Tilted non-spatially-flat inflation
arXiv:2211.02999 · doi:10.1103/PhysRevD.106.123524
Abstract
We construct non-linear inflaton potential energy densities that describe not-necessarily very-slowly-rolling closed and open inflation models, and compute tilted primordial spatial inhomogeneity power spectra that follow from quantum mechanical fluctuations during inflation in these models. Earlier non-flat inflation model power spectra computations assumed an inflaton potential energy density with a linear slope that resulted in very-slow-roll during inflation and untilted power spectra. These new tilted power spectra differ from those that have previously been used to study cosmological data in non-flat cosmological models.
14 pages. PRD accepted version, minor changes
References in corpus (38)
- Measurements of the Hubble Constant: Tensions in Perspective
- Hubble parameter measurement constraints on the redshift of the deceleration-acceleration transition, dynamical dark energy, and space curvature
- Eppur è piatto? The cosmic chronometer take on spatial curvature and cosmic concordance
- Measuring the Hubble constant with Type Ia supernovae as near-infrared standard candles
- A blinded determination of from low-redshift Type Ia supernovae, calibrated by Cepheid variables
- Ultra-compact structure in intermediate-luminosity radio quasars: building a sample of standard cosmological rulers and improving the dark energy constraints up to
- Using Pantheon and DES supernova, baryon acoustic oscillation, and Hubble parameter data to constrain the Hubble constant, dark energy dynamics, and spatial curvature
- The relation for massive bursts of star formation
- An independent determination of the local Hubble constant
- Determining the range of validity of quasar X-ray and UV flux measurements for constraining cosmological model parameters
- Standardizing Platinum Dainotti-correlated gamma-ray bursts, and using them with standardized Amati-correlated gamma-ray bursts to constrain cosmological model parameters
- Recombination-independent determination of the sound horizon and the Hubble constant from BAO
- Constraining cosmic curvature by using age of galaxies and gravitational lenses
- Quasar standardization: Overcoming Selection Biases and Redshift Evolution
- Spectral analysis of Fermi-LAT gamma-ray bursts with known redshift and their potential use as cosmological standard candles
- Full-Shape Galaxy Power Spectra and the Curvature Tension
- Measuring cosmological parameters with a luminosity-time correlation of gamma-ray bursts
- Independent Cosmological Constraints from high-z HII Galaxies
- Cosmological constraints from HII starburst galaxy apparent magnitude and other cosmological measurements
- Implication of Dark Energy Parametrizations on the Determination of the Curvature of the Universe
- Inflation in a closed universe
- The resilience of the Etherington-Hubble relation
- Gamma-ray burst data strongly favor the three-parameter fundamental plane (Dainotti) correlation relation over the two-parameter one
- Generalized tracker quintessence models for dark energy
- Gamma ray burst constraints on cosmological models from the improved Amati correlation
- - correlation of gamma ray bursts: calibration and cosmological applications
- Constraining the curvature density parameter in cosmology
- Standardizing reverberation-measured C IV time-lag quasars, and using them with standardized Mg II quasars to constrain cosmological parameters
- The improved Amati correlations from Gaussian copula
- Exploring the Hubble Tension and Spatial Curvature from the Ages of Old Astrophysical Objects
- Consistency study of high- and low-accreting Mg ii quasars: No significant effect of the Fe ii to Mg ii flux ratio on the radius-luminosity relation dispersion
- Can the Distance-Redshift Relation Be Determined from Correlations Between Luminosities?
- Cosmological Constraints on Non-flat Exponential Gravity
- Multiple measurements of quasars acting as standard probes: model independent calibration and exploring the Dark Energy Equation of States
- A 4% measurement of using the cumulative distribution of strong-lensing time delays in doubly-imaged quasars
- Imprint of spatial curvature on inflation power spectrum
- The Hubble constant and dark energy from cosmological distance measures
- Standardizing reverberation-measured Mg II time-lag quasars, by using the radius-luminosity relation, and constraining cosmological model parameters