English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

We consider diffusive shock acceleration in supernova remnants throughouttheir evolution including a radiative stage. It is found that a more efficientacceleration and fast exit of particles at the radiative stage results in thehardening of the source cosmic ray proton and electron spectra at energies$\sim 100-500$ GeV. The effect is stronger for cosmic ray electrons.

Role of the radiative stage for cosmic ray acceleration in SNRs