Chaplygin inflation in loop quantum cosmology
arXiv:0902.0928 · doi:10.1142/S0217732309030436
Abstract
In this paper we discuss the inflationary universe in the context of a Chaplygin gas equation of state within the framework of the effective theory of loop quantum cosmology. Under the slow-roll approximation, we calculate the primordial perturbations for this model. We give the general expressions of the scalar spectral index, its running, and the tensor-to-scalar ratio, etc. For the chaotic inflation with a quadratic potential, using the WMAP 5-year results, we determine the parameters of the Chaplygin inflation model in loop quantum cosmology. The results are consistent with the WMAP observations.
6 pages, accepted for publication in Mod. Phys. Lett. A
References in corpus (41)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- An alternative to quintessence
- Generalized Chaplygin Gas, Accelerated Expansion and Dark Energy-Matter Unification
- Background Independent Quantum Gravity: A Status Report
- The Ekpyrotic Universe: Colliding Branes and the Origin of the Hot Big Bang
- 4-Year COBE DMR Cosmic Microwave Background Observations: Maps and Basic Results
- Quantum Nature of the Big Bang: Improved dynamics
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Inflation
- Unification of Dark Matter and Dark Energy: the Inhomogeneous Chaplygin Gas
- Quantum Nature of the Big Bang
- Absence of Singularity in Loop Quantum Cosmology
- Quantum Nature of the Big Bang: An Analytical and Numerical Investigation
- A Cyclic Model of the Universe
- Inflationary spacetimes are not past-complete
- Loop Quantum Cosmology
- Generalized Chaplygin gas and CMBR constraints
- Lectures on Loop Quantum Gravity
- Bouncing Braneworlds
- The Revival of the Unified Dark Energy-Dark Matter Model ?
- Non-Singular Bouncing Universes in Loop Quantum Cosmology
- Generalized Chaplygin gas as a unified scenario of dark matter/energy: observational constraints
- Loop cosmological dynamics and dualities with Randall-Sundrum braneworlds
- Constraints on modified Chaplygin gas from recent observations and a comparison of its status with other models
- Generalized Chaplygin gas model: constraints from Hubble parameter versus Redshift Data
- Semi-classical States, Effective Dynamics and Classical Emergence in Loop Quantum Cosmology
- Holographic dark energy in a cyclic universe
- Supernovae constraints on models of dark energy revisited
- Phantom field dynamics in loop quantum cosmology
- Oscillating universe with quintom matter
- Can Universe Experience Many Cycles with Different Vacua ?
- Generalized Chaplygin Gas in a modified gravity approach
- Chaplygin inspired Inflation
- Dynamics of Quintom and Hessence Energies in Loop Quantum Cosmology
- Large-scale inhomogeneities in modified Chaplygin gas cosmologies
- Recycling the universe using scalar fields
- The dynamics of the early universe and the initial conditions for inflation in a model with radiation and a Chaplygin gas
- Tachyon-Chaplygin inflationary universe model
- Can black holes be torn up by phantom dark energy in cyclic cosmology?
- Remarks on the Generalized Chaplygin Gas
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