Correlated Mixture Between Adiabatic and Isocurvature Fluctuations and Recent CMB Observations

Abstract

This work presents a reduced chi^2_nu test to search for non-gaussian signals in the CMBR TT power spectrum of recent CMBR data, WMAP, ACBAR and CBI data sets, assuming a mixed density field including adiabatic and isocurvature fluctuations. We assume a skew positive mixed model with adiabatic inflation perturbations plus additional isocurvature perturbations possibly produced by topological defects. The joint probability distribution used in this context is a weighted combination of Gaussian and non-Gaussian random fields. Results from simulations of CMBR temperature for the mixed field show a distinct signature in CMB power spectrum for very small deviations (~ 0.1%) from a pure Gaussian field, and can be used as a direct test for the nature of primordial fluctuations. A reduced chi^2_nu test applied on the most recent CMBR observations reveals that an isocurvature fluctuations field is not ruled out and indeed permits a very good description for a flat geometry Lambda-CDM universe, chi^2_930 ~ 1.5, rather than the simple inflationary standard model with chi^2_930 ~ 2.3. This result may looks is particular discrepant with the reduced chi^2 of 1.07 obtained with the same model in Spergel et al. (2003) for temperature only, however, our work is restricted to a region of the parameter space that does not include the best fit model for TT only of Spergel et al. (2003).

Accepted for publication in Physical Review D

References in corpus (7)

• Cosmological parameters from SDSS and WMAP
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Inflation
• First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Angular Power Spectrum
• High Resolution Observations of the CMB Power Spectrum with ACBAR
• Non-Gaussianity of the derived maps from the first-year WMAP data
• Properties of groups of galaxies in the vicinity of massive clusters
• Predictions of mixed non-Gaussian cosmological density fields for the cosmic microwave background radiation

Cited by in corpus (4)

• Constraints on primordial isocurvature perturbations and spatial curvature by Bayesian model selection
• Constraints on scalar and tensor perturbations in phenomenological and two-field inflation models: Bayesian evidences for primordial isocurvature and tensor modes
• CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information
• High Order Correction Terms for The Peak-Peak Correlation Function in Nearly-Gaussian Models