1. Coupled Dark Energy and Dark Matter from dilatation symmetry

2. Cosmological Constant - Einstein - Constant λ compatible with all symmetries Constant λ compatible with all symmetries Constant λ compatible with all observations Constant λ compatible with all observations No time variation in contribution to energy density No time variation in contribution to energy density Why so small ? λ/M 4 = 10 -120 Why so small ? λ/M 4 = 10 -120 Why important just today ? Why important just today ?

3. Cosmological mass scales Energy density Energy density ρ ~ ( 2.4×10 -3 eV ) - 4 ρ ~ ( 2.4×10 -3 eV ) - 4 Reduced Planck mass M=2.44×10 18 GeV Newton’s constant G N =(8πM²) Only ratios of mass scales are observable ! homogeneous dark energy: ρ h /M 4 = 7 · 10ˉ¹²¹ homogeneous dark energy: ρ h /M 4 = 7 · 10ˉ¹²¹ matter: ρ m /M= 3 · 10ˉ¹²¹ matter: ρ m /M 4 = 3 · 10ˉ¹²¹

4. Cosm. Const | Quintessence static | dynamical

5. Quintessence Dynamical dark energy, generated by scalar field (cosmon) C.Wetterich,Nucl.Phys.B302(1988)668, 24.9.87 P.J.E.Peebles,B.Ratra,ApJ.Lett.325(1988)L17, 20.10.87

6. Cosmon Scalar field changes its value even in the present cosmological epoch Scalar field changes its value even in the present cosmological epoch Potential und kinetic energy of cosmon contribute to the energy density of the Universe Potential und kinetic energy of cosmon contribute to the energy density of the Universe Time - variable dark energy : Time - variable dark energy : ρ h (t) decreases with time ! ρ h (t) decreases with time ! V(φ) =M 4 exp( - αφ/M )

7. Two key features for realistic cosmology 1 ) Exponential cosmon potential and scaling solution scaling solution V(φ) =M 4 exp( - αφ/M ) V(φ) =M 4 exp( - αφ/M ) V(φ → ∞ ) → 0 ! V(φ → ∞ ) → 0 ! 2 ) Stop of cosmon evolution by cosmological trigger cosmological trigger e.g. growing neutrino quintessence e.g. growing neutrino quintessence

8. Evolution of cosmon field Field equations Field equations Potential V(φ) determines details of the model Potential V(φ) determines details of the model V(φ) =M 4 exp( - αφ/M ) V(φ) =M 4 exp( - αφ/M ) for increasing φ the potential decreases towards zero ! for increasing φ the potential decreases towards zero !

9. exponential potential constant fraction in dark energy can explain order of magnitude of dark energy ! Ω h = 3(4)/α 2

10. Asymptotic solution explain V( φ → ∞ ) = 0 ! effective field equations should have generic solution of this type setting : quantum effective action, all quantum fluctuations included: investigate generic form

11. realized by fixed point of runaway solution in higher dimensions : dilatation symmetry

12. Cosmon and bolon Two scalar fields : common origin from dilatation symmetric fixed point of higher dimensional theory

13. Cosmon – bolon - potential

14. Two characteristic behaviors Bolon oscillates - Bolon oscillates - if mass larger than H if mass larger than H Bolon is frozen - Bolon is frozen - if mass smaller that H if mass smaller that H

15. Cosmon and bolon Dark Energy Dark Matter

16. Early scaling solution dominated by cosmon bolon frozen and negligible bolon mass increases during scaling solution

17. Bolon oscillations ratio bolon mass / H increases ratio bolon mass / H increases bolon starts oscillating once mass larger than H bolon starts oscillating once mass larger than H subsequently bolon behaves as Dark Matter subsequently bolon behaves as Dark Matter matter radiation equality around beginning of oscillations matter radiation equality around beginning of oscillations

18. Bolon oscillations w

19. Transition to matter domination precise timing depends at this stage on initial value of bolon

20. Effective coupling between Dark Energy and Dark matter

21. Scaling solution for coupled Dark Energy

22. Realistic quintessence needs late modification modification of cosmon – bolon potential or growing neutrinos or …

23. Modification of potential for large χ : independence of initial conditions matter - radiation equality depends now on parameters of potential matter - radiation equality depends now on parameters of potential

24. Present bolon mass corresponds to range on subgalactic scales suppression of small scale Dark Matter structures ?

25. conclusions (1) Bolon : new Dark Matter candidate Bolon : new Dark Matter candidate not detectable by local observations – not detectable by local observations – direct or indirect dark matter searches direct or indirect dark matter searches perhaps observation by influence on subgalactic dark matter structures perhaps observation by influence on subgalactic dark matter structures

26. Asymptotically vanishing cosmological constant, Self-tuning and Dark Energy

27. Higher –dimensional dilatation symmetry solves cosmological constant problem

28. graviton and dilaton dilatation symmetric effective action simple example in general : many dimensionless parameters characterize effective action

29. dilatation transformations is invariant

30. flat phase generic existence of solutions of higher dimensional field equations with effective four –dimensional gravity and vanishing cosmological constant

31. torus solution example : Minkowski space x D-dimensional torus Minkowski space x D-dimensional torus ξ = const ξ = const solves higher dimensional field equations solves higher dimensional field equations extremum of effective action extremum of effective action finite four- dimensional gauge couplings finite four- dimensional gauge couplings dilatation symmetry spontaneously broken dilatation symmetry spontaneously broken generically many more solutions in flat phase !

