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Search for Higgs shifts in white dwarfs

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arxiv 1409.8546 v1 pith:BBKVSTIW submitted 2014-09-30 hep-ph astro-ph.IMgr-qc

classification hep-phastro-ph.IMgr-qc
keywords shiftsastrophysicalcouplingcurvaturedifferentialdwarfshiggssearch
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We report on a search for differential shifts between electronic and vibronic transitions in carbon-rich white dwarfs BPM 27606 and Procyon B. The absence of differential shifts within the spectral resolution and taking into account systematic effects such as space motion and pressure shifts allows us to set the first upper bound of astrophysical origin on the coupling between the Higgs field and the Kreschmann curvature invariant. Our analysis provides the basis for a more general methodology to derive bounds to the coupling of long-range scalar fields to curvature invariants in an astrophysical setting complementary to the ones available from high-energy physics or table-top experiments.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Testing bosonic dark matter through white dwarf mass measurements

    astro-ph.HE 2025-10 conditional novelty 5.0 of 10

    Adding a bosonic dark-matter core to white dwarf models reproduces the observed electromagnetic-vs-redshift mass discrepancies and the data favor a boson mass near 10^-10 eV.

  2. Influence of the Vacuum Polarization Effect on the Motion of Charged Particles in the Magnetic Field around a Schwarzschild Black Hole

    gr-qc 2019-08 reject novelty 5.0 of 10

    If vacuum polarization non-minimally couples magnetic fields to gravity, charged particle trajectories around Schwarzschild black holes can shift from unbound to bound, especially near the horizon.

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