Published October 20, 2016 | Version v1
Journal article

SEARCH FOR SOURCES OF HIGH-ENERGY NEUTRONS WITH FOUR YEARS OF DATA FROM THE ICETOP DETECTOR

  • 1. Department of Physics, University of Adelaide, Adelaide, 5005 (Australia)
  • 2. Physik-department, Technische Universität München, D-85748 Garching (Germany)
  • 3. DESY, D-15735 Zeuthen (Germany)
  • 4. Department of Physics and Astronomy, University of Canterbury, Private Bag 4800, Christchurch (New Zealand)
  • 5. Université Libre de Bruxelles, Science Faculty CP230, B-1050 Brussels (Belgium)
  • 6. Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin, Madison, WI 53706 (United States)
  • 7. Oskar Klein Centre and Department of Physics, Stockholm University, SE-10691 Stockholm (Sweden)
  • 8. Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, D-91058 Erlangen (Germany)
  • 9. Department of Physics, Marquette University, Milwaukee, WI 53201 (United States)
  • 10. Department of Physics, Pennsylvania State University, University Park, PA 16802 (United States)
  • 11. Institute of Physics, University of Mainz, Staudinger Weg 7, D-55099 Mainz (Germany)
  • 12. Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139 (United States)
  • 13. III. Physikalisches Institut, RWTH Aachen University, D-52056 Aachen (Germany)
  • 14. Physics Department, South Dakota School of Mines and Technology, Rapid City, SD 57701 (United States)
  • 15. Department of Physics and Astronomy, University of California, Irvine, CA 92697 (United States)
  • 16. Department of Physics, University of California, Berkeley, CA 94720 (United States)

Description

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.

Availability note (English)

Available from http://dx.doi.org/10.3847/0004-637X/830/2/129

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
830
Journal Issue
2
Journal Page Range
[12 p.]
ISSN
0004-637X
CODEN
ASJOAB

Optional Information

Collaborations
IceCube Collaboration