Development toward a ground-based interferometric phased array for radio detection of high energy neutrinos

  • J. Avva
  • , K. Bechtol
  • , T. Chesebro
  • , L. Cremonesi
  • , C. Deaconu
  • , A. Gupta
  • , A. Ludwig
  • , W. Messino
  • , C. Miki
  • , R. Nichol
  • , E. Oberla
  • , M. Ransom
  • , A. Romero-Wolf
  • , D. Saltzberg
  • , C. Schlupf
  • , N. Shipp
  • , G. Varner
  • , A. G. Vieregg
  • , S. A. Wissel

Research output: Contribution to journalArticlepeer-review

13 Scopus citations

Abstract

The in-ice radio interferometric phased array technique for detection of high energy neutrinos looks for Askaryan emission from neutrinos interacting in large volumes of glacial ice, and is being developed as a way to achieve a low energy threshold and a large effective volume at high energies. The technique is based on coherently summing the impulsive Askaryan signal from multiple antennas, which increases the signal-to-noise ratio for weak signals. We report here on measurements and a simulation of thermal noise correlations between nearby antennas, beamforming of impulsive signals, and a measurement of the expected improvement in trigger efficiency through the phased array technique. We also discuss the noise environment observed with an analog phased array at Summit Station, Greenland, a possible site for an interferometric phased array for radio detection of high energy neutrinos.

Original languageEnglish (US)
Pages (from-to)46-55
Number of pages10
JournalNuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Volume869
DOIs
StatePublished - Oct 11 2017

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Instrumentation

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