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We place limits on semiclassical fluctuations that might be present in the primordial perturbation spectrum.
Amsterdam ; New York : North-Holland Pub. Co. ; New York, N.Y. : Elsevier Science Pub. Co., 1982
R. Rajaraman, Solitons and Instantons: An Introduction to Solitons and Instantons in Quantum Field Theory · 1982
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Chapman and Hall, 1996
W. R. Gilks, S. Richardson, and D. J. Spiegelhalter, Markov Chain Monte Carlo In Practice · 1996
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A. D. Linde and V. F. Mukhanov, Nongaussian isocurvature perturbations from inflation
1997
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A. Lewis, A. Challinor, and A. Lasenby, Efficient computation of CMB anisotropies in closed FRW models
2000
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U. H. Danielsson, A note on inflation and transplanckian physics
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S. Dodelson, Modern Cosmology · 2003
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R. Easther, W. H. Kinney, and H. Peiris, Boundary effective field theory and trans-Planckian perturbations: Astrophysical implications
2005
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K. Gorski, E. Hivon, A. Banday, B. Wandelt, F. Hansen, et. al
2005
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K. Land and J. Magueijo, The Axis of Evil revisited
2007
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A. Rakic and D. J. Schwarz, Correlating anomalies of the microwave sky: The Good, the Evil and the Axis
2007
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C. Gordon, Broken Isotropy from a Linear Modulation of the Primordial Perturbations
2007
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2011
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2011
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2011
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2012
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2008
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C. Armendariz-Picon, Do Cosmological Perturbations Have Zero Mean?
2011
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D. Baumann, TASI Lectures on Inflation
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The WMAP Science Working Group, 4.1 ed
M. Limon, Wilkinson Microwave Anisotropy Probe (WMAP): Seven–Year Explanatory Supplement
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