STABILIZING EXTRA DIMENSIONS

Transcription

1 STABILIZING EXTRA DIMENSIONS Gero von Gersdorff (École Polytechnique) Warsaw, October 19th 2009 Collaboration with J.A.Cabrer and M.Quirós

2 OUTLINE Features of Warped Extra Dimensions Stabilizing Models with 2 branes Soft Wall models (Models with 1 brane) Stabilizing the Soft Wall (Soft Walls and the Cosmological Constant)

3 OPEN QUESTIONS IN THE SM (AND BEYOND) What is the origin of Electroweak Symmetry Breaking? Why is the scale of the Z and W bosons times smaller than the Planck mass? (Hierarchy Problem) Why is there such a huge hierarchy in the masses of the Standard Model fermions? What is the origin of neutrino masses? If there is Supersymmetry, how is it broken? If there is a Grand Unified Theory, how is it broken to the SM, and why are there no colored Higgses?

4 All these issues can be addressed in models with Extra Dimensions

5 RS MODELS Randall & Sundrum 99

6 RS MODELS Randall & Sundrum 99 4D Boundary Fifth Dimension 4D Boundary

7 RS MODELS Randall & Sundrum 99 ds 2 = e 2 ky dx µ dx ν η µν + dy 2 Warp factor 4D Boundary Fifth Dimension 4D Boundary

8 RS MODELS Randall & Sundrum 99 ds 2 = e 2 ky dx µ dx ν η µν + dy 2 Warp factor 4D Boundary Fifth Dimension 4D Boundary

9 RS MODELS Randall & Sundrum 99 ds 2 = e 2 ky dx µ dx ν η µν + dy 2 Warp factor 4D Boundary Fifth Dimension M 5d M 5d e ky 1M 5d e ky 4D Boundary Fundamental cutoff scale is redshifted

10 RS MODELS Randall & Sundrum 99 ds 2 = e 2 ky dx µ dx ν η µν + dy 2 Higgs Warp factor 4D Boundary Fifth Dimension M 5d M 5d e ky 1M 5d e ky 4D Boundary Fundamental cutoff scale is redshifted

11 RS MODELS Randall & Sundrum 99 ds 2 = e 2 ky dx µ dx ν η µν + dy 2 Higgs Warp factor 4D Boundary Fifth Dimension M 5d M 5d e ky 1M 5d e ky 4D Boundary Fundamental cutoff scale is redshifted

12 FERMION MASSES Arkani-Hamed & Schmalz 00, Shifman & Dvali 00, Gherghetta & Pomarol 00

13 FERMION MASSES Arkani-Hamed & Schmalz 00, Shifman & Dvali 00, Gherghetta & Pomarol 00 Higgs UV Brane IR brane

14 FERMION MASSES 5D fields Wave functions q(x µ,y)=q 0 (y) q 0 (x µ ) (+ KK modes) 4D fields Higgs Arkani-Hamed & Schmalz 00, Shifman & Dvali 00, Gherghetta & Pomarol 00 UV Brane IR brane

15 FERMION MASSES 5D fields Wave functions q(x µ,y)=q 0 (y) q 0 (x µ ) (+ KK modes) 4D fields Higgs Arkani-Hamed & Schmalz 00, Shifman & Dvali 00, Gherghetta & Pomarol 00 UV Brane Fermions: 5D masses control localization of wave functions IR brane Y 4D = Y 5d Q 0 (y 1 ) U 0 (y 1 ) - Localize heavy fermions on IR brane - Localize light fermions on UV brane

16 SUMMARY RS MODELS

17 SUMMARY RS MODELS Extra Dimensions with WARPED background successful for Explaining electroweak hierarchy Explaining fermion mass hierarchy

18 SUMMARY RS MODELS Extra Dimensions with WARPED background successful for Explaining electroweak hierarchy Explaining fermion mass hierarchy Other features Distinctive Collider Signature (KK gravitons) Dual to strongly coupled gauge theories in 4D Modelling QCD

