If the spatial curvature of the universe at the beginning of inflation is negative, there is an enhancement of the temperature anisotropy of the Cosmic Background Radiation at large angles. On the other hand if at the start of inflation the universe was closed with curvature there will be a suppression of temperature anisotropy at the scale of the present horizon. The observation of a low quadrupole anisotropy by WMAP suggests that the universe was closed with $(\Omega-1)$ of order unity at the time when the perturbation scales of the size of our present horizon were exiting the inflationary horizon
After introducing gauge-invariant cosmological perturbation theory we give an improved set of govern...
The claim of inflationary cosmology to explain certain observable facts, which the Friedmann-Roberst...
We consider an alternative scenario of inflation which can account for a spatially open universe. It...
If the universe had a large curvature before inflation there is a deviation from the scale invariant...
Curvature effects in inflationary Robertson-Walker models, although neg ligible at the present day, ...
Following the recent measurement of the acoustic peak by the BOOMERanG and MAXIMA experiments in the...
It is shown that curvature effects, though completely negligible at the present day, can drastically...
It is shown that curvature effects, though completely negligible at the present day, can drastically...
AbstractWe assay how inflationary models whose properties are dominated by the dynamics of a single ...
In this work the vacuum inflation with a boundary condition specified at a short-distance scale in a...
We present a gauge-invariant formalism to study the evolution of the curvature and entropy perturbat...
Preheating following the inflationary phase in models of open inflation is considered. The most sign...
The cosmic microwave background (CMB) provides a snapshot of the early Universe when matter began to...
Non-flat Friedmann-Lemaitre models solving the horizon problem in which, prior to and during inflati...
We study how the initial inhomogeneities of the spatial curvature affect the onset of inflation in t...
After introducing gauge-invariant cosmological perturbation theory we give an improved set of govern...
The claim of inflationary cosmology to explain certain observable facts, which the Friedmann-Roberst...
We consider an alternative scenario of inflation which can account for a spatially open universe. It...
If the universe had a large curvature before inflation there is a deviation from the scale invariant...
Curvature effects in inflationary Robertson-Walker models, although neg ligible at the present day, ...
Following the recent measurement of the acoustic peak by the BOOMERanG and MAXIMA experiments in the...
It is shown that curvature effects, though completely negligible at the present day, can drastically...
It is shown that curvature effects, though completely negligible at the present day, can drastically...
AbstractWe assay how inflationary models whose properties are dominated by the dynamics of a single ...
In this work the vacuum inflation with a boundary condition specified at a short-distance scale in a...
We present a gauge-invariant formalism to study the evolution of the curvature and entropy perturbat...
Preheating following the inflationary phase in models of open inflation is considered. The most sign...
The cosmic microwave background (CMB) provides a snapshot of the early Universe when matter began to...
Non-flat Friedmann-Lemaitre models solving the horizon problem in which, prior to and during inflati...
We study how the initial inhomogeneities of the spatial curvature affect the onset of inflation in t...
After introducing gauge-invariant cosmological perturbation theory we give an improved set of govern...
The claim of inflationary cosmology to explain certain observable facts, which the Friedmann-Roberst...
We consider an alternative scenario of inflation which can account for a spatially open universe. It...