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Cosmic topology. Part IIIa. Microwave background parity violation without parity-violating microphysics

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arxiv 2407.09400 v2 pith:UHCYGGTT submitted 2024-07-12 astro-ph.CO gr-qchep-phhep-th

classification astro-ph.COgr-qchep-phhep-th
keywords correlationsparitytopologycosmicisotropyobservationsparity-violatingstandard
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

The standard cosmological model, which assumes statistical isotropy and parity invariance, predicts the absence of correlations between even-parity and odd-parity observables of the cosmic microwave background (CMB). Contrary to these predictions, large-angle CMB temperature anomalies generically involve correlations between even-$\ell$ and odd-$\ell$ angular power spectrum $C_\ell$, while recent analyses of CMB polarization have revealed non-zero equal-$\ell$ $EB$ correlations. These findings challenge the conventional understanding, suggesting deviations from statistical isotropy, violations of parity, or both. Cosmic topology, which involves changing only the boundary conditions of space relative to standard cosmology, offers a compelling framework to potentially account for such parity-violating observations. Topology inherently breaks statistical isotropy, and can also break homogeneity and parity, providing a natural paradigm for explaining observations of parity-breaking observables without the need to add parity violation to the underlying microphysics. Our investigation delves into the harmonic space implications of topology for CMB correlations, using as an illustrative example $EB$ correlations generated by tensor perturbations under both parity-preserving and parity-violating scenarios. Consequently, these findings not only challenge the foundational assumptions of the standard cosmological model but also open new avenues for exploring the topological structure of the Universe through CMB observations.

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Forward citations

Cited by 4 Pith papers

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

  1. Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe

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

    The paper derives an exact transfer kernel from primordial gravitational-wave anisotropy multipoles to CMB B-mode covariance, with explicit selection rules and a shared cross-frequency template for compact cubic topology.

  2. Planck constraints on the scale dependence of isotropic cosmic birefringence

    astro-ph.CO 2025-07 conditional novelty 6.0 of 10

    Planck polarization data favor a constant cosmic birefringence angle (β≈0.3°) across multipoles, with scale dependence consistent with zero at up to 1.8σ.

  3. Illustrating the consequences of a misuse of $\sigma_8$ in cosmology

    astro-ph.CO 2025-01 accept novelty 5.0 of 10

    Cosmologists should compare clustering amplitude with the h-independent statistic sigma_12 instead of sigma_8, because sigma_8's smoothing scale shifts with H0 and artificially worsens the growth tension in high-H0 models.

  4. Probing the Cosmological Principle with weak lensing shear

    astro-ph.CO 2024-11 conditional novelty 4.0 of 10

    A Euclid-like weak lensing survey could detect the E-B shear cross-correlation produced by late-time anisotropic expansion, yielding a new probe of the Cosmological Principle.

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