Experimental tests of sub-surface reflectors as an explanation for the ANITA anomalous events
Creators
- 1. Department of Physics, Enrico Fermi Institute, Kavli Institute for Cosmological Physics, University of Chicago, Chicago IL 60637 (United States)
- 2. Department of Physics and Astronomy, University of Kansas, Lawrence, KS 66045 (United States)
- 3. Department of Physics, Ohio State University, Columbus, OH 43210 (United States)
- 4. Department of Physics and Astronomy, University College London, London (United Kingdom)
- 5. Department of Physics and McDonnell Center for the Space Sciences, Washington University in St. Louis, St. Louis, MO 63130 (United States)
- 6. Department of Physics, University of Delaware, Newark, DE 19716 (United States)
- 7. Department of Physics, Indian Institute of Technology, Kanpur, Uttar Pradesh 208016 (India)
- 8. Department of Physics and Astronomy, University of Hawaii, Manoa, HI 96822 (United States)
- 9. Department of Physics, Graduate Institute of Astrophysics, & Leung Center for Cosmology and Particle Astrophysics, National Taiwan University, Taipei, Taiwan (China)
- 10. Department of Physics and Astronomy, University of California, Los Angeles, Los Angeles, CA 90095 (United States)
Description
The balloon-borne ANITA [1] experiment is designed to detect ultra-high energy neutrinos via radio emissions produced by in-ice showers. Although initially purposed for interactions within the Antarctic ice sheet, ANITA also demonstrated the ability to self-trigger on radio emissions from ultra-high energy charged cosmic rays [2] (CR) interacting in the Earth's atmosphere. For showers produced above the Antarctic ice sheet, reflection of the down-coming radio signals at the Antarctic surface should result in a polarity inversion prior to subsequent observation at the ∼35–40 km altitude ANITA gondola. Based on data taken during the ANITA-1 and ANITA-3 flights, ANITA published two anomalous instances of upcoming cosmic-rays with measured polarity opposite the remaining sample of ∼50 UHECR signals [3, 4]. The steep observed upwards incidence angles (25–30 degrees relative to the horizontal) require non-Standard Model physics if these events are due to in-ice neutrino interactions, as the Standard Model cross-section would otherwise prohibit neutrinos from penetrating the long required chord of Earth. Shoemaker et al. [5] posit that glaciological effects may explain the steep observed anomalous events. We herein consider the scenarios offered by Shoemaker et al. and find them to be disfavored by extant ANITA and HiCal experimental data. We note that the recent report of four additional near-horizon anomalous ANITA-4 events [6], at >3σ significance, are incompatible with their model, which requires significant signal transmission into the ice. (paper)
Availability note (English)
Available from http://dx.doi.org/10.1088/1475-7516/2021/04/016Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Cosmology and Astroparticle Physics
- Journal Volume
- 2021
- Journal Issue
- 04
- Journal Page Range
- [24 p.]
- ISSN
- 1475-7516
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 53099828
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC RADIATION; CROSS SECTIONS; ICE; NEUTRINOS
- Descriptors DEC
- ELEMENTARY PARTICLES; FERMIONS; IONIZING RADIATIONS; LEPTONS; MASSLESS PARTICLES; RADIATIONS