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
Hauptverfasser: 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
Format: Artikel
Sprache:eng
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Zusammenfassung: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.
ISSN:0094-243X
DOI:10.1063/1.3160886