CMB spectral distortions as solutions to the Boltzmann equations

DOI10.1088/1475-7516/2017/01/037OpenAlexW3106443533MaRDI QIDQ5024096

Atsuhisa Ota

Publication date: 28 January 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1611.08058

zbMATH Keywords

non-GaussianitySunyaev-Zeldovich effectCMBR theory

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (4)

Unified approach to secondary effects on the CMB B-mode polarization ⋮ Secondary isocurvature perturbations from acoustic reheating ⋮ Exploring compensated isocurvature perturbations with CMB spectral distortion anisotropies ⋮ Spectral distortion anisotropies from single-field inflation

Cites Work

• The radiative transfer for polarized radiation at second order in cosmological perturbations
• Parameterization of temperature and spectral distortions in future CMB experiments
• Second-order Boltzmann equation: gauge dependence and gauge invariance
• Gauge-invariant Boltzmann equation and the fluid limit

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