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Status of the Trinity PeV Neutrino Observatory

Fuente: arXiv

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Bibliographic Details
Main Authors:	Stepanoff, S., Otte, A. N., Bagheri, M., Barletta, A., Bergmann, D., Blose, J., Bogdan, J., Brown, A. M., Cedeno, L., Doro, M., Fedkevych, M., Gadamsetty, S., Giordano, F., Hao, C., Iyengar, V., Kieda, D., Lew, N., Mariotti, M., Onel, Y., O., D. A. Raudales, Castillo, L. Rojas, Ronemus, A., Menon, A., Mitra, A., Schapera, E., Solden, D., Song, N., Springer, W., Taboada, I., Tran, K., Wilcox, A., Zhang, A.
Format:	Preprint
Published:	2025
Subjects:	Instrumentation and Methods for Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena
Online Access:	Acceder al recurso
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_version_	1866912600146575360
author	Stepanoff, S. Otte, A. N. Bagheri, M. Barletta, A. Bergmann, D. Blose, J. Bogdan, J. Brown, A. M. Cedeno, L. Doro, M. Fedkevych, M. Gadamsetty, S. Giordano, F. Hao, C. Iyengar, V. Kieda, D. Lew, N. Mariotti, M. Onel, Y. O., D. A. Raudales Castillo, L. Rojas Ronemus, A. Menon, A. Mitra, A. Schapera, E. Solden, D. Song, N. Springer, W. Taboada, I. Tran, K. Wilcox, A. Zhang, A.
author_facet	Stepanoff, S. Otte, A. N. Bagheri, M. Barletta, A. Bergmann, D. Blose, J. Bogdan, J. Brown, A. M. Cedeno, L. Doro, M. Fedkevych, M. Gadamsetty, S. Giordano, F. Hao, C. Iyengar, V. Kieda, D. Lew, N. Mariotti, M. Onel, Y. O., D. A. Raudales Castillo, L. Rojas Ronemus, A. Menon, A. Mitra, A. Schapera, E. Solden, D. Song, N. Springer, W. Taboada, I. Tran, K. Wilcox, A. Zhang, A.
contents	The Trinity Neutrino Observatory aims to detect tau neutrinos in the energy range of 1 PeV to 10 EeV. We are developing the observatory in three stages. The first stage, known as the Trinity Demonstrator, was deployed in Fall 2023. The Demonstrator serves as a pathfinder for the full observatory and will inform the design of the first Trinity Telescope. We discuss the status and initial results of the Trinity Demonstrator. In 346 hours of observations with the Demonstrator, we do not identify a neutrino candidate event.
format	Preprint
id	arxiv_https___arxiv_org_abs_2509_18236
institution	arXiv
publishDate	2025
record_format	arxiv
spellingShingle	Status of the Trinity PeV Neutrino Observatory Stepanoff, S. Otte, A. N. Bagheri, M. Barletta, A. Bergmann, D. Blose, J. Bogdan, J. Brown, A. M. Cedeno, L. Doro, M. Fedkevych, M. Gadamsetty, S. Giordano, F. Hao, C. Iyengar, V. Kieda, D. Lew, N. Mariotti, M. Onel, Y. O., D. A. Raudales Castillo, L. Rojas Ronemus, A. Menon, A. Mitra, A. Schapera, E. Solden, D. Song, N. Springer, W. Taboada, I. Tran, K. Wilcox, A. Zhang, A. Instrumentation and Methods for Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena The Trinity Neutrino Observatory aims to detect tau neutrinos in the energy range of 1 PeV to 10 EeV. We are developing the observatory in three stages. The first stage, known as the Trinity Demonstrator, was deployed in Fall 2023. The Demonstrator serves as a pathfinder for the full observatory and will inform the design of the first Trinity Telescope. We discuss the status and initial results of the Trinity Demonstrator. In 346 hours of observations with the Demonstrator, we do not identify a neutrino candidate event.
title	Status of the Trinity PeV Neutrino Observatory
topic	Instrumentation and Methods for Astrophysics Astrophysics of Galaxies High Energy Astrophysical Phenomena
url	https://arxiv.org/abs/2509.18236