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Main Author: Krishnan, Tanvi
Format: Preprint
Published: 2025
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Online Access:https://arxiv.org/abs/2507.12316
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author Krishnan, Tanvi
author_facet Krishnan, Tanvi
contents In order to develop a consistent quantum theory of gravity, we must understand the nature of spacetime at the Planck scale. In particular if it exhibits quantum fluctuations, they may cause propagating particles to evolve in an apparently non-unitary manner. Neutrinos, which interact only via the weak force and gravity, maintain quantum coherence while propagating over large distances. Thus, neutrino oscillations serve as a precise interferometer to search for Planck-scale fluctuations of spacetime. The IceCube Neutrino Observatory is the world's largest neutrino telescope, located in the Antarctic icecap. We search the data on atmospheric neutrinos detected by IceCube in the energy range 0.5-100 TeV to test for neutrino decoherence. In this contribution, we present the sensitivity of the analysis, which shows significant improvement compared to previous IceCube results as a result of improved reconstruction and a larger sample of events.
format Preprint
id arxiv_https___arxiv_org_abs_2507_12316
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Search for Quantum Decoherence with 10.7 years of atmospheric $ν_μ$ events in IceCube
Krishnan, Tanvi
High Energy Astrophysical Phenomena
In order to develop a consistent quantum theory of gravity, we must understand the nature of spacetime at the Planck scale. In particular if it exhibits quantum fluctuations, they may cause propagating particles to evolve in an apparently non-unitary manner. Neutrinos, which interact only via the weak force and gravity, maintain quantum coherence while propagating over large distances. Thus, neutrino oscillations serve as a precise interferometer to search for Planck-scale fluctuations of spacetime. The IceCube Neutrino Observatory is the world's largest neutrino telescope, located in the Antarctic icecap. We search the data on atmospheric neutrinos detected by IceCube in the energy range 0.5-100 TeV to test for neutrino decoherence. In this contribution, we present the sensitivity of the analysis, which shows significant improvement compared to previous IceCube results as a result of improved reconstruction and a larger sample of events.
title Search for Quantum Decoherence with 10.7 years of atmospheric $ν_μ$ events in IceCube
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2507.12316