23 citations · 45 across the 3 of their papers we have counts for
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Particle acceleration, escape and non-thermal emission from core-collapse supernovae inside non-identical wind-blown bubbles
Samata Das, Robert Brose, Martin Pohl +2
In the core-collapse scenario, the supernova remnants evolve inside the complex wind-blown bubbles, structured by massive progenitors during their lifetime. Therefore, particle acc…
Spectral softening in core-collapse supernova remnant expanding inside wind-blown bubble
Samata Das, Robert Brose, Dominique M. -A. Meyer +3
Context. Galactic cosmic rays are widely assumed to arise from diffusive shock acceleration, specifically at shocks in supernova remnants (SNRs). These shocks expand in a complex e…
Production of secondary particles in heavy nuclei interactions in supernova remnants
Maulik Bhatt, Iurii Sushch, Martin Pohl +5
Depending on their type, supernova remnants may have ejecta material with high abundance of heavy elements such as carbon or oxygen. In addition, core-collapse supernovae explode i…