Evolving Antennas for Ultra-High Energy Neutrino Detection
Julie Rolla, Dean Arakaki, Maximilian Clowdus, Amy Connolly, Ryan, Debolt, Leo Deer, Ethan Fahimi, Eliot Ferstl, Suren Gourapura, Corey Harris,, Luke Letwin, Alex Machtay, Alex Patton, Carl Pfendner, Cade Sbrocco, Tom, Sinha, Ben Sipe, Kai Staats, Jacob Trevithick

TL;DR
This paper presents the development of genetic algorithms to design more sensitive antennas for ultra-high energy neutrino detection, aiming to significantly improve detection capabilities in astrophysics.
Contribution
It introduces the first use of genetic algorithms with physics-based fitness scores to optimize antenna designs for neutrino detection, advancing astrophysical instrumentation.
Findings
Antennas designed via genetic algorithms show over 2x improvement in sensitivity.
The approach integrates simulation tools like XFdtd and neutrino experiment models.
Initial prototypes are planned for deployment in ice for testing.
Abstract
Evolutionary algorithms are a type of artificial intelligence that utilize principles of evolution to efficiently determine solutions to defined problems. These algorithms are particularly powerful at finding solutions that are too complex to solve with traditional techniques and at improving solutions found with simplified methods. The GENETIS collaboration is developing genetic algorithms to design antennas that are more sensitive to ultra high energy neutrino induced radio pulses than current detectors. Improving antenna sensitivity is critical because UHE neutrinos are rare and require massive detector volumes with stations dispersed over hundreds of km squared. The GENETIS algorithm evolves antenna designs using simulated neutrino sensitivity as a measure of fitness by integrating with XFdtd, a finite difference time domain modeling program, and with simulations of neutrino…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Radio Astronomy Observations and Technology · Neutrino Physics Research
