bosonic higher curvature gravity
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BOSONIC HIGHER-CURVATURE GRAVITY SET 8 G = 1 EINSTEIN ACTION PLUS - PowerPoint PPT Presentation

SINGLE-FIELD INFLATION MODELS IN SUPERGRAVITY GRAVITY AS GRAVITY + SCALAR f ( R ) THE STAROBINSKY CASE f = R + R 2 CORRECTIONS R n SUPERGRAVITY AT LINEAR ORDER R + R 2 THE NEW MINIMAL SUPERGRAVITY NEW MINIMAL


  1. SINGLE-FIELD INFLATION MODELS IN SUPERGRAVITY • GRAVITY AS GRAVITY + SCALAR f ( R ) • THE “STAROBINSKY” CASE f = R + α R 2 • CORRECTIONS R n • SUPERGRAVITY AT LINEAR ORDER R + α R 2 • THE NEW MINIMAL SUPERGRAVITY • NEW MINIMAL COMPLETION OF R + α R 2 GRAVITY • HIGHER-CURVATURE CORRECTIONS • NEW MINIMAL CHAOTIC INFLATION AND F TERMS

  2. BOSONIC HIGHER-CURVATURE GRAVITY SET 8 π G = 1 EINSTEIN ACTION PLUS HIGHER-CURVATURE CORRECTIONS L = 1 2 R + f ( R ) = 1 2 R + f ( X ) + 1 2 Y ( R − X )

  3. BOSONIC HIGHER-CURVATURE GRAVITY SET 8 π G = 1 EINSTEIN ACTION PLUS HIGHER-CURVATURE CORRECTIONS L = 1 2 R + f ( R ) = 1 2 R + f ( X ) + 1 2 Y ( R − X ) RESCALE TO EINSTEIN FRAME g mn → (1 + Y ) − 1 g mn (1 + Y ) √− gR → √− gR − 3 √− g [ ∂ m log(1 + Y )] 2 2

  4. THE LAGRANGIAN DENSITY BECOMES L = 1 2 R − 1 2( ∂ m φ ) 2 − (1 + Y ) − 2 ˜ f [ Y ( φ )] p φ = 3 / 2 log(1 + Y ) ˜ f ( Y ) = Y X − f ( X ) | f 0 ( X )= Y LEGENDRE TRANSFORM

  5. THE LAGRANGIAN DENSITY BECOMES L = 1 2 R − 1 2( ∂ m φ ) 2 − (1 + Y ) − 2 ˜ f [ Y ( φ )] p φ = 3 / 2 log(1 + Y ) ˜ f ( Y ) = Y X − f ( X ) | f 0 ( X )= Y LEGENDRE TRANSFORM 1 2 g 2 X 2 IN PARTICULAR, WHEN f ( X ) = f ( Y ) = g 2 2 / 3 φ ⌘ 2 1 − e − √ (1 + Y ) − 2 ˜ ⇣ THE POTENTIAL IS 2

  6. THE “STAROBINSKY” POTENTIAL (VERTICAL AXIS SCALE MULTIPLIED BY ) 8 /g 2 5 5 4 4 3 3 2 2 1 1 2 2 4 4 6 6 8 8 10 10 -1 -1

  7. HIGHER ORDER CORRECTIONS: WHICH SCALE? 2 g 2 R 2 → Rf ( R/g 2 ) , f ( x ) = 1 + 1 1 2 x + O (1) x 4 + ... R + WHEN CURVATURE IS ALL TERMS ARE EQUAL O ( g 2 ) IS IT POSSIBLE TO GET ANOTHER FACTOR O ( g 2 ) IN FRONT OF THE HIGHER CURVATURE CORRECTIONS? WHAT ABOUT CHAOTIC INFLATION? T.B.C.........

