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https://hdl.handle.net/2440/106105
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Type: | Journal article |
Title: | Search for sources of high-energy neutrons with four years of data from the IceTop detector |
Author: | Aartsen, M. Abraham, K. Ackermann, M. Adams, J. Aguilar, J. Ahlers, M. Ahrens, M. Altmann, D. Andeen, K. Anderson, T. Ansseau, I. Anton, G. Archinger, M. Argüelles, C. Auffenberg, J. Axani, S. Bai, X. Barwick, S. Baum, V. Bay, R. et al. |
Citation: | The Astrophysical Journal: an international review of astronomy and astronomical physics, 2016; 830(2):1-12 |
Publisher: | IOP Publishing |
Issue Date: | 2016 |
ISSN: | 0004-637X 1538-4357 |
Statement of Responsibility: | M.G. Aartsen … S. Robertson … A. Wallace … B.J. Whelan … [et al.] (The ICECUBE Collaboration) |
Abstract: | IceTop is an air-shower array located on the Antarctic ice sheet at the geographic South Pole. IceTop can detect an astrophysical flux of neutrons from Galactic sources as an excess of cosmic-ray air showers arriving from the source direction. Neutrons are undeflected by the Galactic magnetic field and can typically travel 10 (E/PeV) pc before decay. Two searches are performed using 4 yr of the IceTop data set to look for a statistically significant excess of events with energies above 10 PeV (10¹⁶ eV) arriving within a small solid angle. The all-sky search method covers from −90° to approximately −50° in declination. No significant excess is found. A targeted search is also performed, looking for significant correlation with candidate sources in different target sets. This search uses a higher-energy cut (100 PeV) since most target objects lie beyond 1 kpc. The target sets include pulsars with confirmed TeV energy photon fluxes and high-mass X-ray binaries. No significant correlation is found for any target set. Flux upper limits are determined for both searches, which can constrain Galactic neutron sources and production scenarios. |
Keywords: | Astroparticle physics; cosmic rays; methods: data analysis |
Rights: | © 2016. The American Astronomical Society. All rights reserved. |
DOI: | 10.3847/0004-637X/830/2/129 |
Grant ID: | ARC |
Published version: | http://dx.doi.org/10.3847/0004-637X/830/2/129 |
Appears in Collections: | Aurora harvest 3 Chemistry and Physics publications |
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