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The simplest single-field inflation models capture all the relevant contributions to the patterns in the Cosmic Microwave Background (CMB) observed today.
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A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems
Andrei D. Linde · 1982
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Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking
Andreas Albrecht and Paul J. Steinhardt · 1982
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Spontaneous Creation of Almost Scale - Free Density Perturbations in an Inflationary Universe
James M. Bardeen, Paul J. Steinhardt, and Michael S. Turner · 1983
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Bruce Allen · 1985
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Alan H. Guth · 1987
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Nonequilibrium evolution of scalar fields in FRW cosmologies I
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Cosmic microwave background anisotropies
Wayne Hu and Scott Dodelson · 2002
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Reconstructing the primordial power spectrum
Sarah L Bridle, AM Lewis, J Weller, and G Efstathiou · 2003
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An Effective theory of initial conditions in inflation
Hael Collins and R. Holman · 2005
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Primordial power spectrum reconstruction
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The Renormalization of the energy-momentum tensor for an effective initial state
Hael Collins and R. Holman · 2006
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The Dynamics of general relativity
Richard L. Arnowitt, Stanley Deser, and Charles W. Misner · 2008
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Multimodal nested sampling: an efficient and robust alternative to Markov Chain Monte Carlo methods for astronomical data analyses
F. Feroz and M. P. Hobson · 2008
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Flat tree-level inflationary potentials in the light of cosmic microwave background and large scale structure data
Guillermo Ballesteros, JA Casas, JR Espinosa, R Ruiz de Austri, and R Trotta · 2008
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Bayes in the sky: Bayesian inference and model selection in cosmology
Roberto Trotta · 2008
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MultiNest: an efficient and robust Bayesian inference tool for cosmology and particle physics
F. Feroz, M. P. Hobson, and M. Bridges · 2009
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Features of heavy physics in the CMB power spectrum
Modifications to Cosmological Power Spectra from Scalar-Tensor Entanglement and their Observational Consequences
Nadia Bolis, Andreas Albrecht, and Rich Holman · 2017
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Planck intermediate results-li. features in the cosmic microwave background temperature power spectrum and shifts in cosmological parameters
Nabila Aghanim, Yashar Akrami, Mark Ashdown, J Aumont, C Baccigalupi, M Ballardini, AJ Banday, R Belén Barreiro, Nicola Bartolo, S Basak, et al · 2017
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Objective bayesian analysis of neutrino masses and hierarchy
Alan F Heavens and Elena Sellentin · 2018
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Non-Gaussianity from Entanglement During Inflation
Nadia Bolis, Andreas Albrecht, and R. Holman · 2019
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MontePython 3: boosted MCMC sampler and other features
Thejs Brinckmann and Julien Lesgourgues · 2019
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Ana Achucarro, Jinn-Ouk Gong, Sjoerd Hardeman, Gonzalo A. Palma, and Subodh P. Patil · 2011
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The Physics of Inflation
Daniel Baumann · 2011
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The Cosmic Linear Anisotropy Solving System (CLASS). Part II: Approximation schemes
Diego Blas, Julien Lesgourgues, and Thomas Tram · 2011
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Challenges of profile likelihood evaluation in multi-dimensional susy scans
Farhan Feroz, Kyle Cranmer, Mike Hobson, Roberto Ruiz de Austri, and Roberto Trotta · 2011
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Are priors responsible for cosmology favoring additional neutrino species?
Alma X. Gonzalez-Morales, Robert Poltis, Blake D. Sherwin, and Licia Verde · 2011
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On the importance of heavy fields during inflation
Sebastian Cespedes, Vicente Atal, and Gonzalo A. Palma · 2012
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MathGR: a tensor and GR computation package to keep it simple
Yi Wang · 2013
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Importance nested sampling and the MultiNest algorithm
Farhan Feroz, Michael P. Hobson, Ewan Cameron, and Anthony N. Pettitt · 2019
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On the prior dependence of cosmological constraints on some dark matter interactions
James A. D. Diacoumis and Yvonne Y. Y. Wong · 2019
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Generating primordial features at large scales in two field models of inflation
Matteo Braglia, Dhiraj Kumar Hazra, L. Sriramkumar, and Fabio Finelli · 2020
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Planck 2018 results-x. constraints on inflation
Yashar Akrami, Frederico Arroja, M Ashdown, J Aumont, Carlo Baccigalupi, M Ballardini, Anthony J Banday, RB Barreiro, N Bartolo, S Basak, et al · 2020
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Planck 2018 results
N. Aghanim, Y. Akrami, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, A. J. Banday, R. B. Barreiro, N. Bartolo, and et al · 2020
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Does Planck actually “see” the Bunch-Davies state?
Rose Baunach, Nadia Bolis, R. Holman, Stacie Moltner, and Benoit J. Richard · 2021
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Comparing multi-field primordial feature models with the planck data
Matteo Braglia, Xingang Chen, and Dhiraj Kumar Hazra · 2021
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Early dark energy is not excluded by current large-scale structure data
Tristan L Smith, Vivian Poulin, José Luis Bernal, Kimberly K Boddy, Marc Kamionkowski, and Riccardo Murgia · 2021
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Four-mode squeezed states: two-field quantum systems and the symplectic group Sp ( 4 , ℝ ) \mathrm{Sp}(4,{\mathbb{R}})
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One spectrum to cure them all: signature from early Universe solves major anomalies and tensions in cosmology
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