N-Flation

Dimopoulos, S. ; /Stanford U., Phys. Dept. ; Kachru, S. ; /Stanford U., Phys. Dept. /SLAC ; McGreevy, J. ; Wacker, J.G. ; /Stanford U., Phys. Dept.

Stanford Linear Accelerator Center

关键词: String Models;    Theory-Hep,Hepth;    72 Physics Of Elementary Particles And Fields;    Four-Dimensional Calculations Theory-Hep,Hepth;    Axions;   

DOI  :  10.2172/878807
RP-ID  :  SLAC-PUB-11016
RP-ID  :  AC02-76SF00515
RP-ID  :  878807

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来源: UNT Digital Library

【 摘 要 】

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