Isotropic gamma-radiation and the metagalactic cosmic-ray intensity
Mathematical interpretation of OSO-3 data to limit metagalactic cosmic-ray intensity
Engineering topics
Publications and source records attributed to Stecker, F. W..
Mathematical interpretation of OSO-3 data to limit metagalactic cosmic-ray intensity
Cosmic gamma ray spectra from production and decay of neutral pi-mesons produced in metagalactic cosmic-ray proton-proton collisions
General formula for calculating equilibrium spectra of secondary cosmic ray positrons in galaxy and cosmic annihilation gamma ray spectra
Nucleon isobars and hyperons carrying off interstellar and intergalactic proton-proton collision energy, discussing high energy gamma ray decay product
High energy cosmic ray spectrum interaction with microwave thermal radiation for production of photomeson
Gamma ray production from cosmic proton-antiproton interactions
The discovery of soft gamma ray bursts has led to the speculation that these bursts are caused by the bremsstrahlung of electrons accelerated to high energies in a stellar flare event. If the stellar flare hypothesis is verified, it may imply a significant source of low energy cosmic rays in the solar neighborhood, depending on the frequency and intensity of the flares.