Recycling the universe using scalar fields
arXiv:astro-ph/0101448 · doi:10.1103/PhysRevD.63.083520
Abstract
We examine the behaviour of a closed oscillating universe filled with a homogeneous scalar field and find that, contrary to naive expectations, such a universe expands to larger volumes during successive expansion epochs. This intriguing behaviour introduces an arrow of time in a system which is time-reversible. The increase in the maximum size of the universe is closely related to the work done on/by the scalar field during one complete oscillatory cycle which, in turn, is related to the asymmetry in the scalar field equation of state during expansion and collapse. Our analysis shows that scalar fields with polynomial potentials , lead to a growing oscillation amplitude for the universe: the increase in amplitude between successive oscillations is more significant for smaller values of . Such behaviour allows for the effective recycling of the universe. A recycled universe can be quite old and can resolve the flatness problem. These results have strong bearing on cosmological models in which the role of dark matter is played by a scalar field. They are also relevant for chaotic inflationary models of the early universe since they demonstrate that, even if the universe fails to inflate the first time around, it will eventually do so during future oscillatory cycles. Thus, the space of initial conditions favourable for chaotic inflation increases significantly.
9 pages, 7 figures, accepted for publication in Phys. Rev. D
Cited by in corpus (47)
- The Emergent Universe: inflationary cosmology with no singularity
- Tachyons, Scalar Fields and Cosmology
- Bouncing Braneworlds
- Suppressing CMB Quadrupole with a Bounce from Contracting Phase to Inflation
- Spinors, Inflation, and Non-Singular Cyclic Cosmologies
- Non-singular cosmology in a model of non-relativistic gravity
- Big Crunch Avoidance in k = 1 Semi-Classical Loop Quantum Cosmology
- Obtaining the CMB anomalies with a bounce from the contracting phase to inflation
- Oscillatory Universes in Loop Quantum Cosmology and Initial Conditions for Inflation
- Parametric amplification of metric fluctuations through a bouncing phase
- Oscillating universe with quintom matter
- Can Universe Experience Many Cycles with Different Vacua ?
- A classical bounce: constraints and consequences
- Inflation with a Negative Cosmological Constant
- Tachyonic Quintessential Inflation
- Proliferation in Cycle
- Patch dualities and remarks on nonstandard cosmologies
- Inflation in Oscillating Universe
- Cosmological Hysteresis and the Cyclic Universe
- Inflationary Cosmology and Oscillating Universes in Loop Quantum Cosmology
- Cyclic Inflation
- Design of a Cyclic Multiverse
- Amplification of Curvature Perturbations in Cyclic Cosmology
- Equation-of-state formalism for dark energy models on the brane and the future of brane universes
- Dynamics and chaos in the unified scalar field Cosmology
- Quantum gravitational onset of Starobinsky inflation in a closed universe
- Scalar Perturbations Through Cycles
- Chaplygin inflation in loop quantum cosmology
- Hysteresis and beats in loop quantum cosmology
- Topological Defects in Contracting Universes
- Arrow of time in dissipationless cosmology
- Hysteresis in the Sky
- Effective Field Theory of Dark Matter from membrane inflationary paradigm
- Topological defects: A problem for cyclic universes?
- Flat cosmological models with massive scalar field in gauge theories of gravity
- Brane cosmology from observational surveys and its comparison with standard FRW cosmology
- Emergent universe revisited through the CSL theory
- Emergent universe: tensor perturbations within the CSL framework
- The matter-energy intensity distribution in a quantum gravitational system
- Consistency of Anisotropic Inflation during Rapid Oscillations with Planck 2015 Data
- New exact cosmologies on the brane
- Isotropization in Chaplygin matter universes connected by a wormhole
- A novel model of non-singular oscillating cosmology on flat Randall-Sundrum II braneworld
- A dark radiation era prior to the inflationary phase
- AdS cycles in eternally inflating background
- Traversable Lorentzian wormhole on the Shtanov-Sahni braneworld with matter obeying the energy conditions
- A note on the arrow of time in nonminimally coupled scalar field FRW cosmology