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arXiv · astro-ph/0204419

Nearby quasar remnants and ultra-high energy cosmic rays

Diego F. Torres·Elihu Boldt·Timothy Hamilton·Michael Loewenstein
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Abstract

As recently suggested, nearby quasar remnants are plausible sites of black-hole based compact dynamos that could be capable of accelerating ultra-high energy cosmic rays (UHECRs). In such a model, UHECRs would originate at the nuclei of nearby dead quasars, those in which the putative underlying supermassive black holes are suitably spun-up. Based on galactic optical luminosity, morphological type, and redshift, we have compiled a small sample of nearby objects selected to be highly luminous, bulge-dominated galaxies, likely quasar remnants. The sky coordinates of these galaxies were then correlated with the arrival directions of cosmic rays detected at energies $> 40$ EeV. An apparently significant correlation appears in our data. This correlation appears at closer angular scales than those expected when taking into account the deflection caused by typically assumed IGM or galactic magnetic fields over a charged particle trajectory. Possible scenarios producing this effect are discussed, as is the astrophysics of the quasar remnant candidates. We suggest that quasar remnants be also taken into account in the forthcoming detailed search for correlations using data from the Auger Observatory.

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Diego F. Torres, Elihu Boldt, Timothy Hamilton, Michael Loewenstein. 2002-05-09. Nearby quasar remnants and ultra-high energy cosmic rays. https://doi.org/10.1103/physrevd.66.023001

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