  8. SUPERSYMMETRIZATION OF f(R) GRAVITY • GRAVITON (OFF SHELL) DEGREES OF FREEDOM: 10-4=6 • GRAVITINO DEGREES OF FREEDOM 16-4=12 • WE NEED AT LEAST 6 BOSONIC DEGREES OF FREEDOM (AUXILIARY FIELDS)

  9. SUPERSYMMETRIZATION OF f(R) GRAVITY • GRAVITON (OFF SHELL) DEGREES OF FREEDOM: 10-4=6 • GRAVITINO DEGREES OF FREEDOM 16-4=12 • WE NEED AT LEAST 6 BOSONIC DEGREES OF FREEDOM (AUXILIARY FIELDS) • TWO CONVENIENT CHOICES: • OLD MINIMAL: 4+2 DOF A µ , S + iP • NEW MINIMAL: 3+3 DOF B µ ν , A µ

  10. SUPERSYMMETRIZATION OF f(R) GRAVITY • GRAVITON (OFF SHELL) DEGREES OF FREEDOM: 10-4=6 • GRAVITINO DEGREES OF FREEDOM 16-4=12 • WE NEED AT LEAST 6 BOSONIC DEGREES OF FREEDOM (AUXILIARY FIELDS) • TWO CONVENIENT CHOICES: • OLD MINIMAL: 4+2 DOF A µ , S + iP • NEW MINIMAL: 3+3 DOF B µ ν , A µ NO GAUGE INVARIANCE

  11. SUPERSYMMETRIZATION OF f(R) GRAVITY • GRAVITON (OFF SHELL) DEGREES OF FREEDOM: 10-4=6 • GRAVITINO DEGREES OF FREEDOM 16-4=12 • WE NEED AT LEAST 6 BOSONIC DEGREES OF FREEDOM (AUXILIARY FIELDS) • TWO CONVENIENT CHOICES: • OLD MINIMAL: 4+2 DOF A µ , S + iP • NEW MINIMAL: 3+3 DOF B µ ν , A µ NO GAUGE INVARIANCE GAUGE INVARIANCE B µ ν → B µ ν + ∂ [ µ ξ ν ] , A µ → A µ + ∂ µ ξ

  12. OLD MINIMAL AND NEW MINMAL DIFFER BY NON PROPAGATING DEGREES OF FREEDOM IN STANDARD “EINSTEIN” SUPERGRAVITY; WHEN HIGHER CURVATURE TERMS ARE INTRODUCED THEY AUXILIARY FIELDS PROPAGATE AND THE TWO FORMALISMS ARE NO LONGER EQUIVALENT

  13. CONSIDER FIRST THE SUPERSYMMETRIZATION OF THE ACTION R + α R 2

  14. CONSIDER FIRST THE SUPERSYMMETRIZATION OF THE ACTION R + α R 2 THE ANALYSIS OF THIS ACTION WAS DONE IN THE OLD MINIMAL FORMALISM AT QUADRATIC LEVEL BY FERRARA, GRISARU AND VAN NIEUWENHUIZEN IN 1978 AND AT NON-LINEAR LEVEL BY CECOTTI IN 1987

  15. CONSIDER FIRST THE SUPERSYMMETRIZATION OF THE ACTION R + α R 2 THE ANALYSIS OF THIS ACTION WAS DONE IN THE OLD MINIMAL FORMALISM AT QUADRATIC LEVEL BY FERRARA, GRISARU AND VAN NIEUWENHUIZEN IN 1978 AND AT NON-LINEAR LEVEL BY CECOTTI IN 1987 ANALYSIS IN THE NEW MINIMAL FORMALISM: 1988, CECOTTI, FERRARA, M.P . AND SABHARWAL

  16. • EXTRA PROPAGATING DEGREES OF FREEDOM IN BOTH OLD AND NEW MINIMAL: (4B,4F)

  17. • EXTRA PROPAGATING DEGREES OF FREEDOM IN BOTH OLD AND NEW MINIMAL: (4B,4F) • IN OLD MINIMAL THEY FORM TWO CHIRAL MULTIPLETS [1/2,(2)0], [1/2,(2)0]

  18. • EXTRA PROPAGATING DEGREES OF FREEDOM IN BOTH OLD AND NEW MINIMAL: (4B,4F) • IN OLD MINIMAL THEY FORM TWO CHIRAL MULTIPLETS [1/2,(2)0], [1/2,(2)0] • IN NEW MINIMAL THEY FORM ONE VECTOR MULTIPLET [1,(2)1/2,0]

