Effect of Magnetised Discontinuity on Diffusive Shock Acceleration
Anshuman Verma, Saksham Chandna, Divyansh Tripathi, Ritam Mallick

TL;DR
This study explores how magnetic fields and different diffusion mechanisms influence particle acceleration at shocks, revealing that magnetisation and pitch-angle dependence significantly enhance spectral flattening and acceleration efficiency.
Contribution
It provides a comprehensive analysis of magnetised shock conditions and diffusion effects on particle spectra, highlighting the importance of pitch-angle-dependent diffusion in shock acceleration.
Findings
Magnetic fields improve particle confinement and lead to flatter spectra.
Absence of magnetisation results in steeper spectra due to rapid escape.
Pitch-angle-dependent diffusion causes the strongest spectral flattening.
Abstract
We investigate the impact of magnetic fields and diffusion mechanisms on the energy spectra of particles accelerated via diffusive shock acceleration. We analyse magnetised shock jump conditions and demonstrate how magnetisation and angular dependence modify upstream and downstream velocities, which enter the transport equation within a Monte Carlo simulation framework. We consider constant, momentum-dependent, and pitch-angle-dependent diffusion coefficients to assess their influence on particle acceleration. Our results show that magnetic fields enhance particle confinement and facilitate more efficient energy gain. In the absence of magnetisation, particle spectra tend to be steeper due to rapid escape and weaker scattering effects, whereas magnetised shocks systematically produce flatter spectra across all diffusion models. Among them, pitch-angle-dependent diffusion leads to the…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae · Solar and Space Plasma Dynamics