19 PROBLEMS Pure 5D Gravity with negative Cosmological constant (and appropriate brane tensions) has RS as a solution. BUT: Interbrane distance is UNDETERMINED There is an extra massless mode (RADION) g MN = g RS MN + Both brane tensions need to be fine tuned ( hµν h55)

20 STABILIZATION The question of Radius stabilization What determines DISTANCE between UV and IR brane? How can I generate a POTENTIAL and a MASS for the Radion? What ensures that the 4D metric is FLAT? How NATURAL is it?

21 SUPERPOTENTIAL METHOD

22 SUPERPOTENTIAL METHOD Gravity + scalar field with bulk and brane potential ds 2 = e 2A(y) dx µ dx ν η µν + dy 2 λ 0 (φ) λ 1 (φ) Solve Einstein equations coupled to scalar V (φ)

23 SUPERPOTENTIAL METHOD Gravity + scalar field with bulk and brane potential ds 2 = e 2A(y) dx µ dx ν η µν + dy 2 λ 0 (φ) λ 1 (φ) Solve Einstein equations coupled to scalar V (φ) Define a Superpotential V (φ) =3W (φ) 2 12W 2 (φ) NO SUSY INVOLVED Einstein equations become φ (y) =W (φ) A (y) =W (φ) Boundary values from Minimizing the 4D potentials DeWolfe et al 99, Brandhuber & Sfetsos 99 V i (φ) =λ i (φ) 6 W (φ)

24 STABILIZATION

25 STABILIZATION - Solve to get bulk profiles - Minimize to get brane values φ (y) =W (φ) A (y) =W (φ) V i (φ i )=λ i (φ i ) 6 W (φ i )

26 STABILIZATION - Solve to get bulk profiles - Minimize to get brane values φ (y) =W (φ) A (y) =W (φ) V i (φ i )=λ i (φ i ) 6 W (φ i ) - Notice that e ky 1 = = ky Choose some suitable W such that φ1 1 ky 1 = φ W Now shift superpotential W W + k A(y) A(y)+ky - Adds warping without changing the value of ky 1 DeWolfe et al 00, Cabrer, GG & Quirós 09

27 GOLDBERGER WISE Goldberger & Wise 99 - Take W (φ) =kbφ - Then ky 1 = b 1 log φ 1 /φ Moderate fine tuning necessary - Metric A(y) =ky φ2 0 (e 2 b k y 1) Warping - Backreaction small: Exact Backreaction BR ky <.01 for b 1 = 37, φ 0 =1/e, φ 1 =1

28 Do we need two branes?

29 GAUGE/GRAVITY DUALITY

30 GAUGE/GRAVITY DUALITY Gravity/Gauge theory correspondence stipulates that the 5D theory is dual to a strongly coupled 4D gauge theory that is approximately conformal in the UV has large number of colors describes the same physics as 5D theory

31 GAUGE/GRAVITY DUALITY Gravity/Gauge theory correspondence stipulates that the 5D theory is dual to a strongly coupled 4D gauge theory that is approximately conformal in the UV has large number of colors describes the same physics as 5D theory KK modes correspond to resonances of gauge theory RS with two branes: KK spectrum is roughly m 2 n n 2 4D strongly coupled gauge theories have many more possibilities.

32 POSSIBLE SPECTRA ρ(m 2 ) Regge M 2 n ρ(m 2 ) RS M 2 n 2 ρ(m 2 ) Conformal M 2 ρ(m 2 ) M 2 Conformal + Gap (Unparticles) M 2 M 2

33 IR brane can be replaced by SOFT WALL

34 SOFT WALLS

35 SOFT WALLS Soft Walls models only possess a single (UV) brane, but nevertheless exhibit a finite length in the 5th dimension. The IR brane is replaced by a curvature singularity at which the metric vanishes.

