Lepto-hadronic Unified Model of \(\gamma\)-ray Supernova Remnants

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Properties of observed SNRs

Known GeV/TeV SNRs and bimodal age distribution

Leptonic v.s. Hadronic

Useful References

  • Dwarkadas (2013) has similar idea of SNR hadronic \(\gamma\)-ray evolution; also mature SNR evolution.

  • Cristofari et al. (2013) calculated the flux evolution, but doesn’t compare with observations

  • We need progenitor mass v.s. bubble size; ambient density distribution; thin shell baryonic mass bushed by wind; SNR evolution in wind environment; electon propagation and cooling; magnetic field strength evolution at SNR shock, etc.