Polarization in the Cosmic Microwave Background

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Autor principal: James G. Bartlett
Formato: Artículo científico
Lenguaje:en
Publicado: Sociedade Brasileira de Física 2006
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author James G. Bartlett
author_facet James G. Bartlett
contents Polarization in the Cosmic Microwave Background James G. Bartlett Física, Astronomía y Matemáticas CMB observations Cosmic microwave background theory Cosmic microwave background (CMB) studies underpin our understanding of the universe and its history.Until recently, we have relied principally on CMB temperature observations to build our standard cosmologicalmodel, but today the field forges ahead into its next frontier – CMB polarization anistropy. Polarization measurementswill furnish fresh and independent information on the primordial density perturbations and cosmologicalparameters, and they offer the exciting potential to detect primordial gravity waves, constrain dark energy andmeasure the neutrino mass scale. I review the science and long–term goals of CMB polarization measurementsand discuss current results and future observational projects. A vigorous program of ground–based, suborbitaland space–based (e.g., WMAP and Planck [2008]) experiments is guiding us towards a future space missiondedicated to high precision polarization measurements. 2006 artículo científico 0103-9733 https://www.redalyc.org/articulo.oa?id=46436604 en http://www.redalyc.org/revista.oa?id=464 Brazilian Journal of Physics application/pdf Sociedade Brasileira de Física Brazilian Journal of Physics (Brasil) Num.4A Vol.36
format Artículo científico
id redalyc_46436604
language en
publishDate 2006
publisher Sociedade Brasileira de Física
spellingShingle Polarization in the Cosmic Microwave Background
James G. Bartlett
Física, Astronomía y Matemáticas
CMB observations
Cosmic microwave background theory
Polarization in the Cosmic Microwave Background James G. Bartlett Física, Astronomía y Matemáticas CMB observations Cosmic microwave background theory Cosmic microwave background (CMB) studies underpin our understanding of the universe and its history.Until recently, we have relied principally on CMB temperature observations to build our standard cosmologicalmodel, but today the field forges ahead into its next frontier – CMB polarization anistropy. Polarization measurementswill furnish fresh and independent information on the primordial density perturbations and cosmologicalparameters, and they offer the exciting potential to detect primordial gravity waves, constrain dark energy andmeasure the neutrino mass scale. I review the science and long–term goals of CMB polarization measurementsand discuss current results and future observational projects. A vigorous program of ground–based, suborbitaland space–based (e.g., WMAP and Planck [2008]) experiments is guiding us towards a future space missiondedicated to high precision polarization measurements. 2006 artículo científico 0103-9733 https://www.redalyc.org/articulo.oa?id=46436604 en http://www.redalyc.org/revista.oa?id=464 Brazilian Journal of Physics application/pdf Sociedade Brasileira de Física Brazilian Journal of Physics (Brasil) Num.4A Vol.36
title Polarization in the Cosmic Microwave Background
topic Física, Astronomía y Matemáticas
CMB observations
Cosmic microwave background theory
url https://www.redalyc.org/articulo.oa?id=46436604