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/10.1088/1475-7516/2012/06/005

Additional details

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