Using evolutionary algorithms to design antennas with greater sensitivity to ultrahigh energy neutrinos
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PhysRevD.108.102002.pdf
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Author
Rolla, J.Machtay, A.
Patton, A.
Banzhaf, W.
Connolly, A.
Debolt, R.
Deer, L.
Fahimi, E.
Ferstle, E.
Kuzma, P.
Pfendner, C.
Sipe, B.
Staats, K.
Wissel, S.A.
Affiliation
Biosphere 2, University of ArizonaIssue Date
2023-11-03
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American Physical SocietyCitation
J. Rolla, A. Machtay, A. Patton, W. Banzhaf, A. Connolly, R. Debolt, L. Deer, E. Fahimi, E. Ferstle, P. Kuzma, C. Pfendner, B. Sipe, K. Staats, and S. A. Wissel (GENETIS Collaboration). Phys. Rev. D 108, 102002 – Published 3 November 2023Journal
Physical Review DRights
© 2023 American Physical Society.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The Genetically Evolved NEutrino Telescopes for Improved Sensitivity project seeks to optimize detectors in physics for science outcomes in high-dimensional parameter spaces. In this project, we designed an antenna using a genetic algorithm with a science outcome directly as the sole figure of merit. This paper presents initial results on the improvement of an antenna design for in-ice neutrino detectors using the current Askaryan Radio Array (ARA) experiment as a baseline. By optimizing for the effective volume using the evolved antenna design in ARA, we improve upon ARA's simulated sensitivity to ultrahigh energy neutrinos by 11%, despite using limited parameters in this initial investigation. Future improvements will continue to increase the computational efficiency of the genetic algorithm and the complexity and fitness of the antenna designs. This work lays the foundation for continued research and development of methods to increase the sensitivity of detectors in physics and other fields in parameter spaces of high dimensionality. © 2023 American Physical Society.Note
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2470-0010Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1103/PhysRevD.108.102002