The Spectrum of Fluctuations in the · 2016. 2. 17. · Starobinsky + term to fix direcon in...

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Transcript of The Spectrum of Fluctuations in the · 2016. 2. 17. · Starobinsky + term to fix direcon in...

Page 1: The Spectrum of Fluctuations in the · 2016. 2. 17. · Starobinsky + term to fix direcon in complex T plane • Isocurvature effects on curvature perturbations may suppress tensor/scalar
Page 2: The Spectrum of Fluctuations in the · 2016. 2. 17. · Starobinsky + term to fix direcon in complex T plane • Isocurvature effects on curvature perturbations may suppress tensor/scalar
Page 3: The Spectrum of Fluctuations in the · 2016. 2. 17. · Starobinsky + term to fix direcon in complex T plane • Isocurvature effects on curvature perturbations may suppress tensor/scalar

The Spectrum of Fluctuations in the Cosmic Microwave Background

The position of the first peak à total density ΩTot

The other peaks depend on density of ordinary matter Ωatoms & dark matter ΩDark

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First No-Scale Supergravity Model of Inflation

•  No ‘holes’ in effective potential with negative cosmological constant

JE, Enqvist, Nanopoulos, Olive & Srednicki, 1984

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•  A no-scale supergravity model of inflation that interpolates between Planck and BICEP2:

•  Identify inflaton with components of modulus T:

•  Effective Lagrangian:

A No-Scale Inflationary Model to Fit Them All

JE, García, Nanopoulos & Olive, arXiv:1405.0271

Starobinsky Quadra0c

Mo0vatedbyorbifoldcompac0fica0on

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A No-Scale Inflationary Model to Fit Them All

JE, García, Nanopoulos & Olive, arXiv:1405.0271

Starobinsky

Quadra0c

Starobinsky

+termtofixdirec0onincomplexTplane

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•  Isocurvature effects on curvature perturbations may suppress tensor/scalar ratio r

•  ns, r, non-Gaussianity dependences on initial values

Two-Field Analysis of No-Scale Inflationary Model

JE, García, Nanopoulos & Olive, arXiv:1409.8197

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No-Scale Framework for Particle Physics & Dark Matter

•  Incorporating LHC constraints, Higgs mass, flavour, supersymmetric dark matter, Starobinsky-like inflation, leptogenesis, neutrino masses, …

JE, Nanopoulos & Olive, arXiv:1310.4770

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No-Scale Framework for Particle Physics & Dark Matter

•  Incorporating LHC constraints, Higgs mass, flavour, supersymmetric dark matter, Starobinsky-like inflation, leptogenesis, neutrino masses, …

JE, Nanopoulos & Olive, arXiv:1310.4770

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Observedconstraints:8 TeV: ! !! → !! ≈ !.! ± !.! !" CMS 1σ ,!.! ± !.! !" ATLAS 1σ ,< !.! !" (95% CL)13 TeV: ! !! → !! ≈ ! ± ! !" CMS 1σ ,!" ± ! !" (ATLAS 1σ) MS≈750GeVΓ ≈ 5 − 45 GeV!!!!!!!!!

≈ 7×10!! (Γ = 5 GeV)!!!!!!!!!≈ 6×10!! (Γ = 45 GeV)

F-SU(5)Model! = !!!"!"!!! + !!!"!!"!! + !!!"#!"! + !!!"#!"! + !!!"#!"! + !!!"#!"! +!!"!"!"! +!!"!"!"! +!!"!"!"! +!!"!"!"! Γ!! = !!" !

!! !!where!!" = !!"!!

!!!!!!

!!!!!"! !! +!!!!!!!!

! !!!!!"! !!!! Γ!! = ! !! !

! !!where!! = !!!!

!!!!!!

!!!!! +!!!!!!!!

! !!!!!!! Results:!!" = 860 − 1200 GeV !!" = 735 − 1100 GeV !!" = 200 − 400 GeV !!" = 1209 − 1697 GeV !!" = 1039 − 1556 GeV !!" = 283 − 566 GeV !! = 0.80 − 0.83 !! = 0.70 − 0.83 !! = 0.31Γ = 5 GeV: Γ!! = 0.0005 − 0.0016 GeV Γ!! = 0.53 − 0.93 GeV !! = 2500 − 3000 GeV !! = 2200 − 3000 GeV !! = 1200 − 2400 GeV BR ! → !! = 0.010 − 0.032% BR ! → !! = 11 − 19% BR ! → !"!"! + !"!" = 0 − 35% BR ! → !" = 50 − 81% Γ = 45 GeV: Γ!! = 0.0005 − 0.0017 GeV Γ!! = 0.41 − 0.95 GeV !! = 2565 − 3600 GeV !! = 2205 − 3300 GeV !! = 1500 − 2400 GeV BR ! → !! = 0.0012 − 0.0037% BR ! → !! = 0.9 − 2.1% BR ! → !"!"! + !"!" = 0 − 2.6% BR ! → !" = 95.6 − 97.9%

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