|  |
| --- |
| Part of a series on |
| Physical cosmology |
| Gravitational inverse-square law |
| * Big Bang **·** Universe
* Age of the universe
* Chronology of the universe
 |
| Early universe

|  |
| --- |
| * Planck epoch
* Grand unification epoch
* Quark epoch
* Hadron epoch
* Lepton epoch
* Photon epoch
* Big Bang nucleosynthesis
* Inflation
* Dark Ages
 |
| 
Backgrounds |
| * Cosmic background radiation (CBR)
* Gravitational wave background (GWB)
* Cosmic microwave background (CMB) **·** Cosmic neutrino background (CNB)
* Cosmic infrared background (INB)
 |

 |
| Expansion **·** Future
* Hubble's law **·** Redshift
* Expansion of the universe
* Accelerating expansion of the universe
* FLRW metric **·** Friedmann equations
* Inhomogeneous cosmology
* Future of an expanding universe
* Ultimate fate of the universe
* Heat death of the universe
* Big Rip
* Big Crunch
* Big Bounce
 |
| Components **·** Structure

| 
Components |
| --- |
| * Lambda-CDM model
* Baryonic matter
* Energy
* Radiation
* Dark energy
	+ Quintessence
	+ Phantom energy
* Dark matter
	+ Cold dark matter
	+ Warm dark matter
	+ Hot dark matter
* Dark radiation
 |
| 
Structure |
| * Shape of the universe
* Reionization **·** Structure formation
* Galaxy formation
* Large-scale structure
* Large quasar group
* Galaxy filament
* Supercluster
* Galaxy cluster
* Galaxy group
* Local Group
* Void
 |

 |
| Experiments
* BOOMERanG
* Cosmic Background Explorer (COBE)
* Illustris project
* Planck space observatory
* Dark Energy Survey
* Euclid
* Large Synoptic Survey Telescope
* Sloan Digital Sky Survey (SDSS)
* 2dF Galaxy Redshift Survey ("2dF")
* Wilkinson Microwave AnisotropyProbe (WMAP)
 |
| 
* Scientists

* Aaronson
* Alfvén
* Alpher
* Bharadwaj
* Copernicus
* de Sitter
* Dicke
* Ehlers
* Einstein
* Ellis
* Friedman
* Galileo
* Gamow
* Guth
* Hawking
* Hubble
* Lemaître
* Linde
* Mather
* Newton
* Penrose
* Penzias
* Rubin
* Schmidt
* Smoot
* Starobinsky
* Steinhardt
* Suntzeff
* Sunyaev
* Tolman
* Wilson
* Zel'dovich

 |
| Subject history
* Discovery of cosmic microwavebackground radiation
* History of the Big Bang theory
* Religious interpretations ofthe Big Bang theory
* Timeline of cosmological theories
 |
| * v
* t
* e
 |

In physical cosmology, the idea of **inflation** is a proposed theory that would explain many features of the present-day universe, including the existence of large-scale structures such as galaxies. The theory was proposed by Alan Guth in the 1970s.

Basic Idea of Inflation
-----------------------

Based on the Standard Model of Cosmology, the universe has been and is expanding. The classical Big Bang theory assumes that the universe expanded at the same rate throughout universal history. Inflation says that the universe *has not* always expanded at the same rate, and that the universe has experienced many periods of brief but immense expansions in which the size of the universe nearly doubled. These periods, as said, were extremely short, lasting less than a second. After a single period, the expansion slowed down until the next rapid inflation came and, again, massively increased the size of the universe.

Problems Solved by Inflation Theory
-----------------------------------

The main problem solved by inflation is the origin of large-scale structures, such as galaxies. Inflation theory says that in a slow expansion of the universe, quantum fluctuations were only on the tiny distance scales; when the universe experienced a brief period of inflation, however, these quantum fluctuations are "stretched" much larger to cause density fluctuations. The places of higher density later caused matter to clump in those locations and form large-scale objects. 

Another problem is that of temperature uniformity in the universe: why is the temperature so evenly distributed? Inflation says that objects that were previously in close proximity to one another were separated very quickly during a period of inflation, so the temperature balance was still held. In the classical Big Bang theory this was a problem because the uniform expansion would mean that objects would have to travel many times the speed of light to maintain temperature balance. 

Another problem that inflation possibly solves is the problem of magnetic monopoles. Why do we no longer see magnetic monopoles in our universe? Inflation says that the few existing monopoles were so dispersed during periods of inflation that it is virtually impossible to find them now.

Mathematical Formulation
------------------------

Inflation theory uses General relativity to model the inflation mathematically. The metric of inflation theory is

{\displaystyle ds^{2}=-(1-\Lambda r^{2})dt^{2}+{\frac {1}{1-\Lambda r^{2}}}dr^{2}+r^{2}d\Omega ^{2}}

Predictions of Inflation Theory
-------------------------------

### Inflatons

The main prediction of inflation theory is that particles called **inflatons** are created from a scalar field from Quantum field theory. These inflatons would drive the inflation periods of the universe, but they quickly decay so the inflation periods are not very long at all. It was initially thought that the Higgs boson was an inflaton, but that has recently been discredited. 

### Multiverse

Inflation theory also suggests that there might be other universes. People's argument for the idea of multiverse is in a nutshell *"If inflation caused our universe, could it not also cause many other universes as well?"* [*source?*]. This prediction has no empirical basis, but it has been explored in modern physics.