Polarity classification is still indexing.
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3D MHD simulations of CCSN remnants from RSG and WR stars show faster shocks from photoionization and CSM expansion, plus coherent reflected shocks in WR cases, with weakly magnetized bubbles limiting PeV acceleration.
New wideband radio polarization data for SNR G315.4-2.3 indicate low internal rotation measures, a weak regular line-of-sight magnetic field of about 1.4 microGauss, and turbulent-to-regular field ratios exceeding 3, with similar properties across regions of differing evolution.
citing papers explorer
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Self-confinement of ultra-high-energy nuclei in cosmic filaments: implications for the UHECR spectrum and composition
Self-generated magnetic turbulence in cosmic filaments suppresses low-rigidity UHECR escape for cluster-scale sources, photodisintegrates heavy nuclei into secondary protons below the ankle, and yields neutrino and gamma-ray fluxes compatible with or constrained by current limits.
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Multi-Dimensional MHD simulations of young Core-Collapse Supernova Remnants
3D MHD simulations of CCSN remnants from RSG and WR stars show faster shocks from photoionization and CSM expansion, plus coherent reflected shocks in WR cases, with weakly magnetized bubbles limiting PeV acceleration.
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A new wideband radio polarization observation of the Supernova Remnant G315.4$-$2.3
New wideband radio polarization data for SNR G315.4-2.3 indicate low internal rotation measures, a weak regular line-of-sight magnetic field of about 1.4 microGauss, and turbulent-to-regular field ratios exceeding 3, with similar properties across regions of differing evolution.