Indication of a composition anisotropy at energies above the ankle in the hybrid data of the Pierre Auger Observatory
ORAL
Abstract
A study testing for a cosmic ray primary mass composition anisotropy correlated with the galactic plane of the Milky Way is presented. The depth of airshower maximum, Xmax, from 14 years of hybrid data from the Pierre Auger Observatory is used as a mass sensitive parameter. The data are split to form two Xmax distributions, the on- and off-plane datasets using the arriving galactic latitude of each event. These are then compared using the Anderson-Darling 2-samples test to generate a Test Statistic describing how much the distributions differ.
A scan over half the data finds that a lower threshold energy of 1018.7 eV and an opening angle of 30° in galactic latitude produce the largest difference between the two datasets. These thresholds are set as a prescription for the remaining data and result in the on-plane distribution having a shallower mean and narrower width than the off-plane distribution, indicating that, on average, primary cosmic rays arriving from near-to the galactic plane have a higher mass than those arriving far from it. Monte-Carlo studies penalized to include all systematic effects conservatively estimate a post-trial significance of 3.3σ. Discussions on the possible interpretations and impacts on astrophysical models, if confirmed, will be included.
A scan over half the data finds that a lower threshold energy of 1018.7 eV and an opening angle of 30° in galactic latitude produce the largest difference between the two datasets. These thresholds are set as a prescription for the remaining data and result in the on-plane distribution having a shallower mean and narrower width than the off-plane distribution, indicating that, on average, primary cosmic rays arriving from near-to the galactic plane have a higher mass than those arriving far from it. Monte-Carlo studies penalized to include all systematic effects conservatively estimate a post-trial significance of 3.3σ. Discussions on the possible interpretations and impacts on astrophysical models, if confirmed, will be included.
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Publication: Astrophysics Journal publication in preparation
Presenters
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Eric W Mayotte
Colorado School of Mines
Authors
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Eric W Mayotte
Colorado School of Mines