The ratio of branching fractions , where is an electron or muon, is measured using a Belle II data sample with an integrated luminosity of at the SuperKEKB asymmetric-energy collider. Data is collected at the resonance, and one meson in the decay is fully reconstructed in hadronic decay modes. The accompanying signal meson is reconstructed as using leptonic decays. The normalization decay, , produces the same observable final-state particles. The ratio of branching fractions is extracted in a simultaneous fit to two signal-discriminating variables in both channels and yields . This result is consistent with the current world average and with Standard Model predictions. Published by the American Physical Society2024
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This content will become publicly available on November 1, 2025
Resonant conversion of axion dark radiation into terahertz electromagnetic radiation in a neutron star magnetosphere
In the strong magnetic field of a neutron star’s magnetosphere, axions coupled to electromagnetism develop a nonzero probability to convert into photons. Past studies have revealed that the axion-photon conversion can be resonantly enhanced. We recognize that the axion-photon resonance admits two parametrically distinct resonant solutions, which we call the mass-matched resonance and the Euler-Heisenberg assisted resonance. The mass-matched resonance occurs at a point in the magnetosphere where the radially-varying plasma frequency crosses the axion mass . The Euler-Heisenberg assisted resonance occurs where the axion energy satisfies . This second resonance is made possible though the strong background magnetic field , as well as the nonzero Euler-Heisenberg four-photon self-interaction, which has the coupling . We study the resonant conversion of relativistic axion dark radiation into photons via the Euler-Heisenberg assisted resonance, and we calculate the expected electromagnetic radiation assuming different values for the axion-photon coupling and different amplitudes for the axion flux onto the neutron star . We briefly discuss several possible sources of axion dark radiation. Achieving a sufficiently strong axion flux to induce a detectable electromagnetic signal seems unlikely. Published by the American Physical Society2024
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- Award ID(s):
- 2114024
- PAR ID:
- 10562237
- Publisher / Repository:
- Physical Review D
- Date Published:
- Journal Name:
- Physical Review D
- Volume:
- 110
- Issue:
- 10
- ISSN:
- 2470-0010
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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