Cornering Extended Starobinsky Inflation with CMB and SKA
arXiv:2210.05698 · doi:10.21468/SciPostPhys.15.2.047
Abstract
Starobinsky inflation is an attractive, fundamental model to explain the Planck measurements, and its higher-order extension may allow us to probe quantum gravity effects. We show that future CMB data combined with the 21cm intensity map from SKA will meaningfully probe such an extended Starobinsky model. A combined analysis will provide a precise measurement and intriguing insight into inflationary dynamics, even accounting for correlations with astrophysical parameters.
arXiv commentMatches with published version
References in corpus (65)
- Planck 2018 results. X. Constraints on inflation
- The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- Revising the Halofit Model for the Nonlinear Matter Power Spectrum
- Planck 2013 results. XXII. Constraints on inflation
- Inflation Dynamics and Reheating
- 21-cm cosmology
- Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code
- 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal
- Cosmological perturbations
- Reionization of the Inhomogeneous Universe
- CMB Lensing Reconstruction on the Full Sky
- Reionization and Cosmology with 21 cm Fluctuations
- Fingers of God
- Cosmological Parameter Estimation Using 21 cm Radiation from the Epoch of Reionization
- CMB-S4 Science Case, Reference Design, and Project Plan
- Mission design of LiteBIRD
- Fundamental Physics with the Square Kilometre Array
- Inflationary cosmology in modified gravity theories
- Reionization and the Cosmic Dawn with the Square Kilometre Array
- Late-time cosmology with 21cm intensity mapping experiments
- Cosmology with Phase 1 of the Square Kilometre Array; Red Book 2018: Technical specifications and performance forecasts
- 21 cm fluctuations from inhomogeneous X-ray heating before reionization
- CMB-S4: Forecasting Constraints on Primordial Gravitational Waves
- Gravitational lensing as a contaminant of the gravity wave signal in CMB
- A Method for Separating the Physics from the Astrophysics of High-Redshift 21cm Fluctuations
- Statistical Probes of Reionization With 21 cm Tomography
- The X-ray spectra of the first galaxies: 21cm signatures
- The Fast Fourier Transform Telescope
- A polynomial f(R) inflation model
- 21cmFAST v3: A Python-integrated C code forgenerating 3D realizations of the cosmic 21cm signal
- Characteristic Scales During Reionization
- The Epoch of Reionization
- The promising future of a robust cosmological neutrino mass measurement
- Cosmic Reionization Redux
- Cosmology in the era of Euclid and the Square Kilometre Array
- The effect of Limber and flat-sky approximations on galaxy weak lensing
- Constraining the astrophysics and cosmology from 21cm tomography using deep learning with the SKA
- Computer Simulations of Cosmic Reionization
- Consistency relation for inflation
- Analytic extensions of Starobinsky model of inflation
- Bouncing inflation in nonlinear gravitational model
- Beyond the Starobinsky model for inflation
- The Cosmic Linear Anisotropy Solving System (CLASS) III: Comparision with CAMB for LambdaCDM
- The impact of spin temperature fluctuations on the 21-cm moments
- Reconstructing a theory from the -Attractors
- What do WMAP and SDSS really tell about inflation?
- Removing Astrophysics in 21 cm maps with Neural Networks
- Constraints on the neutrino parameters by future cosmological 21cm line and precise CMB polarization observations
- Reinterpretation of the Starobinsky model
- Flat-Sky Pseudo-Cls Analysis for Weak Gravitational Lensing
- Higher-order extension of Starobinsky inflation: initial conditions, slow-roll regime, and reheating phase
- Cosmological parameter measurement and neutral hydrogen 21 cm sky survey with the Square Kilometre Array
- Isocurvature bounds on axion-like particle dark matter in the post-inflationary scenario
- The Structure of Reionization in Hierarchical Galaxy Formation Models
- X-ray background and its correlation with the 21 cm signal
- Generalized non-local -like inflation
- The Dark Ages of the Universe and Hydrogen Reionization
- Tabletop potentials for inflation from gravity
- Modification of the 21-cm power spectrum by X-rays during the epoch of reionisation
- Modification of the 21-cm power spectrum by quasars during the epoch of reionisation
- Snowmass 2021 CMB-S4 White Paper
- The Theory and Simulation of the 21-cm Background from the Epoch of Reionization
- Let there be Light: the Emergence of Structure out of the Dark Ages in the Early Universe
- Detectability of CMB Weak Lensing and HI Cross Correlation and constraints on cosmological parameters
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- The -Higgs inflation: contribution and preheating after ACT and SPT data
- Optimal, fast, and robust inference of reionization-era cosmology with the 21cmPIE-INN
- Stability investigations of isotropic and anisotropic exponential inflation in the Starobinsky-Bel-Robinson gravity
- SKATR: A Self-Supervised Summary Transformer for SKA
- Baryogenesis in -Higgs Inflation: the Gravitational Connection
- Observational Constraints on Extended Starobinsky and Weyl Gravity Model of Inflation
- Stage IV CMB forecasts for warm inflation
- Stability investigations of de Sitter inflationary solutions in power-law extensions of the Starobinsky model
- Inflation in light of ACT/SPT: A new perspective from Weyl gravity
- Echoes of modification and Goldstone preheating in the CMB-BAO landscape