36 SOFT WALLS Soft Walls models only possess a single (UV) brane, but nevertheless exhibit a finite length in the 5th dimension. The IR brane is replaced by a curvature singularity at which the metric vanishes. A(y) φ(y) y y s

37 SOFT WALLS Soft Walls models only possess a single (UV) brane, but nevertheless exhibit a finite length in the 5th dimension. The IR brane is replaced by a curvature singularity at which the metric vanishes. A(y) φ(y) Profiles diverge at finite y if W (φ) φ 2 or faster! y y s

38 APPLICATIONS

39 APPLICATIONS Things that CAN be done with Soft Walls Electroweak Breaking Strong interactions (AdS/QCD) Batell, Gherghetta & Sword 08, Falkowski & Perez-V. 08, Cabrer, GG & Quiros (in progr.) Karch et al 06, Gursoy et al 07, Batell & Gherghetta 08,

40 APPLICATIONS Things that CAN be done with Soft Walls Electroweak Breaking Strong interactions (AdS/QCD) Batell, Gherghetta & Sword 08, Falkowski & Perez-V. 08, Cabrer, GG & Quiros (in progr.) Karch et al 06, Gursoy et al 07, Batell & Gherghetta 08, Things that CANNOT be done with Soft Walls Solve Cosmological Constant problem Arkani-Hamed et al 00, Kachru, Schulz & Silverstein 00, Csaki et al 00 Forste et al 00, Cabrer, GG & Quirós 09

41 SPECTRA WITH SOFT WALLS

42 SPECTRA WITH SOFT WALLS Even though the physical length is finite, the conformal length might be either finite or infinite: Proper Length coordinates ds 2 = e 2A(y) dx µ dx ν η µν + dy 2 Conformally flat coordinates ds 2 = e 2A(z) (dx µ dx ν η µν + dz 2 ) y s <, z s = z(y s ) can be finite or infinite

43 SPECTRA WITH SOFT WALLS Even though the physical length is finite, the conformal length might be either finite or infinite: Proper Length coordinates ds 2 = e 2A(y) dx µ dx ν η µν + dy 2 Conformally flat coordinates ds 2 = e 2A(z) (dx µ dx ν η µν + dz 2 ) y s <, z s = z(y s ) can be finite or infinite In the conformally flat frame, the KK spectrum of any bulk field follows a Schrödinger Equation ψ (z)+ ˆV (z)ψ(z) =m 2 ψ(z) Depends on the background

44 NON CONFINING POTENTIALS Conformal length infinite ˆV (z) Conformal (continuous) ˆV (z) Unparticle (continuous + gap) z CONFINING POTENTIALS Conformal length finite or infinite z Regge: M 2 n RS like: M 2 n 2 ˆV (z) ˆV (z) z z z s

45 SOFT WALL SPECTRA φ W (φ) 2 > φ 2 e φ e φ φ β >e φ φ 1 2 e 2φ <e φ 0 < β 1 2 <e 2φ y s finite z s finite mass continuous discrete continuous spectrum w/ mass gap m n n 2β m n n consistent yes no solution Gursoy et al 07, Cabrer, GG & Quirós 09

46 SOFT WALL SPECTRA φ W (φ) 2 > φ 2 e φ e φ φ β >e φ φ 1 2 e 2φ <e φ 0 < β 1 2 <e 2φ y s finite z s finite mass continuous discrete continuous spectrum w/ mass gap m n n 2β m n n consistent yes no solution Asymptotic behaviour of W Gursoy et al 07, Cabrer, GG & Quirós 09

47 SOFT WALL SPECTRA φ W (φ) 2 > φ 2 e φ e φ φ β >e φ φ 1 2 e 2φ <e φ 0 < β 1 2 <e 2φ y s finite z s finite mass continuous discrete continuous spectrum w/ mass gap m n n 2β m n n consistent yes no solution Asymptotic behaviour of W Singularity in proper distance Gursoy et al 07, Cabrer, GG & Quirós 09

