Published June 1, 2012
| Version v1
Journal article
Direct recovery of fluctuation spectra from tomographic shear spectra
- 1. Department of Physics, Astronomy Unit, Trieste University, Via Tiepolo 11, I 34143 Trieste (Italy)
- 2. Departamento de Fisica, UFES, Avenida Fernando Ferrari 514, Vitória, Espírito Santo (Brazil)
Description
Forthcoming experiments will enable us to determine high precision tomographic shear spectra. Matter density fluctuation spectra, at various z, should then be recovered from them, in order to constrain the model and determine the DE state equation. Available analytical expressions, however, do the opposite, enabling us to derive shear spectra from fluctuation spectra. Here we find the inverse expression, yielding density fluctuation spectra from observational tomographic shear spectra. The procedure involves SVD techniques for matrix inversion. We show in detail how the approach works and provide a few examples
Availability note (English)
Available from http://dx.doi.org/10.1088/1475-7516/2012/06/005Additional details
Identifiers
Publishing Information
- Journal Title
- Journal of Cosmology and Astroparticle Physics
- Journal Volume
- 2012
- Journal Issue
- 06
- Journal Page Range
- p. 005
- ISSN
- 1475-7516
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 45101352
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ASTROPHYSICS; COSMOLOGY; DENSITY; ENERGY SPECTRA; FLUCTUATIONS; SHEAR
- Descriptors DEC
- PHYSICAL PROPERTIES; PHYSICS; SPECTRA; VARIATIONS