Parametrizing the power spectrum: beyond the truncated Taylor expansion
Open Access
- 1 August 2005
- journal article
- Published by IOP Publishing in Journal of Cosmology and Astroparticle Physics
- Vol. 2005 (8) , 008
- https://doi.org/10.1088/1475-7516/2005/08/008
Abstract
No abstract availableKeywords
All Related Versions
This publication has 17 references indexed in Scilit:
- From the spectrum to inflation: an inverse formula for the general slow-roll spectrumJournal of Cosmology and Astroparticle Physics, 2005
- Second order general slow-roll power spectrumJournal of Cosmology and Astroparticle Physics, 2004
- The Three‐Dimensional Power Spectrum of Galaxies from the Sloan Digital Sky SurveyThe Astrophysical Journal, 2004
- Inflation on moduli space and cosmic perturbationsJournal of High Energy Physics, 2003
- First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: Determination of Cosmological ParametersThe Astrophysical Journal Supplement Series, 2003
- First‐Year Wilkinson Microwave Anisotropy Probe ( WMAP ) Observations: The Angular Power SpectrumThe Astrophysical Journal Supplement Series, 2003
- Successful modular cosmologyJournal of High Energy Physics, 2003
- Cosmological parameters from CMB and other data: A Monte Carlo approachPhysical Review D, 2002
- Efficient cosmological parameter estimation from microwave background anisotropiesPhysical Review D, 2002
- Spectrum of density perturbations produced during inflation to leading order in a general slow-roll approximationPhysical Review D, 2002