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Your search keyword '"Waxman E"' showing total 9 results

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9 results on '"Waxman E"'

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1. AMS-02 results support the secondary origin of cosmic ray positrons.

2. Astrophysical neutrinos: flavor ratios depend on energy.

3. Energy spectrum of particles accelerated in relativistic collisionless shocks.

4. TeV neutrinos from core collapse supernovae and hypernovae.

5. High energy neutrinos from gamma-ray bursts with precursor supernovae.

6. Probing microquasars with TeV neutrinos.

7. TeV neutrinos from successful and choked gamma-ray bursts.

8. TeV neutrinos and GeV photons from shock breakout in supernovae.

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