| Home > Publications database > Resonant backreaction in axion inflation | 
| Journal Article | PUBDB-2020-03826 | 
  ;   ;   ;  
2020
IOP
London
  This record in other databases: 
  
  
    
Please use a persistent id in citations: doi:10.1088/1475-7516/2020/09/009 doi:10.3204/PUBDB-2020-03826
Report No.: DESY-20-017; arXiv:2002.02952
Abstract: Axion inflation entails a coupling of the inflaton field to gauge fields through the Chern-Simons term. This results in a strong gauge field production during inflation, which backreacts on the inflaton equation of motion. Here we show that this strongly non-linear system generically experiences a resonant enhancement of the gauge field production, resulting in oscillatory features in the inflaton velocity as well as in the gauge field spectrum. The gauge fields source a strongly enhanced scalar power spectrum at small scales, exceeding previous estimates. For appropriate parameter choices, the collapse of these over-dense regions can lead to a large population of (light) primordial black fholes with remarkable phenomenological consequences.
Keyword(s): inflaton: field equations ; inflaton: coupling ; black hole: primordial ; power spectrum: scalar ; resonance: enhancement ; gauge field theory ; inflation ; axion ; Chern-Simons term ; back reaction: nonlinear ; gravitation: collapse ; numerical calculations ; cosmological model
        
        
        
        
         
        
 | 
 The record appears in these collections:  | 
Preprint
Resonant backreaction in axion inflation
[10.3204/PUBDB-2020-00857]
 
 
 Files  
Fulltext by arXiv.org
    BibTeX |
    EndNote:
    XML,
    Text |
    RIS