48 SOFT WALL SPECTRA φ W (φ) 2 > φ 2 e φ e φ φ β >e φ φ 1 2 e 2φ <e φ 0 < β 1 2 <e 2φ y s finite z s finite mass continuous discrete continuous spectrum w/ mass gap m n n 2β m n n consistent yes no solution Asymptotic behaviour of W Singularity in proper distance Singularity in conformal distance Gursoy et al 07, Cabrer, GG & Quirós 09

49 SOFT WALL SPECTRA φ W (φ) 2 > φ 2 e φ e φ φ β >e φ φ 1 2 e 2φ <e φ 0 < β 1 2 <e 2φ y s finite z s finite mass continuous discrete continuous spectrum w/ mass gap m n n 2β m n n consistent yes no solution Asymptotic behaviour of W Singularity in proper distance Singularity in conformal distance Asymptotic form of the spectrum Gursoy et al 07, Cabrer, GG & Quirós 09

50 SOFT WALL SPECTRA φ W (φ) 2 > φ 2 e φ e φ φ β >e φ φ 1 2 e 2φ <e φ 0 < β 1 2 <e 2φ y s finite z s finite mass continuous discrete continuous spectrum w/ mass gap m n n 2β m n n consistent yes no solution Asymptotic behaviour of W Singularity in proper distance Singularity in conformal distance Asymptotic form of the spectrum Finite Length Gursoy et al 07, Cabrer, GG & Quirós 09

51 SOFT WALL SPECTRA φ W (φ) 2 > φ 2 e φ e φ φ β >e φ φ 1 2 e 2φ <e φ 0 < β 1 2 <e 2φ y s finite z s finite mass continuous discrete continuous spectrum w/ mass gap m n n 2β m n n consistent yes no solution Asymptotic behaviour of W Singularity in proper distance Singularity in conformal distance Asymptotic form of the spectrum Finite Length Mass gap appears Gursoy et al 07, Cabrer, GG & Quirós 09

52 SOFT WALL SPECTRA φ W (φ) 2 > φ 2 e φ e φ φ β >e φ φ 1 2 e 2φ <e φ 0 < β 1 2 <e 2φ y s finite z s finite mass continuous discrete continuous spectrum w/ mass gap m n n 2β m n n consistent yes no solution Asymptotic behaviour of W Singularity in proper distance Singularity in conformal distance Asymptotic form of the spectrum Finite Length Mass gap appears Spectrum discrete Gursoy et al 07, Cabrer, GG & Quirós 09

53 SOFT WALL STABILIZATION

54 SOFT WALL STABILIZATION - Stabilization works similar as before - Choose some suitable W such that ky s = φ 0 1 W (φ) 37 - Now shift superpotential W W + k A(y) A(y)+ky - Shift does not change position of singularity

55 SOFT WALL STABILIZATION - Stabilization works similar as before - Choose some suitable W such that ky s = φ 0 1 W (φ) 37 - Now shift superpotential W W + k A(y) A(y)+ky - Shift does not change position of singularity The Warping affects the Mass scale: - The Unparticle mass gap - The level spacing in the discrete case warped down Cabrer, GG & Quirós 09

56 PARTICULAR MODELS Consider the class of models W (φ) =k(1 + e νφ ) ky s = ν 2 e νφ 0 37 for O(1) negative values for φ 0 log 10 (ρ/k) ν =1 ν = φ 0 Spectrum can be - Continuous - Continuous+gap - Discrete

