Cosmic topology. Part IIIa. Microwave background parity violation without parity-violating microphysics
arXiv:2407.09400 · doi:10.1088/1475-7516/2024/11/020
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- and odd- angular power spectrum , while recent analyses of CMB polarization have revealed non-zero equal- 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 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.
20 pages, 4 figures. v2: version published in JCAP
References in corpus (24)
- Chiral Primordial Gravitational Waves from a Lifshitz Point
- New Extraction of the Cosmic Birefringence from the Planck 2018 Polarization Data
- Relativistic cosmology and large-scale structure
- Predictions from an anisotropic inflationary era
- New physics from the polarised light of the cosmic microwave background
- Cosmic Birefringence from Planck Data Release 4
- Improved Constraints on Cosmic Birefringence from the WMAP and Planck Cosmic Microwave Background Polarization Data
- Analyzing the Large-Scale Bulk Flow using CosmicFlows4: Increasing Tension with the Standard Cosmological Model
- Frequency-Dependent Constraints on Cosmic Birefringence from the LFI and HFI Planck Data Release 4
- Extending the WMAP Bound on the Size of the Universe
- Power spectrum of domain-wall network and its implications for isotropic and anisotropic cosmic birefringence
- The kinematic dipole in galaxy redshift surveys
- Inflationary power asymmetry from primordial domain walls
- Theoretical systematics in testing the Cosmological Principle with the kinematic quasar dipole
- Statistical Anisotropies in Gravitational Waves in Solid Inflation
- Promise of Future Searches for Cosmic Topology
- Chirality oscillation of primordial gravitational waves during inflation
- The expected kinematic matter dipole is robust against source evolution
- Can primordial parity violation explain the observed cosmic birefringence?
- Cosmic topology. Part I. Limits on orientable Euclidean manifolds from circle searches
- On the detectability of non-trivial topologies
- Cosmic topology. Part IIa. Eigenmodes, correlation matrices, and detectability of orientable Euclidean manifolds
- Exact CMB B-mode power spectrum from anisotropic cosmic birefringence
- Cosmic topology. Part IVa. Classification of manifolds using machine learning: a case study with small toroidal universes
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