Parity-odd power spectra: concise statistics for cosmological parity violation

ABSTRACT We introduce the parity-odd power (POP) spectra, a novel set of observables for probing parity violation in cosmological N-point statistics. POP spectra are derived from composite fields obtained by applying non-linear transformations, involving also gradients, curls, and filtering functions, to a scalar field. This compresses the parity-odd trispectrum into a power spectrum. These new statistics offer several advantages: they are computationally fast to construct, estimating their covariance is less demanding compared to estimating that of the full parity-odd trispectrum, and they are simple to model theoretically. We measure the POP spectra on simulations of a scalar field with a specific parity-odd trispectrum shape. We compare these measurements to semi-analytic theoretical calculations and find agreement. We also explore extensions and generalizations of these parity-odd observables.

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Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2024-08-08
DOI
https://doi.org/10.1093/mnras/stae1924
Citations
15
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
4.97

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article

Parity-odd power spectra: concise statistics for cosmological parity violation

Jiamin Hou, Eiichiro Komatsu, Angelo Caravano, Zachary Slepian et al.
15 citations
Monthly Notices of the Royal Astronomical Society
Cosmology and Gravitation Theories
4.97
article

Parity-odd power spectra: concise statistics for cosmological parity violation

Jiamin Hou, Eiichiro Komatsu, Angelo Caravano, Zachary Slepian, Drew Jamieson
article en
15 citations

Abstract

ABSTRACT We introduce the parity-odd power (POP) spectra, a novel set of observables for probing parity violation in cosmological N-point statistics. POP spectra are derived from composite fields obtained by applying non-linear transformations, involving also gradients, curls, and filtering functions, to a scalar field. This compresses the parity-odd trispectrum into a power spectrum. These new statistics offer several advantages: they are computationally fast to construct, estimating their covariance is less demanding compared to estimating that of the full parity-odd trispectrum, and they are simple to model theoretically. We measure the POP spectra on simulations of a scalar field with a specific parity-odd trispectrum shape. We compare these measurements to semi-analytic theoretical calculations and find agreement. We also explore extensions and generalizations of these parity-odd observables.

Monthly Notices of the Royal Astronomical SocietyVol. 533(3)
Centre National de la Recherche Scientifique (FR), Kavli Institute for the Physics and Mathematics of the Universe (JP), Institut d'Astrophysique de Paris (FR), University of Florida (US), Sorbonne Université (FR), Max Planck Institute for Extraterrestrial Physics (DE), Max Planck Institute for Astrophysics (DE), The University of Tokyo (JP), Ludwig-Maximilians-Universität München (DE)
European Commission, Deutsche Forschungsgemeinschaft, Ministry of Education, Culture, Sports, Science and Technology, Pasteur Institute of Iran, Max-Planck-Institut für Astrophysik, Horizon 2020 Framework Programme
Peace, Justice and strong institutions
Openalex Percentile: Top 5%
Cosmology and Gravitation Theories
4.97
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