The Trinity-One PeV-Neutrino Telescope

Abstract: Following the Trinity Demonstrator, Trinity One will be the first of the 18 Cherenkov telescopes that make up the Trinity PeV-Neutrino Observatory. Located on Frisco Peak in Utah, Trinity One can observe 64\% of the sky, allowing it to detect potential neutrino point sources with unprecedented sensitivity, ranging from 1 PeV to 10 EeV. We outline the design of Trinity One, which features a 60 m$<sup>2$ light-collection surface and the ability to rotate in azimuth. It has a field of view measuring $5<sup>\circ$ by $60<sup>\circ$, which is equipped with a silicon photomultiplier camera with a resolution of $0.3<sup>\circ$. Utilizing the design of Trinity One, we present performance calculations in relation to various source classes.