Linde proposed a theory known as chaotic inflation in which he suggested that the conditions for inflation were actually satisfied quite generically.
Inflation will occur in virtually any universe that begins in a chaotic, high energy state that has a scalar field with unbounded potential energy..
In Brief.
Cosmic inflation is so widely accepted that it is often taken as established fact.
The idea is that the geometry and uniformity of the cosmos were established during an intense early growth spurt..
They are the flatness and horizon problems..
Inflation is a general term for models of the very early Universe which involve a short period of extremely rapid (exponential) expansion, blowing the size of what is now the observable Universe up from a region far smaller than a proton to about the size of a grapefruit (or even bigger) in a small fraction of a second .
In physical cosmology, cosmic inflation, cosmological inflation, or just inflation, is a theory of exponential expansion of space in the early universe.
The inflationary epoch is believed to have lasted from 10−36 seconds to between 10−33 and 10−32 seconds after the Big Bang..
According to the theory of inflation, the early Universe expanded exponentially fast for a fraction of a second after the Big Bang.
Cosmologists introduced this idea in 1981 to solve several important problems in cosmology.
One of these problems is the horizon problem..
In physical cosmology, cosmic inflation, cosmological inflation, or just inflation, is a theory of exponential expansion of space in the early universe.
The inflationary epoch is believed to have lasted from 10−36 seconds to between 10−33 and 10−32 seconds after the Big Bang..
At some point the expansion stopped because the energy density dropped and the elementary particles in the table were created out of the available energy.
The inflaton field is a hypothetical scalar field that is theorized to drive cosmic inflation in the very early universe..
In physical cosmology, cosmic inflation, cosmological inflation, or just inflation, is a theory of exponential expansion of space in the early universe
Around 1930, Edwin Hubble discovered that light from remote galaxies was redshifted; the more remote, the more shifted
An expanding universe generally has a cosmological horizon, which, by analogy with the more familiar horizon caused by the curvature of Earth's surface
Inflation resolves several problems in Big Bang cosmology that were discovered in the 1970s
In the early days of General Relativity, Albert Einstein introduced the cosmological constant to allow a static solution
Hypothetical inflationary universe model
Topics referred to by the same term
A theoretical model of cosmic inflation
