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Inflaton information


The inflaton field is a hypothetical scalar field which is conjectured to have driven cosmic inflation in the very early universe.[1][2][3] The field, originally postulated by Alan Guth,[1] provides a mechanism by which a period of rapid expansion from 10−35 to 10−34 seconds after the initial expansion can be generated, forming a universe consistent with observed spatial isotropy and homogeneity.

  1. ^ a b Guth, Alan H. (1997). The Inflationary Universe: The Quest for a New Theory of Cosmic Origins. Basic Books. pp. 233–234. ISBN 978-0201328400.
  2. ^ Steinhardt, Paul J.; Turok, Neil (2007). Endless Universe: Beyond the Bang. Random House. p. 114. ISBN 978-0-7679-1501-4.
  3. ^ Steinhardt, Paul J. (April 2011). "Inflation Debate: Is the theory at the heart of modern cosmology deeply flawed?" (PDF). Scientific American. Archived from the original (PDF) on 2014-08-24. Retrieved 2013-12-31.

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Inflaton

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The inflaton field is a hypothetical scalar field which is conjectured to have driven cosmic inflation in the very early universe. The field, originally...

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Eternal inflation

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where quantum fluctuation pushed the inflaton value up more than the slow inflation decay rate brought the inflaton value down. Originally there was one...

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Higgs boson

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other hypothetical scalar fields suggested by other theories, from the inflaton to quintessence, could perhaps exist as well. There has been considerable...

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Inflationary epoch

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inflationary epoch. Most inflationary models propose a scalar field called the inflaton field, with properties necessary for having (at least) two vacuum states...

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De Sitter universe

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constant, thought to correspond to dark energy in our universe or the inflaton field in the early universe. According to the models of inflation and current...

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Electroweak epoch

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approximately 10−32 seconds after the Big Bang when the potential energy of the inflaton field that had driven the inflation of the universe during the inflationary...

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Curvaton

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instead it generates curvature perturbations at late times after the inflaton field has decayed and the decay products have redshifted away, when the...

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Tachyonic field

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Ginzburg–Landau and BCS theories of superconductivity. Other examples include the inflaton field in certain models of cosmic inflation (such as new inflation), and...

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Molecule

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Superpartners Others Axion Curvaton Dilaton Dual graviton Graviphoton Graviton Inflaton Leptoquark Magnetic monopole Majoron Majorana fermion Dark photon Preon...

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Electron

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Superpartners Others Axion Curvaton Dilaton Dual graviton Graviphoton Graviton Inflaton Leptoquark Magnetic monopole Majoron Majorana fermion Dark photon Preon...

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Fermion

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Superpartners Others Axion Curvaton Dilaton Dual graviton Graviphoton Graviton Inflaton Leptoquark Magnetic monopole Majoron Majorana fermion Dark photon Preon...

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Gravitational wave background

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"preheating" mechanisms after inflation involving energy transfer from inflaton particles to regular matter, cosmological phase transitions in the early...

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Elementary particle

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Superpartners Others Axion Curvaton Dilaton Dual graviton Graviphoton Graviton Inflaton Leptoquark Magnetic monopole Majoron Majorana fermion Dark photon Preon...

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Photon

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Superpartners Others Axion Curvaton Dilaton Dual graviton Graviphoton Graviton Inflaton Leptoquark Magnetic monopole Majoron Majorana fermion Dark photon Preon...

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Neutrino

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Superpartners Others Axion Curvaton Dilaton Dual graviton Graviphoton Graviton Inflaton Leptoquark Magnetic monopole Majoron Majorana fermion Dark photon Preon...

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Atom

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Superpartners Others Axion Curvaton Dilaton Dual graviton Graviphoton Graviton Inflaton Leptoquark Magnetic monopole Majoron Majorana fermion Dark photon Preon...

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Boson

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Superpartners Others Axion Curvaton Dilaton Dual graviton Graviphoton Graviton Inflaton Leptoquark Magnetic monopole Majoron Majorana fermion Dark photon Preon...

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Big Bang

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having increased by a factor of at least 1078. Reheating followed as the inflaton field decayed, until the universe obtained the temperatures required for...

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Massless particle

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Superpartners Others Axion Curvaton Dilaton Dual graviton Graviphoton Graviton Inflaton Leptoquark Magnetic monopole Majoron Majorana fermion Dark photon Preon...

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Positron

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Superpartners Others Axion Curvaton Dilaton Dual graviton Graviphoton Graviton Inflaton Leptoquark Magnetic monopole Majoron Majorana fermion Dark photon Preon...

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Cosmic microwave background

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The remaining irregularities were caused by quantum fluctuations in the inflaton field that caused the inflation event. Long before the formation of stars...

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Matter

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Superpartners Others Axion Curvaton Dilaton Dual graviton Graviphoton Graviton Inflaton Leptoquark Magnetic monopole Majoron Majorana fermion Dark photon Preon...

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Particle physics

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Superpartners Others Axion Curvaton Dilaton Dual graviton Graviphoton Graviton Inflaton Leptoquark Magnetic monopole Majoron Majorana fermion Dark photon Preon...

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Standard Model

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Superpartners Others Axion Curvaton Dilaton Dual graviton Graviphoton Graviton Inflaton Leptoquark Magnetic monopole Majoron Majorana fermion Dark photon Preon...

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General relativity

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potential function that is crucial to determining the dynamics of the inflaton is simply postulated, but not derived from an underlying physical theory...

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Expansion of the universe

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occurred at a time of around 10−32 seconds. It would have been driven by the inflaton, a field that has a positive-energy false vacuum state. Inflation was originally...

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