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We present constraints on canonical single-field inflation derived from WMAP five year, ACBAR, QUAD, BICEP data combined with the halo power spectrum from SDSS LRG7.
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J. Martin and C. Ringeval, Inflation after WMAP3: confronting the slow-roll and exact power spectra with CMB data
2006
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W. Y. Wong, A. Moss and D. Scott, How well do we understand cosmological recombination?
2008
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P. Adshead and R. Easther, Constraining inflation
2008
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R. Easther and H. Peiris, Implications of a running spectral index for slow roll inflation
2006
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G. Ballesteros, J. A. Casas and J. R. Espinosa, Running spectral index as a probe of physics at high scales
2006
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W. H. Kinney, E. W. Kolb, A. Melchiorri and A. Riotto, Inflation model constraints from the Wilkinson microwave anisotropy probe three-year data
2006
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H. Peiris and R. Easther, Recovering the Inflationary Potential and Primordial Power Spectrum With a Slow Roll Prior: Methodology and Application to WMAP 3 Year Data
2006
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H. Peiris and R. Easther, Slow Roll Reconstruction: Constraints on Inflation from the 3 Year WMAP Dataset
2006
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F. Finelli, M. Rianna and N. Mandolesi, Constraints on the Inflationary Expansion from Three Year WMAP, small scale CMB anisotropies and Large Scale Structure Data Sets
2006
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