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Cosmic Microwave Background Polarization

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Kosowsky, Arthur·1996·Annals of Physics

Abstract

Abstract Polarization of the cosmic microwave background, though not yet detected, provides a source of information about cosmological parameters complementary to temperature fluctuations. This paper provides a complete theoretical treatment of polarization fluctuations. After a discussion of the physics of polarization, the Boltzmann equation governing the evolution of the photon density matrix is derived from quantum theory and applied to microwave background fluctuations, resulting in a complete set of transport equations for the Stokes parameters from both scalar and tensor metric perturbations. This approach is equivalent at lowest order in scattering kinematics to classical radiative transfer, and provides a general framework for treating the cosmological evolution of density matrices. The metric perturbations are treated in the physically appealing longitudinal gauge. Expressions for various temperature and polarization correlation functions are derived. Detection prospects and theoretical utility of microwave background polarization are briefly discussed.

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Metadata

Authors
Kosowsky, A.
Venue
Annals of Physics
Publisher
Elsevier BV
Published
1996-02
Volume
246
Issue
1
Pages
49-85
ISSN
0003-4916 (ISSN-L)
OpenAlex
W2046002164
Cited by
237
References
0
FWCI
9.07
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Cosmic Microwave Background Polarization. https://app.cochat.ai/papers/10.1006/aphy.1996.0020
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Kosowsky, A. (1996). Cosmic Microwave Background Polarization. Annals of Physics. https://doi.org/10.1006/aphy.1996.0020

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.