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N-flation

Journal of Cosmology and Astroparticle Physics · 2008 · Vol. 2008(08) · pp. 003–003
Savas DimopoulosShamit KachruJohn McGreevyJay G. Wacker

Abstract

The presence of many axion fields in four-dimensional string vacua can lead to a simple, radiatively stable realization of chaotic inflation.

Cosmology and Gravitation TheoriesBlack Holes and Theoretical PhysicsGalaxies: Formation, Evolution, PhenomenaPhysicsAxionInflation (cosmology)Realization (probability)Theoretical physicsEternal inflationString (physics)Simple (philosophy)ChaoticParticle physics
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References
Chiral quarks and the non-relativistic quark model
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Non-gaussian features of primordial fluctuations in single field inflationary models
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