![]() ![]() The theoretical curves were fit to the data by eye, by requiring the model flux at 3 × 10 19 eV to provide the whole intensity at this energy. The three theoretical curves are for differing assumed equatorial ellipticities of the neutron stars: ǫ = 0 ("no GR") ǫ = 10 −2 ("moderate GR") ǫ = 10 −1 ("strong GR"). ![]() The experimental data are from Nagano and Watson's (2000) summary except for the data from the Hi-Res (monocular) results, which are taken from Abu-Zayyad et al. ![]() The Auger experiment should see such bursts every few years.Ĭomparison of bare magnetar theory to UHECR data. Such bursts of gravitational radiation should correlate with bursts of ultra-high energy particles. I show that the relativistic winds of newly born magnetars with khz initial spin rates, occurring in all normal galaxies, can accelerate ultrarelativistic light ions with an E^. ![]()
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