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This work presents theoretical models for high-energy astrophysical sources, including gamma-ray bursts (GRBs), active galactic nuclei (AGN), and pulsars. We explore cosmic rays, gamma rays, and X-rays, providing insights into their emissions and interactions. Our findings are relevant to a variety of high-energy missions such as Swift, HETE, GLAST, XMM, and Chandra. Additionally, we discuss UHECR spectra, photomeson production, and time-dependent GRB model spectra, as well as models for high-energy emissions from millisecond pulsars.
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Theoretical Astrophysics • Theoretical modeling of high energy astrophysics sources • Cosmic rays, gamma rays, x-rays… • GRBs, AGN, pulsars, jets • Results relevant to variety of high energy missions, including Swift, HETE, GLAST, XMM, Chandra UHECR Spectra w/ Photomeson Production Time-dependent GRB model spectra Model HE emission from millisec pulsar