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Are Gamma-Ray Bursts at Cosmological Distances Optically-Thin?

Abraham Loeb
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Abstract

The observed spatial distribution of $γ-$ray bursts indicates that they probably originate at cosmological distances. At this distance scale their variability timescale and flux above MeV imply an initial optical-depth to pair production $> 10^{10}$. This appears to be in conflict with their highly non-thermal spectra. We show that this difficulty can be removed if axion bursts from supernovae are converted to $γ-$rays over cosmological distances. Nonthermal bursts with the relevant flux, duration, variability and spectra are obtained just for the range of axion masses of $10^{-5}-10^{-4}{\rm eV}$ that accounts for the cold dark matter in the universe. The observed rate of $γ-$ray bursts implies that axions should be converted efficiently to photons in only one out of $\sim 10^{4}$ supernovae.

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Abraham Loeb. 1993-08-31. Are Gamma-Ray Bursts at Cosmological Distances Optically-Thin?. https://doi.org/10.1103/physrevd.48.r3419

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