Experimental Development Towards the BEACON Prototype Array and the Radio Neutrino Observatory in Greenland

The field of experimental ultra-high-energy (UHE) neutrino physics has seen significant expansion in the past decade, with ongoing developments towards new experiments such as the Beamforming Elevated Array for COsmic Neutrinos (BEACON) as well as the Radio Neutrino observatory in Greenland (RNO-G)....

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Main Author: Southall, Daniel John
Format: Text
Language:English
Published: The University of Chicago 2022
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Online Access:https://doi.org/10.6082/uchicago.5212
http://knowledge.uchicago.edu/record/5212
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spelling ftunichicagoknow:oai:uchicago.tind.io:5212 2024-09-15T18:09:36+00:00 Experimental Development Towards the BEACON Prototype Array and the Radio Neutrino Observatory in Greenland Southall, Daniel John 2022-12-16T19:05:55Z https://doi.org/10.6082/uchicago.5212 http://knowledge.uchicago.edu/record/5212 en eng The University of Chicago https://knowledge.uchicago.edu/record/5212/files/Southall_uchicago_0330D_16566.pdf doi:10.6082/uchicago.5212 http://knowledge.uchicago.edu/record/5212 http://knowledge.uchicago.edu/record/5212 Text 2022 ftunichicagoknow https://doi.org/10.6082/uchicago.5212 2024-08-05T14:08:09Z The field of experimental ultra-high-energy (UHE) neutrino physics has seen significant expansion in the past decade, with ongoing developments towards new experiments such as the Beamforming Elevated Array for COsmic Neutrinos (BEACON) as well as the Radio Neutrino observatory in Greenland (RNO-G). These experiments aim to probe production mechanisms by measuring the flux of astrophysical and cosmogenic UHE neutrinos, as well as to provide new information of neutrino cross sections at the highest energies. I discuss my role in the development, deployment, and data analysis efforts for the BEACON prototype array, which was installed at Barcroft Station in California in 2018. BEACON is designed to detect radio emission from upgoing air showers generated by UHE tau neutrino interactions in the Earth. This detection mechanism provides a measurement of the tau flavor flux of cosmic neutrinos. The BEACON prototype is at high elevation to maximize effective volume and uses a directional beamforming trigger to improve rejection of anthropogenic background noise at the trigger level. In discussion of BEACON I present details of the radio frequency environment observed by the prototype instrument, and categorize the types of events seen by the instrument, including a likely cosmic ray candidate event. In addition to BEACON I also discuss my work on RNO-G, which seeks to measure neutrinos above 10 PeV by exploiting the Askaryan effect in neutrino-induced cascades in ice. I present work towards a robust Monte Carlo simulation which was used in the early planning stages of RNO-G. I also discuss the RNO-G horizontally-polarized antenna design and outline the prototyping and development process from which they are a result. Text Greenland Knowledge@UChicago (University of Chicago)
institution Open Polar
collection Knowledge@UChicago (University of Chicago)
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language English
description The field of experimental ultra-high-energy (UHE) neutrino physics has seen significant expansion in the past decade, with ongoing developments towards new experiments such as the Beamforming Elevated Array for COsmic Neutrinos (BEACON) as well as the Radio Neutrino observatory in Greenland (RNO-G). These experiments aim to probe production mechanisms by measuring the flux of astrophysical and cosmogenic UHE neutrinos, as well as to provide new information of neutrino cross sections at the highest energies. I discuss my role in the development, deployment, and data analysis efforts for the BEACON prototype array, which was installed at Barcroft Station in California in 2018. BEACON is designed to detect radio emission from upgoing air showers generated by UHE tau neutrino interactions in the Earth. This detection mechanism provides a measurement of the tau flavor flux of cosmic neutrinos. The BEACON prototype is at high elevation to maximize effective volume and uses a directional beamforming trigger to improve rejection of anthropogenic background noise at the trigger level. In discussion of BEACON I present details of the radio frequency environment observed by the prototype instrument, and categorize the types of events seen by the instrument, including a likely cosmic ray candidate event. In addition to BEACON I also discuss my work on RNO-G, which seeks to measure neutrinos above 10 PeV by exploiting the Askaryan effect in neutrino-induced cascades in ice. I present work towards a robust Monte Carlo simulation which was used in the early planning stages of RNO-G. I also discuss the RNO-G horizontally-polarized antenna design and outline the prototyping and development process from which they are a result.
format Text
author Southall, Daniel John
spellingShingle Southall, Daniel John
Experimental Development Towards the BEACON Prototype Array and the Radio Neutrino Observatory in Greenland
author_facet Southall, Daniel John
author_sort Southall, Daniel John
title Experimental Development Towards the BEACON Prototype Array and the Radio Neutrino Observatory in Greenland
title_short Experimental Development Towards the BEACON Prototype Array and the Radio Neutrino Observatory in Greenland
title_full Experimental Development Towards the BEACON Prototype Array and the Radio Neutrino Observatory in Greenland
title_fullStr Experimental Development Towards the BEACON Prototype Array and the Radio Neutrino Observatory in Greenland
title_full_unstemmed Experimental Development Towards the BEACON Prototype Array and the Radio Neutrino Observatory in Greenland
title_sort experimental development towards the beacon prototype array and the radio neutrino observatory in greenland
publisher The University of Chicago
publishDate 2022
url https://doi.org/10.6082/uchicago.5212
http://knowledge.uchicago.edu/record/5212
genre Greenland
genre_facet Greenland
op_source http://knowledge.uchicago.edu/record/5212
op_relation https://knowledge.uchicago.edu/record/5212/files/Southall_uchicago_0330D_16566.pdf
doi:10.6082/uchicago.5212
http://knowledge.uchicago.edu/record/5212
op_doi https://doi.org/10.6082/uchicago.5212
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