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A New Probe of Cosmic Birefringence Using Galaxy Polarization and Shapes

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arxiv 2402.18568 v2 pith:5NOZUTGR submitted 2024-02-28 astro-ph.CO astro-ph.GAhep-ph

classification astro-ph.COastro-ph.GAhep-ph
keywords galaxyanglebirefringencecirccosmicpolarizationpowerrotation
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abstract

We propose a novel statistical method to measure cosmic birefringence and demonstrate its power in probing parity violation due to axions. Exploiting an empirical correlation between the integrated radio polarization direction of a spiral galaxy and its apparent shape, we devise an unbiased minimum-variance estimator for the rotation angle, which should achieve an uncertainty of $5^\circ$--$ 15^\circ$ per galaxy. Large galaxy samples from the forthcoming SKA continuum surveys, together with optical shape catalogs, promise a comparable or even lower noise power spectrum for the rotation angle than in the CMB Stage-IV (CMB-S4) experiment, with different systematics.

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Forward citations

Cited by 5 Pith papers

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

  1. 3-form dark energy and cosmic birefringence

    astro-ph.CO 2026-08 conditional novelty 6.0 of 10

    3-form dark energy can explain cosmic birefringence with a dimension-4 photon coupling, yielding redshift profiles that can mimic or differ from axion dark energy, but the implied photon mass estimate is numerically shaky.

  2. Limits on global cosmic birefringence using radio sources

    astro-ph.CO 2026-07 conditional novelty 6.0 of 10

    X-band radio sources yield μ_β = (0.2 ± 1.0)° for global cosmic birefringence, with stacking to ~0.6° and a forecast that ~10^5 sources could reach ~0.1° to test Planck claims.

  3. Searching for coupled, hyperlight scalars across cosmic history

    hep-ph 2025-02 conditional novelty 6.0 of 10

    Hyperlight quadratically coupled scalars making up a few percent of dark matter are bounded to near- or sub-gravitational couplings to electrons and photons over 10^-31 to 10^-28 eV, with quasar spectra setting the st...

  4. Wading the String Bog: CMB Birefringence in the Swampland

    hep-th 2026-07 conditional novelty 5.0 of 10

    Ultralight-axion explanations of cosmic birefringence sit in tension with Swampland bounds, while thin axionic domain walls predict exactly isotropic birefringence, so anisotropy measurements can discriminate the alte...

  5. Planck PR4 (NPIPE) map-space cosmic birefringence

    astro-ph.CO 2025-02 conditional novelty 4.0 of 10

    A map-space stacking analysis of Planck PR4 maps finds a CMB polarization rotation angle of about 0.46 to 0.48 degrees, dominated by instrument calibration uncertainty and consistent with no parity-violating cosmic bi...

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