Published August 15, 2008
| Version v1
Journal article
Universal weak lensing distortion of cosmological correlation functions
- 1. Institut d'Astrophysique de Paris, UMR7095 CNRS, Universite Pierre et Marie Curie, 98 bis Boulevard Arago, 75014 Paris (France)
- 2. Kavli Institute for Cosmological Physics, Chicago, Illinois 60637-1433 (United States)
- 3. Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637-1433 (United States)
- 4. Center for Particle Astrophysics, Fermi National Accelerator Laboratory, Batavia, Illinois 60510-0500 (United States)
Description
Gravitational lensing affects observed cosmological correlation functions because observed images do not coincide with true source locations. We treat this universal effect in a general way here, deriving a single formula that can be used to determine to what extent this effect distorts any correlation function. We then apply the general formula to the correlation functions of galaxies, the 21-cm radiation field, and the cosmic microwave background.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.78.043508;
- arXiv
- arXiv:0806.0331v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 78
- Journal Issue
- 4
- Journal Page Range
- p. 043508-043508.12
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41001785
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- CORRELATION FUNCTIONS; COSMOLOGICAL MODELS; GALAXIES; GRAVITATIONAL LENSES; RELICT RADIATION; WAVELENGTHS
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; FUNCTIONS; LENSES; MATHEMATICAL MODELS; MICROWAVE RADIATION; RADIATIONS
Optional Information
- Notes
- (c) 2008 The American Physical Society