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A Search for Ultra-High Energy Neutrinos and Cosmic-Rays with ANITA-2Event Simulation

A Search for Ultra-High Energy Neutrinos and Cosmic-Rays with ANITA-2: Event Simulation [The default UHE neutrino Monte-Carlo simulation used by ANITA is icemc, written by Amy Connolly and others [1]. This simulation generates neutrinos from a given energy spectrum and propagates them through the Earth. Upon a simulated neutrino interacting in ice (or other desired medium), icemc generates and propagates the resultant Askaryan radiation. Icemc also simulates the ANITA-2 payload, with the response to radio signals, a trigger simulation and thermal noise generation. Finally, icemc contains an array of editable options, providing control over a range of aspects from the UHE neutrino energy spectrum through to ANITA trigger banding and logic. A schematic of the steps required for a simulation that will inform us of ANITA’s sensitivity to UHE neutrinos is given in Fig. 5.1.] http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png

A Search for Ultra-High Energy Neutrinos and Cosmic-Rays with ANITA-2Event Simulation

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Publisher
Springer Berlin Heidelberg
Copyright
© Springer-Verlag Berlin Heidelberg 2012
ISBN
978-3-642-30031-8
Pages
55 –64
DOI
10.1007/978-3-642-30032-5_5
Publisher site
See Chapter on Publisher Site

Abstract

[The default UHE neutrino Monte-Carlo simulation used by ANITA is icemc, written by Amy Connolly and others [1]. This simulation generates neutrinos from a given energy spectrum and propagates them through the Earth. Upon a simulated neutrino interacting in ice (or other desired medium), icemc generates and propagates the resultant Askaryan radiation. Icemc also simulates the ANITA-2 payload, with the response to radio signals, a trigger simulation and thermal noise generation. Finally, icemc contains an array of editable options, providing control over a range of aspects from the UHE neutrino energy spectrum through to ANITA trigger banding and logic. A schematic of the steps required for a simulation that will inform us of ANITA’s sensitivity to UHE neutrinos is given in Fig. 5.1.]

Published: Jul 11, 2012

Keywords: Tunnel Diode; Picosecond Pulser; Trigger Threshold; Signal Chain; Trigger Rate

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