The Polarization of the Cosmic Microwave Background

dc.creatorZaldarriaga, Matias
dc.date2003-05-15
dc.date2003-05-15
dc.date.accessioned2026-07-07T02:08:30Z
dc.date.available2026-07-07T02:08:30Z
dc.descriptionWe summarize the physical mechanism by which the Cosmic Microwave Background acquires a small degree of polarization. We discuss the imprint left by gravitational waves and the use of polarization as a test of the inflationary paradigm. We discuss some physical processes that affect the CMB polarization after recombination such as gravitational lensing and the reionization of the universe.
dc.descriptionReview written for the Carnegie Observatories Centenial Symposium II
dc.identifierhttps://arxiv.org/abs/astro-ph/0305272
dc.identifierhttp://arxiv.org/abs/astro-ph/0305272
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6075
dc.subjectAstrophysics
dc.titleThe Polarization of the Cosmic Microwave Background
dc.typetext

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