Reinterpretation of the Fermi acceleration of cosmic rays in terms of the ballistic surfing acceleration in supernova shocks
Krzysztof Stasiewicz

TL;DR
This paper reexamines cosmic ray acceleration mechanisms, demonstrating that ballistic surfing acceleration (BSA) better explains observed spectra and challenges the traditional Fermi acceleration model, especially in supernova shocks.
Contribution
It introduces BSA as a more accurate alternative to Fermi acceleration for cosmic rays, clarifying its physical basis and implications for shock physics.
Findings
BSA reproduces the observed spectral index below the knee.
Fermi acceleration is inconsistent with electrodynamics.
The knee in the spectrum corresponds to ions with specific gyroradii.
Abstract
The applicability of first-order Fermi acceleration in explaining the cosmic ray spectrum has been reexamined using recent results on shock acceleration mechanisms from the Multiscale Magnetospheric mission in Earth's bow shock. It is demonstrated that the Fermi mechanism is a crude approximation of the ballistic surfing acceleration (BSA) mechanism. While both mechanisms yield similar expressions for the energy gain of a particle after encountering a shock once, leading to similar power-law distributions of the cosmic ray energy spectrum, the Fermi mechanism is found to be inconsistent with fundamental equations of electrodynamics. It is shown that the spectral index of cosmic rays is determined by the average magnetic field compression rather than the density compression, as in the Fermi model. It is shown that the knee observed in the spectrum at an energy of 5x10^{15} eV could…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena · Solar and Space Plasma Dynamics
