... Supernova-remnants Signatures of 1050 ergs of energetic protons: Within the SNR: p+ISM/ejecta baryons+mesons gamma-rays, neutrinos, and secondary electrons uCR modifies the shock structure non-linear feedback on diffusive shock acceleration changes of ...
... p e p Integrated spectra of RX J1713.7-3946 Emax=800 TeV for this SNR in the hadronic model Spectral modeling of RXJ1713.7-3946 The main problem of hadronic origin of the gamma-rays of this supernova absence of thermal X-ray emission (Katz & Waxman 2007 ...
... They combine high-risk research addressing most fundamental questions of physics with exciting "guaranteed physics" and the chance to meet the next galactic supernova and exploit it as a bonanza for new physics and astrophysics. ...