A geometric description of the non-Gaussianity generated at the end of multi-field inflation

Journal of Cosmology and Astroparticle Physics

Volumn 2009, Issue 6, 2009, Pages

  Huang, Qing Guo ^a,b  

^a Korea Institute for Advanced Study   (South Korea)

^b INSTITUTE OF THEORETICAL PHYSICS   (China)

Author keywords

Cosmological perturbation theory; Inflation; Non gaussianity

Indexed keywords

EID: 70350673982     PISSN: 14757516     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2009/06/035     Document Type: Article

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