TY - JOUR
T1 - The Beamforming Elevated Array for COsmic Neutrinos (BEACON)
T2 - 9th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities, ARENA 2022
AU - Zeolla, Andrew
AU - Alvarez-Muñiz, J.
AU - Cummings, A.
AU - Curtis-Ginsberg, Z.
AU - Deaconu, C.
AU - Decoene, V.
AU - Hendrick, A.
AU - Hughes, K.
AU - Krebs, R.
AU - Ludwig, A.
AU - Mulrey, K.
AU - Oberla, E.
AU - Prohira, S.
AU - Rodrigues de Carvalho, W.
AU - Rodriguez, A.
AU - Romero-Wolf, A.
AU - Schoorlemmer, H.
AU - Southall, D.
AU - Vieregg, A. G.
AU - Wissel, S. A.
AU - Zas, E.
N1 - Publisher Copyright:
© Copyright owned by the author(s) under the terms of the Creative Commons.
PY - 2023/10/25
Y1 - 2023/10/25
N2 - When ultrahigh energy tau neutrinos skim the Earth, they can generate tau leptons that then decay in the atmosphere, forming upgoing extensive air showers. The Beamforming Elevated Array for COsmic Neutrinos (BEACON) is a novel detector concept that utilizes a mountaintop radio interferometer to search for the radio emission due to these extensive air showers. The prototype, located at the White Mountain Research Station in California, consists of 4 custom crossed-dipole antennas operating in the 30-80 MHz range and uses a directional interferometric trigger to achieve reduced thresholds and background rejection. The prototype will first be used to detect extensive air showers from down-going cosmic rays to validate the detector model. In this talk, we give an overview of the BEACON concept and the status of its prototype. We also discuss the ongoing cosmic ray search which utilizes both data analysis and simulation.
AB - When ultrahigh energy tau neutrinos skim the Earth, they can generate tau leptons that then decay in the atmosphere, forming upgoing extensive air showers. The Beamforming Elevated Array for COsmic Neutrinos (BEACON) is a novel detector concept that utilizes a mountaintop radio interferometer to search for the radio emission due to these extensive air showers. The prototype, located at the White Mountain Research Station in California, consists of 4 custom crossed-dipole antennas operating in the 30-80 MHz range and uses a directional interferometric trigger to achieve reduced thresholds and background rejection. The prototype will first be used to detect extensive air showers from down-going cosmic rays to validate the detector model. In this talk, we give an overview of the BEACON concept and the status of its prototype. We also discuss the ongoing cosmic ray search which utilizes both data analysis and simulation.
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M3 - Conference article
AN - SCOPUS:85179139210
SN - 1824-8039
VL - 424
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 023
Y2 - 7 June 2022 through 10 June 2022
ER -