Extending the FLRW model and applying to the earliest continuum Universe, we show that an exponentially accelerating solution for the Scale Factor approaches a flat Universe for any initial condition, resulting in an equation of state similar to that of Dark Energy. The largest total energy density of the expanding observable Universe is due to the inflation solution of a constant energy density starting with the Planck energy density at the initial Planck time. Assuming that this initial inflation ends in the phase change that results in the constituents attaining the finite mass of the observable Universe, the time of this phase change is determined at about 10-22 secs. At this time the observable Universe is about the size of a nucleon. ...
The standard hot big bang cosmology is unable to naturally explain some important features of our ...
The standard hot big bang cosmology is unable to naturally explain some important features of our ...
International audienceWe propose a model of inflation driven by the relaxation of an initially Planc...
<p>At the beginning Planck space-time, Inflation initiation requires a primordial white-hole that on...
At the beginning Planck space-time, Inflation initiation requires a primordial white-hole that only ...
We evaluate both the spectral energy density and the total energy density for relic gravity waves pr...
We study the energy distribution and equation of state of the universe between the end of inflation ...
The standard model of the Universe has it evolving from a concentrated uniform high energy density t...
AbstractIn a unified picture both inflation and present dynamical dark energy arise from the same sc...
We study the energy distribution and equation of state of the universe between the end of inflation ...
In a spatially-flat Friedmann–Lemaître–Robertson–Walker universe, the incorporation of bulk viscous ...
In a spatially-flat Friedmann–Lemaître–Robertson–Walker universe, the incorporation of bulk viscous ...
© 2018 American Physical Society. We examine the class of initial conditions that give rise to infla...
International audienceThe inflationary paradigm is now part of the standard cosmological model as a ...
We analyse the process of reheating the Universe in the electroweak theory where the Higgs field pla...
The standard hot big bang cosmology is unable to naturally explain some important features of our ...
The standard hot big bang cosmology is unable to naturally explain some important features of our ...
International audienceWe propose a model of inflation driven by the relaxation of an initially Planc...
<p>At the beginning Planck space-time, Inflation initiation requires a primordial white-hole that on...
At the beginning Planck space-time, Inflation initiation requires a primordial white-hole that only ...
We evaluate both the spectral energy density and the total energy density for relic gravity waves pr...
We study the energy distribution and equation of state of the universe between the end of inflation ...
The standard model of the Universe has it evolving from a concentrated uniform high energy density t...
AbstractIn a unified picture both inflation and present dynamical dark energy arise from the same sc...
We study the energy distribution and equation of state of the universe between the end of inflation ...
In a spatially-flat Friedmann–Lemaître–Robertson–Walker universe, the incorporation of bulk viscous ...
In a spatially-flat Friedmann–Lemaître–Robertson–Walker universe, the incorporation of bulk viscous ...
© 2018 American Physical Society. We examine the class of initial conditions that give rise to infla...
International audienceThe inflationary paradigm is now part of the standard cosmological model as a ...
We analyse the process of reheating the Universe in the electroweak theory where the Higgs field pla...
The standard hot big bang cosmology is unable to naturally explain some important features of our ...
The standard hot big bang cosmology is unable to naturally explain some important features of our ...
International audienceWe propose a model of inflation driven by the relaxation of an initially Planc...