Progress in ultra high energy neutrino experiments using radio techniques

Journal Article · Thu May 23 00:00:00 EDT 2013 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.4807368· OSTI ID:22118517

Jiali, Liu ^[1]; Tiedt, Douglas ^[2]

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1. Physics department, Kunming University, Kunming, 650214 (China)
2. Physics department, South Dakota School of Mines and Technology, Rapid City, SD, 57701-3995 (United States)

Studying the source of Ultra High Energy Cosmic Ray (UHECR) can provide important clues on the understanding of UHE particle physics, astrophysics, and other extremely energetic phenomena in the universe. However, charged CR particles are deflected by magnetic fields and can not point back to the source. Furthermore, UHECR charged particles above the Greisen-Zatsepin-Kuzmin (GZK) cutoff (about 5 Multiplication-Sign 10{sup 19} eV) suffer severe energy loss due to the interaction with the Cosmic Microwave Background Radiation (CMBR). Consequently almost all the information carried by CR particles about their origin is lost. Neutrinos, which are neutral particles and have extremely weak interactions with other materials can arrive at the earth without deflection and absorption. Therefore UHE neutrinos can be traced back to the place where they are produced. Due to their weak interaction and ultra high energies (thus extremely low flux) the detection of UHE neutrinos requires a large collecting area and massive amounts of material. Cherenkov detection at radio frequency, which has long attenuation lengths and can travel freely in natural dense medium (ice, rock and salt et al), can fulfill the detection requirement. Many UHE neutrino experiments are being performed by radio techniques using natural ice, lunar, and salt as detection mediums. These experiments have obtained much data about radio production, propagation and detection, and the upper limit of UHE neutrino flux.

• OSTI ID: 22118517
• Journal Information: AIP Conference Proceedings, Vol. 1534, Issue 1; Conference: CETUP 2012: Workshop on dark matter, unification and neutrino physics, Lead-Deadwood, SD (United States), 10 Jul - 1 Aug 2012; Other Information: (c) 2013 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY
79 ASTROPHYSICS
COSMOLOGY AND ASTRONOMY
ABSORPTION
ASTROPHYSICS
ATTENUATION
CHARGED PARTICLES
CHERENKOV COUNTERS
COSMIC NEUTRINOS
COSMIC RAY DETECTION
COSMIC RAY PROPAGATION
COSMIC RAY SOURCES
ENERGY LOSSES
ICE
INTERSTELLAR MAGNETIC FIELDS
MULTIPARTICLE SPECTROMETERS
NEUTRAL PARTICLES
NEUTRINO DETECTION
PARTICLE IDENTIFICATION
RADIOWAVE RADIATION
RELICT RADIATION
UNIVERSE
WEAK INTERACTIONS