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Effective Field Theory of
Multi-Field Inflation a la Weinberg


              Nima Khosravi
African Institute for Mathematical Sciences



                                arXiv:1203.2266
map:


    keywords: Effective Field Theory, Inflation
Effective Field Theory


    an effective theory:

                       is true for a certain domain of energy.




    two cases:
        
            as a part of a true theory for whole energy scales
                 
                     using EFT to simplify calculations!
        
            in lack of a complete theory for the energy scales of
               interests
                 
                     using EFT since there is no other choice!
                 
                     constructing EFT, by considering e.g. symmetry
                      properties of the model.
                 
EFT for Multi-Field Inflation


    the most general form of Lagrangian up to the 4th order
      derivatives:
          after simplifications:




                                      before simplifications!
perturbations:


    perturbations in single field model (Weinberg’s paper)
















    -- it is up to 4th order of perturbations automatically.

    -- speed of sound ≠ 1

                                      -- large non-Gaussianity   ?
    -- speed of sound is constrained by validity of EFT!





perturbations:


    multi-field case:
     background terms:





















           perturbations!
perturbations:


    two-field case:
     the most general form of the Lagrangian:




                                     second order perturbations!
…. and cubic and quartic terms!


. . . transition to adiabatic and entropy curvature perturbations!


        
perturbations: adiabatic & entropy modes


    adiabatic mode:         entropy mode:





























                      Gordon et al. arXiv:astro-ph/0009131


perturbations: adiabatic & entropy modes

 
     as an example:
 second order perturbation terms (containing time derivatives) due to correction term:




                      note that just these two combinations appear in this formalism!
shape of non-Gaussianity


     due to previous slide: for example:




    equilateral NG                  local NG
in adiabatic mode                    in entropy mode


--- in this formalism
               the “Cosine” between different kinds of NG is fixed!
amplitude of NG






















-- validity condition of EFT i.e.                  constrains the
amplitude of NG!
-- except if the curvature of classical (background) path be large!
-- or: if by a mechanism (e.g. Vainshtein) one can modify the validity
condition of EFT!
compare with Senatore & Zaldarriaga

-- Senatore & Zaldarriaga model is based on Cheung et al.’s work!
-- in Cheung’s work, EFT is constructed on perturbations’ level!
   -- since their model is single field, the perturbation is
associated to adiabatic mode!
-- so in Senatore & Z., the entropy modes are added into a base with
already known adiabatic mode!
but
-- in our case we started with zeroth order term of perturbations.
   -- then defined the perturbations without any      distinguishability
between adiabatic and entropy modes!
compare with Senatore & Zaldarriaga

    GR + a scalar field     1       perturbation





                                                           Modification
             Modification






                                                             (EFT)
               (EFT)












            2                                      3


Cheung et al. and Senatore & Z.: 0 perturbation
                                          1            3
Weinberg and this talk: 0       2        3













compare with Senatore & Zaldarriaga


    so in Senatore & Zaldarriaga, the shift symmetry results in a
      Lagrangian similar to














i.e. there are just derivatives of adiabatic and entropy perturbations!
                               but in our model the case is different!




compare with Senatore & Zaldarriaga

   shift symmetry:
   due to




results in




which causes a new symmetry for adiabatic and entropy modes:
conclusions

-- this model does not predict a large non-Gaussianity except:
   -- for a highly curved classical path in phase-space!
   -- or if a shielding mechanism allows large first correction
term in EFT.
-- different shapes of non-Gaussianity are correlated!
-- in contrast to Senatore & Zaldarriaga, we suggest EFT for
multi-filed inflation should be constructed as
thank you!
























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Effective Field Theory of Multifield Inflation

  • 1. Effective Field Theory of Multi-Field Inflation a la Weinberg Nima Khosravi African Institute for Mathematical Sciences arXiv:1203.2266
  • 2. map:  keywords: Effective Field Theory, Inflation
  • 3. Effective Field Theory  an effective theory:  is true for a certain domain of energy.   two cases:  as a part of a true theory for whole energy scales  using EFT to simplify calculations!  in lack of a complete theory for the energy scales of interests  using EFT since there is no other choice!  constructing EFT, by considering e.g. symmetry properties of the model. 
  • 4. EFT for Multi-Field Inflation  the most general form of Lagrangian up to the 4th order derivatives: after simplifications: before simplifications!
  • 5. perturbations:  perturbations in single field model (Weinberg’s paper)     -- it is up to 4th order of perturbations automatically. -- speed of sound ≠ 1 -- large non-Gaussianity ? -- speed of sound is constrained by validity of EFT!  
  • 6. perturbations:  multi-field case: background terms:       perturbations!
  • 7. perturbations:  two-field case: the most general form of the Lagrangian: second order perturbations! …. and cubic and quartic terms! . . . transition to adiabatic and entropy curvature perturbations! 
  • 8. perturbations: adiabatic & entropy modes  adiabatic mode: entropy mode:        Gordon et al. arXiv:astro-ph/0009131 
  • 9. perturbations: adiabatic & entropy modes  as an example: second order perturbation terms (containing time derivatives) due to correction term: note that just these two combinations appear in this formalism!
  • 10. shape of non-Gaussianity  due to previous slide: for example: equilateral NG local NG in adiabatic mode in entropy mode --- in this formalism the “Cosine” between different kinds of NG is fixed!
  • 11. amplitude of NG      -- validity condition of EFT i.e. constrains the amplitude of NG! -- except if the curvature of classical (background) path be large! -- or: if by a mechanism (e.g. Vainshtein) one can modify the validity condition of EFT!
  • 12. compare with Senatore & Zaldarriaga -- Senatore & Zaldarriaga model is based on Cheung et al.’s work! -- in Cheung’s work, EFT is constructed on perturbations’ level! -- since their model is single field, the perturbation is associated to adiabatic mode! -- so in Senatore & Z., the entropy modes are added into a base with already known adiabatic mode! but -- in our case we started with zeroth order term of perturbations. -- then defined the perturbations without any distinguishability between adiabatic and entropy modes!
  • 13. compare with Senatore & Zaldarriaga GR + a scalar field 1 perturbation  Modification Modification  (EFT) (EFT)   2 3 Cheung et al. and Senatore & Z.: 0 perturbation 1 3 Weinberg and this talk: 0 2 3    
  • 14. compare with Senatore & Zaldarriaga  so in Senatore & Zaldarriaga, the shift symmetry results in a Lagrangian similar to     i.e. there are just derivatives of adiabatic and entropy perturbations! but in our model the case is different!  
  • 15. compare with Senatore & Zaldarriaga shift symmetry: due to results in which causes a new symmetry for adiabatic and entropy modes:
  • 16. conclusions -- this model does not predict a large non-Gaussianity except: -- for a highly curved classical path in phase-space! -- or if a shielding mechanism allows large first correction term in EFT. -- different shapes of non-Gaussianity are correlated! -- in contrast to Senatore & Zaldarriaga, we suggest EFT for multi-filed inflation should be constructed as