Observation of the Askaryan Effect

Technical Report · Mon Oct 11 04:00:00 EDT 2004

DOI:https://doi.org/10.2172/839956· OSTI ID:839956

Saltzberg, D ^[1]

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1. SLAC

We present direct experimental evidence for the charge excess in high energy particle showers and corresponding radio emission predicted nearly 40 years ago by Askaryan. We directed picosecond pulses of GeV bremsstrahlung photons at the SLAC Final Focus Test Beam into a 3.5 ton silica sand target, producing electromagnetic showers several meters long. A series of antennas spanning 0.3 to 6 GHz detected strong, sub-nanosecond radio frequency pulses produced by the showers. Measurements of the polarization, coherence, timing, field strength vs. shower depth, and field strength vs. frequency are completely consistent with predictions. We also show the emission peaks at the Cherenkov angle in sand. These measurements thus provide strong support for experiments designed to detect high energy cosmic rays such as neutrinos via coherent radio emission from their cascades in dense dielectric media.

• Research Organization: Stanford Linear Accelerator Center (SLAC), Menlo Park, CA
• Sponsoring Organization: SC
• DOE Contract Number: AC02-76SF00515
• OSTI ID: 839956
• Report Number(s): SLAC-PUB-10802
• Country of Publication: United States
• Language: English

Related Subjects

36 MATERIALS SCIENCE
43 PARTICLE ACCELERATORS
ANTENNAS
BREMSSTRAHLUNG
DIELECTRIC MATERIALS
METERS
NEUTRINOS
PHOTONS
POLARIZATION
SAND
SILICA
STANFORD LINEAR ACCELERATOR CENTER