Inflation with violation of the null energy condition
- 6 October 2005
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review D
- Vol. 72 (8) , 083504
Abstract
Inflation may have been driven by a component which violated the Null-Energy Condition, thereby leading to super inflation. We provide the formalism to study cosmological perturbations when such a component is described by a scalar field with arbitrary Lagrangian. Since the background curvature grows with time, gravitational waves always have a blue spectrum. We apply our formalism to the case of phantom inflation with an exponential potential (whose polelike inflationary stage is an attractor for inhomogeneous cosmological models for any value of the potential slope) as an example. We finally compare the predictions of super inflation with those of standard inflation stressing the role of gravitational waves.Keywords
All Related Versions
This publication has 21 references indexed in Scilit:
- Crossing the phantom divide: Dark energy internal degrees of freedomPhysical Review D, 2005
- Can dark energy evolve to the phantom?Physical Review D, 2005
- Second-order corrections to the power spectrum in the slow-roll expansion with a time-dependent sound speedPhysics Letters B, 2004
- New Constraints on ΩM, ΩΛ, andwfrom an Independent Set of 11 High‐Redshift Supernovae Observed with theHubble Space TelescopeThe Astrophysical Journal, 2003
- Perturbations in k-inflationPhysics Letters B, 1999
- Constraints on inflation at the Planck scale from the relic graviton spectrumPhysics Letters B, 1992
- Power-law inflation as an attractor solution for inhomogeneous cosmological modelsClassical and Quantum Gravity, 1990
- Scalar fields in cosmology with an exponential potentialPhysics Letters B, 1987
- Kinematical properties of generalized inflationPhysics Letters B, 1985
- Power-law inflationPhysical Review D, 1985