Effects of Variable Newton Constant During Inflation
arXiv:1206.0903 · doi:10.1103/PhysRevD.86.043522
Abstract
In this paper the effects of time-dependent Newton constant G during inflation are studied. We present the formalism of curvature perturbations in an inflationary system with a time-dependent Newton constant. As an example we consider a toy model in which G undergoes a sudden change during inflation. By imposing the appropriate matching conditions the imprints of this sharp change in G on curvature perturbation power spectrum are studied. We show that if G increases (decreases) during the transition the amplitude of curvature perturbations on large scales decreases (increases). In our model with a sudden change in G a continuous sinusoidal modulations on curvature power spectrum is induced. However, in a realistic scenario in which the change in G has some finite time scale we expect these sinusoidal modulations to be damped on short scales. The generated features may be used to explain the observed glitches on CMB power spectrum. This puts a bound on during inflation of roughly the same order as current bounds on during the entire observed age of the universe.
15 pages, 2 figures. Typos fixed, new references added, conforms with the journal version
References in corpus (30)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Monodromy in the CMB: Gravity Waves and String Inflation
- A Parameterized Post-Friedmann Framework for Modified Gravity
- Generation and Characterization of Large Non-Gaussianities in Single Field Inflation
- Superconformal Symmetry, NMSSM, and Inflation
- Observational Tests of Modified Gravity
- New models of chaotic inflation in supergravity
- Holographic dark energy with varying gravitational constant
- Non-Gaussianity from Step Features in the Inflationary Potential
- New Universal Local Feature in the Inflationary Perturbation Spectrum
- Hybrid inflation along waterfall trajectories
- Effects of particle production during inflation
- On Features and Nongaussianity from Inflationary Particle Production
- Formation of primordial black holes from non-Gaussian perturbations produced in a waterfall transition
- Is a step in the primordial spectral index favored by CMB data ?
- The hybrid inflation waterfall and the primordial curvature perturbation
- Curvature perturbation in multi-field inflation with non-minimal coupling
- Nongaussianity from Particle Production During Inflation
- Rapid roll Inflation with Conformal Coupling
- Stochastic Effects in Hybrid Inflation
- The Importance of Slow-roll Corrections During Multi-field Inflation
- The Conformal Transformation in General Single Field Inflation with Non-Minimal Coupling
- Strong scale dependent bispectrum in the Starobinsky model of inflation
- Wiggles in the cosmic microwave background radiation: echoes from non-singular cyclic-inflation
- Waterfall field in hybrid inflation and curvature perturbation
- No Large Scale Curvature Perturbations during Waterfall of Hybrid Inflation
- Local Features with Large Spiky non-Gaussianities during Inflation
- Fields Annihilation and Particles Creation in DBI inflation
- Short Distance Physics and Initial State Effects on the CMB Power Spectrum
- Non-minimally coupled hybrid inflation