Cosmogenic photons as a test of ultra-high energy cosmic ray composition

Details Cosmogenic photons as a test of ultra-high energy cosmic ray composition Cosmogenic photons as a test of ultra-high energy cosmic ray composition

2010-07-08

arxiv.org/abs/1007.1306v1

Astropart.Phys.34:340-343,2011

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

4 pages, 2 figures

Scientific paper

10.1016/j.astropartphys.2010.09.

Although recent measurements of the shower profiles of ultra-high energy cosmic rays suggest that they are largely initiated by heavy nuclei, such conclusions rely on hadronic interaction models which have large uncertainties. We investigate an alternative test of cosmic ray composition which is based on the observation of ultra-high energy photons produced through cosmic ray interactions with diffuse low energy photon backgrounds during intergalactic propagation. We show that if the ultra-high energy cosmic rays are dominated by heavy nuclei, the flux of these photons is suppressed by approximately an order of magnitude relative to the proton-dominated case. Future observations by the Pierre Auger Observatory may be able to use this observable to constrain the composition of the primaries, thus providing an important cross-check of hadronic interaction models.

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