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A Search for Ultra-High Energy Neutrinos and Cosmic-Rays with ANITA-2The Antarctic Impulsive Transient Antenna

A Search for Ultra-High Energy Neutrinos and Cosmic-Rays with ANITA-2: The Antarctic Impulsive... [The Antarctic Impulsive Transient Antenna (ANITA) was conceived to be the most sensitive instrument for the detection of UHE neutrinos (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$E_{\nu }>10^{18}$$\end{document} eV) to date. A balloon-borne array of radio antennas, ANITA observes the Antarctic ice sheet and searches for the impulsive radio emission expected to arise when an UHE neutrino interacts in the ice.] http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png

A Search for Ultra-High Energy Neutrinos and Cosmic-Rays with ANITA-2The Antarctic Impulsive Transient Antenna

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Publisher
Springer Berlin Heidelberg
Copyright
© Springer-Verlag Berlin Heidelberg 2012
ISBN
978-3-642-30031-8
Pages
29 –53
DOI
10.1007/978-3-642-30032-5_4
Publisher site
See Chapter on Publisher Site

Abstract

[The Antarctic Impulsive Transient Antenna (ANITA) was conceived to be the most sensitive instrument for the detection of UHE neutrinos (\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$E_{\nu }>10^{18}$$\end{document} eV) to date. A balloon-borne array of radio antennas, ANITA observes the Antarctic ice sheet and searches for the impulsive radio emission expected to arise when an UHE neutrino interacts in the ice.]

Published: Jul 11, 2012

Keywords: Radio Emission; Trigger Threshold; Trigger Rate; Impulsive Signal; Antenna Ring

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