Published November 12, 2012 | Version v1
Journal article

An ultra-high-energy-neutrino detector using rock salt and ice as detection media for radar method

  • 1. School of Medicine, Shimane University, Izumo-shi, Shimane 693-8501 (Japan)
  • 2. Department of Applied Science and Energy Engineering, School of Engineering, Tokai University, Hiratsuka-shi, Kanagawa 259-1292 (Japan)
  • 3. Faculty of Science and Technology, Seikei University, Musashino-shi, Tokyo 180-8633 (Japan)
  • 4. Graduate School of Science and Engineering, Tokyo Metropolitan University, 1-1 Minami-Ohsawa, Hachioji-shi, Tokyo 192-0397 (Japan)

Description

We had found radio-wave-reflection effect in rock salt for detection of an ultra-high energy neutrino (UHEν) which is generated in GZK processes in the universe. When an UHEν interacts with rock salt or ice as a detection medium, the energy converts to a thermal energy. Consequently, a temperature gives rise along an UHEν shower at the interaction location. The permittivity arises with respect to the temperature at ionization processes of the UHEν shower which is composed of hadronic and electromagnetic multiplication processes. The irregularity of the refractive index in the medium for radio wave rises to a reflection. The reflection effect with a long attenuation length of radio wave in rock salt and ice would yield a new method to detect UHEν. They could be used for detection media in which the UHEν interacts with. We could find a huge amount of rock salt or ice over 50 Gt in a natural rock salt formation or Antarctic ice sheet. Radio wave transmitted into the medium generated by a radar system could be reflected by the irregularity of the refractive index at the shower. Receiving the reflected radio wave yields information about the UHEν.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1484
Journal Issue
1
Journal Page Range
p. 409-411
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
Conference on origin of matter and evolution of galaxies 2011
Dates
14-17 Nov 2011
Place
Wako (Japan)

Optional Information

Notes
(c) 2012 American Institute of Physics