Probing Ultralight Dark Matter at the Mega-Planck Scale with the Thorium Nuclear Clock

Fuente: arXiv
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Autori principali: Arakawa, Jason, Doyle, Jack F., Fuchs, Elina, Higgins, Jacob S., Kirk, Fiona, Li, Kai, Ooi, Tian, Perez, Gilad, Ratzinger, Wolfram, Safronova, Marianna S., Schumm, Thorsten, Ye, Jun, Zhang, Chuankun
Natura: Preprint
Pubblicazione: 2026
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author Arakawa, Jason
Doyle, Jack F.
Fuchs, Elina
Higgins, Jacob S.
Kirk, Fiona
Li, Kai
Ooi, Tian
Perez, Gilad
Ratzinger, Wolfram
Safronova, Marianna S.
Schumm, Thorsten
Ye, Jun
Zhang, Chuankun
author_facet Arakawa, Jason
Doyle, Jack F.
Fuchs, Elina
Higgins, Jacob S.
Kirk, Fiona
Li, Kai
Ooi, Tian
Perez, Gilad
Ratzinger, Wolfram
Safronova, Marianna S.
Schumm, Thorsten
Ye, Jun
Zhang, Chuankun
contents Ultralight dark matter is expected to induce oscillations of nuclear parameters. These oscillations are characterized by extremely weak couplings or high suppression scales, with the Planck scale - the characteristic scale of quantum gravity - serving as a natural benchmark. Probing this phenomenon requires systems with exceptional sensitivity to shifts in nuclear energies. The uniquely low-energy nuclear isomeric transition in ${}^{229}$Th provides such sensitivity: it directly probes the nuclear interaction and, owing to a near cancellation between electromagnetic and nuclear contributions, its response to changes in nuclear structure is greatly amplified. We devise and perform a new type of ultrasensitive search for dark matter which uses the precision nuclear spectroscopy at JILA to set the strongest bounds in the mass range $10^{-21}\,{\rm eV} \lesssim m_{\rm DM} \lesssim 10^{-19}\,{\rm eV}$. Our results probe effective interaction scales exceeding $10^6$ times the Planck scale (the Mega-Planck scale) and establish the ${}^{229}$Th system as the leading probe of dark matter couplings to the nuclear sector.
format Preprint
id arxiv_https___arxiv_org_abs_2602_16804
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Probing Ultralight Dark Matter at the Mega-Planck Scale with the Thorium Nuclear Clock
Arakawa, Jason
Doyle, Jack F.
Fuchs, Elina
Higgins, Jacob S.
Kirk, Fiona
Li, Kai
Ooi, Tian
Perez, Gilad
Ratzinger, Wolfram
Safronova, Marianna S.
Schumm, Thorsten
Ye, Jun
Zhang, Chuankun
High Energy Physics - Phenomenology
Nuclear Experiment
Atomic Physics
Ultralight dark matter is expected to induce oscillations of nuclear parameters. These oscillations are characterized by extremely weak couplings or high suppression scales, with the Planck scale - the characteristic scale of quantum gravity - serving as a natural benchmark. Probing this phenomenon requires systems with exceptional sensitivity to shifts in nuclear energies. The uniquely low-energy nuclear isomeric transition in ${}^{229}$Th provides such sensitivity: it directly probes the nuclear interaction and, owing to a near cancellation between electromagnetic and nuclear contributions, its response to changes in nuclear structure is greatly amplified. We devise and perform a new type of ultrasensitive search for dark matter which uses the precision nuclear spectroscopy at JILA to set the strongest bounds in the mass range $10^{-21}\,{\rm eV} \lesssim m_{\rm DM} \lesssim 10^{-19}\,{\rm eV}$. Our results probe effective interaction scales exceeding $10^6$ times the Planck scale (the Mega-Planck scale) and establish the ${}^{229}$Th system as the leading probe of dark matter couplings to the nuclear sector.
title Probing Ultralight Dark Matter at the Mega-Planck Scale with the Thorium Nuclear Clock
topic High Energy Physics - Phenomenology
Nuclear Experiment
Atomic Physics
url https://arxiv.org/abs/2602.16804