Search for PeVatrons at the Galactic Center using a radio air-shower array at the South Pole

• Published in: The European Physical Journal C
• Main Authors: Balagopal V., A., Haungs, A., Huege, T., Schröder, F. G.
• Format: Article in Journal/Newspaper
• Language: English
• Published: Springer Science and Business Media LLC 2018
• Subjects: Physics and Astronomy (miscellaneous); Engineering (miscellaneous); South Pole; South pole
• Online Access: http://dx.doi.org/10.1140/epjc/s10052-018-5537-2; https://link.springer.com/article/10.1140/epjc/s10052-018-5537-2/fulltext.html; https://link.springer.com/content/pdf/10.1140/epjc/s10052-018-5537-2.pdf

Abstract The South Pole, which hosts the IceCube Neutrino Observatory, has a complete and around-the-clock exposure to the Galactic Center. Hence, it is an ideal location to search for gamma rays of PeV energy coming from the Galactic Center. However, it is hard to detect air showers initiated by these gamma rays using cosmic-ray particle detectors due to the low elevation of the Galactic Center. The use of antennas to measure the radio footprint of these air showers will help in this case, and would allow for a 24/7 operation time. So far, only air showers with energies well above $$10^{16}$$ 10 16 eV have been detected with the radio technique. Thus, the energy threshold has to be lowered for the detection of gamma-ray showers of PeV energy. This can be achieved by optimizing the frequency band in order to obtain a higher level of signal-to-noise ratio. With such an approach, PeV gamma-ray showers with high inclination can be measured at the South Pole.