Experimental tests of the supernovae origin of cosmic rays
Detection of supernovae pulse by gamma ray telescope and atmospheric scintillation method
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Detection of supernovae pulse by gamma ray telescope and atmospheric scintillation method
Survival of heavy nuclei in Colgates supernova cosmic ray acceleration model
Supernova process noting electron type neutrino interactions, gravitational collapse and stability and neutrino energy transfer at extreme densities and temperatures
Nucleosynthesis by neutron capture on fast time scale in supernova explosion models for dynamics of highly evolved massive star cores
Young Virgo cluster supernova X ray to optical luminosity ratio upper limit from Mt. Palomar Schmidt telescope and Aerobee rocket observations
Animal extinction on earth in geological times by nearby exploding supernovae cosmic radiation shown irreconcilable with galactic cosmic ray propagation
Stars with core greater than 30 solar masses become unstable due to electron-positron pair production at 1.5-2 billion K leading to supernova
Statistical mechanics of origin of cosmic rays in supernovae explosions
Nucleosynthesis in dynamics of massive star cores, noting element synthesis by neutron capture in supernova explosions
Pulsars and ancient chinese records of supernova explosions, relating luminous intensities, radio sources and evolution
Design of photomultiplier system for observing energy photon bursts from supernovae
Pulsars and X ray emitting supernova remnants
Heavy nuclei survival in cosmic rays Colgate supernova acceleration model, assuming plasma wave instability in shock wave
Supernova light emitted from surrounding gas layer, describing gas density role in type I and type II events
Pulsars pulse duration and shape as key to neutron stars linkage with supernova explosions
Pulsars in supernova remnants emitting X rays
Galactic cosmic rays origin in terms of statistical mechanical model of supernova explosions