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Title:Search for Anisotropy in the Ultra High Energy Cosmic Ray Spectrum using the Telescope Array Surface Detector
Authors:ID Abbasi, R.U. (Author)
ID Lundquist, Jon Paul (Author), et al.
Files:.pdf 1707.04967.pdf (169,05 KB)
MD5: D2AB3EAEE9DAF6A1A2911FF8449FBF88
 
Language:English
Work type:Not categorized
Typology:1.25 - Other Component Parts
Organization:UNG - University of Nova Gorica
Abstract:The Telescope Array (TA) experiment is located in the western desert of Utah, USA, and observes ultra high energy cosmic rays (UHECRs) in the Northern hemisphere. At the highest energies, E>10~EeV, the shape of cosmic ray energy spectrum may carry an imprint of the source density distribution along the line of sight different in different directions of the sky. In this study, we search for such directional variations in the shape of the energy spectrum using events observed with the Telescope Array's surface detector. We divide the TA field of view into two nearly equal-exposure regions: the "on-source" region which we define as ±30∘ of the supergalactic plane containing mostly nearby structures, and the complementary "off-source" region where the sources are further away on average. We compare the UHECR spectra in these regions by fitting them to the broken power law and comparing the resulting parameters. We find that the off-source spectrum has an earlier break at highest energies. The chance probability to obtain such or larger difference in statistically equivalent distributions is estimated as 6.2±1.1×10−4 (3.2σ) by a Monte-Carlo simulation. The observed difference in spectra is in a reasonable quantitative agreement with a simplified model that assumes that the UHECR sources trace the galaxy distribution from the 2MRS catalogue, primary particles are protons and the magnetic deflections can be neglected.
Keywords:cosmic radiation: UHE, detector: surface, cosmic radiation: spectrum, cosmic radiation: energy spectrum, deflection: magnetic, numerical calculations: Monte Carlo, anisotropy
Publication version:Preprint, working version of publication, not peer-reviewed
Year of publishing:2017
Number of pages:17
Numbering:1707.04967v3
PID:20.500.12556/RUNG-5154-32bcf13b-24a0-5b2b-d07d-776266619e28 New window
COBISS.SI-ID:12841219 New window
NUK URN:URN:SI:UNG:REP:PBVD0NXF
Publication date in RUNG:27.04.2020
Views:2794
Downloads:98
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Record is a part of a journal

Title:arXiv
Year of publishing:2017

Licences

License:CC BY-NC-ND 4.0, Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International
Link:http://creativecommons.org/licenses/by-nc-nd/4.0/
Description:The most restrictive Creative Commons license. This only allows people to download and share the work for no commercial gain and for no other purposes.
Licensing start date:27.04.2020

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