Constraints on the canonical single-field slow-roll inflation model from observations
astro-ph.CO
Submitted: 2025-11-14
Updated: 2026-09-12
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Signatures of Modified Dispersion Relation of Graviton in the Cosmic Microwave Background
- Measuring the spectral running from cosmic microwave background and primordial black holes
- Measuring the tilt of primordial gravitational-wave power spectrum from observations
- Measuring the primordial gravitational waves from cosmic microwave background and stochastic gravitational wave background observations
- Measuring the modified gravitational waves propagation beyond general relativity from CMB observations
- Measuring the primordial curvature perturbations from the scalar induced gravitational waves
- Measuring the scalar induced gravitational waves from observations
- Measuring the speed of scalar induced gravitational waves from observations
- Probing the speed of scalar-induced gravitational waves with pulsar timing arrays
- Planck 2018 results. VI. Cosmological parameters
- BICEP / Keck XIII: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season
- The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
- The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- The (p,q) inflation model
- A more accurate analytic calculation of the spectrum of cosmological perturbations produced during inflation
- Cosmological parameter estimation and the inflationary cosmology
- Slow-roll reconstruction for running spectral index
- Monodromy in the CMB: Gravity Waves and String Inflation
- Gravity Waves and Linear Inflation from Axion Monodromy
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