57 THE GRAVITON SPECTRUM

58 THE GRAVITON SPECTRUM m/ρ(ν) ν

59 THE GRAVITON SPECTRUM m/ρ(ν) ν gap + continuous

60 THE GRAVITON SPECTRUM m/ρ(ν) ν gap+very densely spaced discretuum

61 THE GRAVITON SPECTRUM m/ρ(ν) ν Discrete, hard-wall like

62 WAVE FUNCTIONS z s h(z) n=0 n=1 n= z/z s

63 THE RADION SPECTRUM

64 THE RADION SPECTRUM m/ρ(ν) ν

65 THE RADION SPECTRUM m/ρ(ν) ν NO ZERO MODE

66 THE CC PROBLEM

67 THE CC PROBLEM V (φ) =3W (φ) 2 12W 2 (φ) φ (y) =W (φ) A (y) =W (φ) } 3 constants of integration

68 THE CC PROBLEM V (φ) =3W (φ) 2 12W 2 (φ) φ (y) =W (φ) A (y) =W (φ) } 3 constants of integration 2 Branes: V 0(φ 0 )=0 V 0 (φ 0 V 1(φ 1 V 1 (φ 0 )=0} 4 boundary conditions

69 THE CC PROBLEM V (φ) =3W (φ) 2 12W 2 (φ) φ (y) =W (φ) A (y) =W (φ) } 3 constants of integration 2 Branes: V 0(φ 0 )=0 V 0 (φ 0 V 1(φ 1 V 1 (φ 0 )=0} 4 boundary conditions 1 fine tuning

70 THE CC PROBLEM V (φ) =3W (φ) 2 12W 2 (φ) φ (y) =W (φ) A (y) =W (φ) } 3 constants of integration 1 Brane: V 0(φ 0 )=0 V 0 (φ 0 )=0 } 2 boundary conditions

71 THE CC PROBLEM V (φ) =3W (φ) 2 12W 2 (φ) φ (y) =W (φ) A (y) =W (φ) } 3 constants of integration 1 Brane: V 0(φ 0 )=0 V 0 (φ 0 )=0 } 2 boundary conditions No fine tuning??

72 THE CC PROBLEM This is incorrect!!! Forste et al 00, Cabrer, GG & Quirós 09

73 THE CC PROBLEM This is incorrect!!! Forste et al 00, Cabrer, GG & Quirós 09 4D CC = dy L on shell! =0

74 THE CC PROBLEM This is incorrect!!! Forste et al 00, Cabrer, GG & Quirós 09 4D CC = dy L on shell = lim y y s W [φ(y)]e 4A(y)

75 THE CC PROBLEM This is incorrect!!! Forste et al 00, Cabrer, GG & Quirós 09 4D CC = dy L on shell = lim y y s W [φ(y)]e 4A(y) - There is a contribution to the CC from the singularity!

76 THE CC PROBLEM This is incorrect!!! Forste et al 00, Cabrer, GG & Quirós 09 4D CC = dy L on shell = lim y y s W [φ(y)]e 4A(y) - There is a contribution to the CC from the singularity! - Equations of motion are NOT satisfied at the singularity

77 THE CC PROBLEM This is incorrect!!! Forste et al 00, Cabrer, GG & Quirós 09 4D CC = dy L on shell = lim y y s W [φ(y)]e 4A(y) - There is a contribution to the CC from the singularity! - Equations of motion are NOT satisfied at the singularity - Can be fixed by choosing the integration constant for W

78 THE CC PROBLEM This is incorrect!!! Forste et al 00, Cabrer, GG & Quirós 09 4D CC = dy L on shell = lim y y s W [φ(y)]e 4A(y) - There is a contribution to the CC from the singularity! - Equations of motion are NOT satisfied at the singularity - Can be fixed by choosing the integration constant for W - Fine tuning is restored

79 CONCLUSIONS RS models provide neat way of obtaining electroweak and fermion mass hierarchy Stabilization can be achieved by adding extra scalar field IR brane can be consistently replaced by Soft Walls Spectra of Soft Wall models richer than in usual RS (gapped continuum, gapped, discretuum, Regge-like, etc.) Stabilization can be achieved without ANY fine tuning