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The gamma-ray visibility of supernova remnants: a test of cosmic ray origin
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Gamma ray production in supernova remnants is discussed on the basis of current ideas about cosmic ray acceleration.
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Cited by 4 Pith papers
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Superdiffusion of cosmic rays in the vicinity of their accelerators and the resulting $\gamma$-ray emission
Superdiffusion produces constant or r^{α-3} CR radial profiles near sources; the associated γ-ray morphology can distinguish it from normal diffusion with IACTs.
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Hybrid Simulations of Proton Acceleration at Oblique High-$\beta$ Shocks
Weak quasi-perpendicular high-β ICM shocks accelerate protons inefficiently (ε_CR ≲ 0.1%), while Ms ≳ 10 or ϑ ≲ 45° shocks reach a few percent with steep spectra.
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SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics
A self-consistent multi-zone kinetic model reproduces SN 1006's spectrum and morphology, finding ~20% CR acceleration efficiency in quasi-parallel shocks, <1% in quasi-perpendicular shocks, and predominantly leptonic ...
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A HINSA view of cosmic-ray ionization in IC 348 and NGC 1333: evidence for a strong low-energy cosmic-ray disparity
HINSA observations show CRIR decreasing with H2 column density in both clouds, with IC 348 values an order of magnitude above NGC 1333, modeled as an order-of-magnitude difference in low-energy CR populations from loc...
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