Astrophysics (Index)About


(cosmic inflation, cosmological inflation)
(theorized rapid expansion of the very early universe)

Inflation is a theorized expansion of the universe by 78 orders-of-magnitude within its first 10-32 seconds of existence. The theory explains both the homogeneity observed in the universe as well as characteristics of its large scale structure. The theorized driver is negative-pressure vacuum energy density. The theory was proposed by physicist Alan Guth in 1980.

One homogeneity-issue addressed is termed the horizon problem: that without some such mechanism, different regions of the early universe would not be casually connected given the speed of light was insufficient to get from some point in the earlier universe to each of the different parts, within the age of the universe (at the time). The smoothness of the cosmic microwave background from every direction must result from some common origin that couldn't exist, given a Big Bang without something like inflation. The rapid inflation carries with it the seeds of later events that happen everywhere uniformly.

Another issue inflation addresses is the flatness problem: the question of why the universe shows so little curvature.

(cosmology,CMB,early universe)
Further reading:

Referenced by pages:
Atacama B-Mode Search (ABS)
alternative cosmologies
baryon acoustic oscillations (BAO)
CMB polarization
cosmological simulation
early universe
false vacuum
initial fluctuations
initial fluctuation spectrum
non-Gaussian (NG)
primordial black hole
primordial gravitational waves
quantum fluctuations