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A Search for Ultra-High Energy Neutrinos and Cosmic-Rays with ANITA-2ANITA-2 Data Analysis

A Search for Ultra-High Energy Neutrinos and Cosmic-Rays with ANITA-2: ANITA-2 Data Analysis [During its flight ANITA-2 recorded \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${\sim }21.4$$\end{document} million RF triggered events. Simulations of ANITA-2 inform us that the experiment was likely to see very few neutrino-induced signals, with typical estimates in the range \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$O$$\end{document}(0.01–1) events, depending on the neutrino flux model used. Meanwhile, the number of cosmic-rays that triggered ANITA-2 is expected to be lower than the 16 observed by ANITA-1 due to modifications in the trigger scheme used.] http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png

A Search for Ultra-High Energy Neutrinos and Cosmic-Rays with ANITA-2ANITA-2 Data Analysis

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References (1)

Publisher
Springer Berlin Heidelberg
Copyright
© Springer-Verlag Berlin Heidelberg 2012
ISBN
978-3-642-30031-8
Pages
65 –105
DOI
10.1007/978-3-642-30032-5_6
Publisher site
See Chapter on Publisher Site

Abstract

[During its flight ANITA-2 recorded \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${\sim }21.4$$\end{document} million RF triggered events. Simulations of ANITA-2 inform us that the experiment was likely to see very few neutrino-induced signals, with typical estimates in the range \documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$O$$\end{document}(0.01–1) events, depending on the neutrino flux model used. Meanwhile, the number of cosmic-rays that triggered ANITA-2 is expected to be lower than the 16 observed by ANITA-1 due to modifications in the trigger scheme used.]

Published: Jul 11, 2012

Keywords: Continuous Wave; Thermal Noise; Interferometric Image; Thermal Background; Minimum Bias Event

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