Gravitational Lensing
Gravitational lensing of the cosmic microwave background by large-scale structure in the late universe is both a source of cosmological information and a potential contaminant of primordial gravity waves. Because lensing imprints growth of structure in the late universe on the CMB, measurements of C...
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Veröffentlicht in: | CMB polarization workshop : theory and foregrounds : CMBPol mission concept study : Batavia, IL, 23-26 June 2008 IL, 23-26 June 2008, 2009-01, Vol.1141, p.121-178 |
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container_title | CMB polarization workshop : theory and foregrounds : CMBPol mission concept study : Batavia, IL, 23-26 June 2008 |
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creator | Smith, Kendrick M Cooray, Asantha Das, Sudeep Dore, Olivier Hanson, Duncan Hirata, Chris Kaplinghat, Manoj Keating, Brian Loverde, Marilena Miller, Nathan Rocha, Graga Shimon, Meir Zahn, Oliver |
description | Gravitational lensing of the cosmic microwave background by large-scale structure in the late universe is both a source of cosmological information and a potential contaminant of primordial gravity waves. Because lensing imprints growth of structure in the late universe on the CMB, measurements of CMB lensing will constrain parameters to which the CMB would not otherwise be sensitive, such as neutrino mass. |
doi_str_mv | 10.1063/1.3160886 |
format | Article |
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identifier | ISSN: 0094-243X |
ispartof | CMB polarization workshop : theory and foregrounds : CMBPol mission concept study : Batavia, IL, 23-26 June 2008, 2009-01, Vol.1141, p.121-178 |
issn | 0094-243X |
language | eng |
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source | AIP Journals Complete |
title | Gravitational Lensing |
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