Inflaton

This article is about a particle/quantum field posited in cosmology. For a general rise in the level of prices, see Inflation. For other uses of "inflation", see Inflation (disambiguation).
Not to be confused with Instanton.

The inflaton is a hypothetical scalar field that is supposed to be responsible for cosmic inflation[1] in the very early universe.[2] [3] A quantized particle for this field is expected, similar to other quantum fields, called an inflaton (see Inflation (cosmology)). The field provides a mechanism by which a period of rapid expansion from 1035 to 1034 seconds after the initial expansion can be generated, forming the universe.

The basic process of inflation consists of three steps:

  1. Prior to the expansion period, the inflaton field was at a higher-energy state.
  2. Random quantum fluctuations triggered a phase transition whereby the inflaton field released its potential energy as matter and radiation as it settled to its lowest-energy state.
  3. This action generated a repulsive force that drove the portion of the universe that is observable to us today to expand from approximately 1050 metres in radius at 1035 seconds to almost 1 metre in radius at 1034 seconds.

The inflaton field's lowest energy state may or may not be a zero energy state. This depends on the chosen potential energy density of the field.

The term inflaton was derived from inflation following the typical naming style of other quantum fields such as photon, gluon, boson and fermion. The term was first used in a paper entitled ‘After Primordial Inflation’ by, D.V. Nanopoulos, K.A. Olive and M. Srednicki.[4]

It is suggested that the Higgs boson might act as the inflaton.[5]

See also

References

This article is issued from Wikipedia - version of the Saturday, March 26, 2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.