The Trinity-One PeV-Neutrino Telescope

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 m2 light-collection surface and the ability to rotate in azimuth. It has a field of view measuring 5 deg by 60 deg, which is equipped with a silicon photomultiplier camera with a resolution of 0.3 deg. Utilizing the design of Trinity One, we present performance calculations in relation to various source classes.

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Publication Details

Published
2025-09-24
DOI
https://doi.org/10.22323/1.501.1136
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
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article

The Trinity-One PeV-Neutrino Telescope

A. N. Otte
Astrophysics and Cosmic Phenomena
article

The Trinity-One PeV-Neutrino Telescope

A. N. Otte
article en

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 m2 light-collection surface and the ability to rotate in azimuth. It has a field of view measuring 5 deg by 60 deg, which is equipped with a silicon photomultiplier camera with a resolution of 0.3 deg. Utilizing the design of Trinity One, we present performance calculations in relation to various source classes.

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Astrophysics and Cosmic Phenomena
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The Trinity-One PeV-Neutrino Telescope — A. N. Otte · (2025) | TGRS Research Map | TGRS