  19. • EXTRA PROPAGATING DEGREES OF FREEDOM IN BOTH OLD AND NEW MINIMAL: (4B,4F) • IN OLD MINIMAL THEY FORM TWO CHIRAL MULTIPLETS [1/2,(2)0], [1/2,(2)0] • IN NEW MINIMAL THEY FORM ONE VECTOR MULTIPLET [1,(2)1/2,0] IN OLD-MINIMAL, THE BOSONIC PART OF THE ACTION IS R + S 2 + P 2 + A 2 µ + α [( ∂ µ S ) 2 + ( ∂ µ P ) 2 + ( ∂ µ A µ ) 2 + R 2 ]

  20. • EXTRA PROPAGATING DEGREES OF FREEDOM IN BOTH OLD AND NEW MINIMAL: (4B,4F) • IN OLD MINIMAL THEY FORM TWO CHIRAL MULTIPLETS [1/2,(2)0], [1/2,(2)0] • IN NEW MINIMAL THEY FORM ONE VECTOR MULTIPLET [1,(2)1/2,0] IN OLD-MINIMAL, THE BOSONIC PART OF THE ACTION IS R + S 2 + P 2 + A 2 µ + α [( ∂ µ S ) 2 + ( ∂ µ P ) 2 + ( ∂ µ A µ ) 2 + R 2 ] ONE SCALAR GRAVITON PLUS ONE SCALAR

  21. THE OLD MINIMAL SUPERSYMMETRIZATION OF ACTIONS WITH HIGHER POWERS OF THE SCALAR CURVATURE CONTAINS FOUR SCALARS. IN THE SIMPLEST REALIZATIONS OF INFLATIONARY POTENTIALS THESE SCALARS MAY BECOME UNSTABLE DURING SLOW ROLL. THE NEW MINIMAL FORMALISM HAS ONLY ONE (STABLE) SCALAR.

  22. THE OLD MINIMAL SUPERSYMMETRIZATION OF ACTIONS WITH HIGHER POWERS OF THE SCALAR CURVATURE CONTAINS FOUR SCALARS. IN THE SIMPLEST REALIZATIONS OF INFLATIONARY POTENTIALS THESE SCALARS MAY BECOME UNSTABLE DURING SLOW ROLL. THE NEW MINIMAL FORMALISM HAS ONLY ONE (STABLE) SCALAR. THE SUPERMULTIPLET CONTAINING THE DEGREES OF FREEDOM RELEVANT TO A NEW MINIMAL SUPERSYMMETRIZATION OF ACTIONS WITH HIGHER POWERS OF THE SCALAR CURVATURE CAN BE WRITTEN AT THE FULL NON-LINEAR LEVEL USING SUPECONFORMAL CALCULUS

  23. CONFORMAL CALCULUS: (ADD DILATON DOF AND WEYL INVARIANCE TO REMOVE IT) g µ ν ≡ φ 2 g µ ν s.t. g µ ν → Ω 2 g µ ν , φ → Ω − 1 φ g µ ν → ˆ

  24. CONFORMAL CALCULUS: (ADD DILATON DOF AND WEYL INVARIANCE TO REMOVE IT) g µ ν ≡ φ 2 g µ ν s.t. g µ ν → Ω 2 g µ ν , φ → Ω − 1 φ g µ ν → ˆ SUPERCONFORMAL CALCULUS: (ADD DILATON CHIRAL MULTIPLET AND SUPER-WEYL INVARIANCE TO REMOVE IT) THE BOSONIC PART OF SUPER-WEYL CONTAINS SCALE PLUS CHIRAL TRANSFORMATION: SUPER- WEYL MULTIPLETS ARE CLASSIFIED BY CHARGE AND SCALING DIMENSION

  25. THE NEW MINIMAL EINSTEIN ACTION DEPENDS ON A CHIRAL COMPENSATOR WITH (SCALING DIMENSION,CHIRAL WEIGHT)=(1,1) AND A LINEAR MULTIPLET WITH WEIGHTS (2,0) V R = log( L/S ¯ L E = [ LV R ] D , S ) θ 2 TERM θ 2 ¯

