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- W1570472045 abstract "Some recent experiments detecting very high energy (VHE) gamma rays above 10-20 TeV independently reported VHE bursts for some bright gamma-ray bursts (GRBs). If these signals are truly from GRBs, these GRBs must emit a much larger amount of energy as VHE gamma rays than in the ordinary photon energy range of GRBs (keV-MeV). We show that such extreme phenomena can be reasonably explained by synchrotron radiation of protons accelerated to ~1020-1021 eV, which we predicted recently. Protons seem to carry about (mp/me) times larger energy than electrons, and hence the total energy liberated by one GRB becomes as large as ~1056 (ΔΩ/4π) ergs. Therefore, a strong beaming of GRB energy is highly likely. Extension of the VHE spectrum beyond 20 TeV gives a nearly model-independent lower limit of the Lorentz factor of GRBs, as γ≳500. Furthermore, our model gives the correct energy range and time variability of ordinary keV-MeV gamma rays of GRBs by synchrotron radiation of electrons. Therefore, the VHE bursts of GRBs strongly support the hypothesis that ultra-high-energy cosmic rays observed on the Earth are produced by GRBs." @default.
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- W1570472045 date "1998-12-20" @default.
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- W1570472045 title "T[CLC]e[/CLC]V Burst of Gamma-Ray Bursts and Ultra–High-Energy Cosmic Rays" @default.
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- W1570472045 doi "https://doi.org/10.1086/311772" @default.
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