# Lepto-hadronic Unified Model of $$\gamma$$-ray Supernova Remnants

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# 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.