  26. THE NEW MINIMAL EINSTEIN ACTION DEPENDS ON A CHIRAL COMPENSATOR WITH (SCALING DIMENSION,CHIRAL WEIGHT)=(1,1) AND A LINEAR MULTIPLET WITH WEIGHTS (2,0) V R = log( L/S ¯ L E = [ LV R ] D , S ) θ 2 TERM θ 2 ¯ CHIRAL MULTIPLET ¯ D α S = 0

  27. THE NEW MINIMAL EINSTEIN ACTION DEPENDS ON A CHIRAL COMPENSATOR WITH (SCALING DIMENSION,CHIRAL WEIGHT)=(1,1) AND A LINEAR MULTIPLET WITH WEIGHTS (2,0) V R = log( L/S ¯ L E = [ LV R ] D , S ) θ 2 TERM θ 2 ¯ CHIRAL MULTIPLET ¯ D α S = 0 θσ µ θ A µ + .., ∂ µ A µ = 0 D 2 L = ¯ D 2 L = 0 → L = ... + ¯ LINEAR MULTIPLET

  28. THE ACTION IS INDEPENDENT OF THE CHIRAL COMPENSATOR BECAUSE IT CAN BE SCALED TO A CONSTANT WITH A GAUGE TRANSFORMATION PARAMETRIZED BY A CHIRAL SUPERFIELD S → S 0 = e Ω S, S 0 = 1 , V R → V R + Ω + ¯ Ω THE EINSTEIN TERM IS INVARIANT BECAUSE [ L ( Ω + ¯ Ω )] D = 0

  29. THE ACTION IS INDEPENDENT OF THE CHIRAL COMPENSATOR BECAUSE IT CAN BE SCALED TO A CONSTANT WITH A GAUGE TRANSFORMATION PARAMETRIZED BY A CHIRAL SUPERFIELD S → S 0 = e Ω S, S 0 = 1 , V R → V R + Ω + ¯ Ω THE EINSTEIN TERM IS INVARIANT BECAUSE [ L ( Ω + ¯ Ω )] D = 0 HIGHER ORDER TERMS ARE WRITTEN IN TERMS OF THE GAUGE-INVARIANT FIELD STRENGTH W α ( V R ) = ¯ D 2 D α V R = θ α R + ...

  30. THE NEW MINIMAL ACTION R + α R 2 1 2 g 2 [ W 2 L = [ LV R ] D + α ( V R )] F + c.c. θ 2 TERM THE ACTION IS DUAL TO A STANDARD SUPERGRAVITY ACTION DESCRIBING GRAVITON+GRAVITINO PLUS A MASSIVE VECTOR MULTIPLET [1,(2)1/2, 0] (CECOTTI, FERRARA, M.P ., SABHARWAL, 1988; RIOTTO, KEHAGIAS, 2013)

  31. THE NEW MINIMAL ACTION R + α R 2 1 2 g 2 [ W 2 L = [ LV R ] D + α ( V R )] F + c.c. θ 2 TERM THE ACTION IS DUAL TO A STANDARD SUPERGRAVITY ACTION DESCRIBING GRAVITON+GRAVITINO PLUS A MASSIVE VECTOR MULTIPLET [1,(2)1/2, 0] (CECOTTI, FERRARA, M.P ., SABHARWAL, 1988; RIOTTO, KEHAGIAS, 2013) TRICK: INTRODUCE AN UNCONSTRAINED REAL MULTIPLET AS LAGRANGE MULTIPLIER: R

  32. 1 L = − [ S ¯ Se U U ] D + [ R ( S ¯ Se U − L )] D + 2 g 2 [ W 2 α ( U )] F + c.c. ACTION DOES NOT DEPEND ON BECAUSE OF GAUGE S INVARIANCE S → Se Y , U → U − Y − ¯ R → R − Y − ¯ Y , Y

  33. 1 L = − [ S ¯ Se U U ] D + [ R ( S ¯ Se U − L )] D + 2 g 2 [ W 2 α ( U )] F + c.c. ACTION DOES NOT DEPEND ON BECAUSE OF GAUGE S INVARIANCE S → Se Y , U → U − Y − ¯ R → R − Y − ¯ Y , Y SOLVE E.O.M. OF REAL MULTIPLET TO GET NEW R MINIMAL ACTION

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