32. massless scalars dilaton geometrical scalars ( moduli ) variation of circumference of tori change of volume of internal space bolon is associated to one such scalar

33. Higher dimensional dilatation symmetry for arbitrary values of effective couplings within a certain range : for arbitrary values of effective couplings within a certain range : higher dimensional dilatation symmetry implies existence of higher dimensional dilatation symmetry implies existence of a large class of solutions with vanishing four –dimensional a large class of solutions with vanishing four –dimensional cosmological constant cosmological constant all stable quasi-static solutions of higher dimensional field all stable quasi-static solutions of higher dimensional field equations, which admit a finite four-dimensional gravitational equations, which admit a finite four-dimensional gravitational constant and non-zero value for the dilaton, have V=0 constant and non-zero value for the dilaton, have V=0 self-tuning mechanism self-tuning mechanism

34. look for extrema of effective action for general field configurations

35. warping most general metric with maximal four – dimensional symmetry general form of quasi – static solutions ( non-zero or zero cosmological constant )

36. effective four – dimensional action flat phase : extrema of W in higher dimensions, those exist generically !

37. extrema of W provide large class of solutions with vanishing four – dimensional constant provide large class of solutions with vanishing four – dimensional constant dilatation transformation dilatation transformation extremum of W must occur for W=0 ! extremum of W must occur for W=0 ! effective cosmological constant is given by W effective cosmological constant is given by W

38. extremum of W must occur for W = 0 for any given solution : rescaled metric and dilaton is again a solution for rescaled solution : use extremum condition :

39. extremum of W is extremum of effective action

40. effective four – dimensional cosmological constant vanishes for extrema of W expand effective 4 – d - action in derivatives : 4 - d - field equation

41. Quasi-static solutions for arbitrary parameters of dilatation symmetric effective action : for arbitrary parameters of dilatation symmetric effective action : large classes of solutions with extremum of W and W ext = 0 are explicitly known ( flat phase ) large classes of solutions with extremum of W and W ext = 0 are explicitly known ( flat phase ) example : Minkowski space x D-dimensional torus example : Minkowski space x D-dimensional torus only for certain parameter regions : further solutions without extremum of W exist : only for certain parameter regions : further solutions without extremum of W exist : ( non-flat phase ) ( non-flat phase )

42. sufficient condition for vanishing cosmological constant extremum of W exists extremum of W exists

43. self tuning in higher dimensions involves infinitely many degrees of freedom ! involves infinitely many degrees of freedom ! for arbitrary parameters in effective action : flat phase solutions are present for arbitrary parameters in effective action : flat phase solutions are present extrema of W exist extrema of W exist for flat 4-d-space : W is functional for flat 4-d-space : W is functional of internal geometry, independent of x of internal geometry, independent of x solve field equations for internal metric and σ and ξ solve field equations for internal metric and σ and ξ

44. Dark energy if cosmic runaway solution has not yet reached fixed point : dilatation symmetry of field equations dilatation symmetry of field equations not yet exact not yet exact “ dilatation anomaly “ “ dilatation anomaly “ non-vanishing effective potential V in reduced four –dimensional theory non-vanishing effective potential V in reduced four –dimensional theory

45. conclusions (2) cosmic runaway towards fixed point may solve the cosmological constant problem solve the cosmological constant problem and and account for dynamical Dark Energy account for dynamical Dark Energy

46. effective dilatation symmetry in full quantum theory realized for fixed points realized for fixed points

47. Cosmic runaway large class of cosmological solutions which never reach a static state : runaway solutions large class of cosmological solutions which never reach a static state : runaway solutions some characteristic scale χ changes with time some characteristic scale χ changes with time effective dimensionless couplings flow with χ effective dimensionless couplings flow with χ ( similar to renormalization group ) ( similar to renormalization group ) couplings either diverge or reach fixed point couplings either diverge or reach fixed point for fixed point : exact dilatation symmetry of full quantum field equations and corresponding quantum effective action for fixed point : exact dilatation symmetry of full quantum field equations and corresponding quantum effective action

48. approach to fixed point dilatation symmetry not yet realized dilatation symmetry not yet realized dilatation anomaly dilatation anomaly effective potential V(φ) effective potential V(φ) exponential potential reflects anomalous dimension for vicinity of fixed point exponential potential reflects anomalous dimension for vicinity of fixed point V(φ) =M 4 exp( - αφ/M )

49. cosmic runaway and the problem of time varying constants It is not difficult to obtain quintessence potentials from higher dimensional ( or string ? ) theories It is not difficult to obtain quintessence potentials from higher dimensional ( or string ? ) theories Exponential form rather generic Exponential form rather generic ( after Weyl scaling) ( after Weyl scaling) Potential goes to zero for φ → ∞ Potential goes to zero for φ → ∞ But most models show too strong time dependence of constants ! But most models show too strong time dependence of constants !

50. higher dimensional dilatation symmetry generic class of solutions with vanishing effective four-dimensional cosmological constant and and constant effective dimensionless couplings

51. effective four – dimensional theory

52. characteristic length scales l : scale of internal space ξ : dilaton scale

53. effective Planck mass dimensionless, depends on internal geometry, from expansion of F in R

54. effective potential

55. canonical scalar fields consider field configurations with rescaled internal length scale and dilaton value potential and effective Planck mass depend on scalar fields

56. phase diagram stable solutions

57. phase structure of solutions solutions in flat phase exist for arbitrary values of effective parameters of higher dimensional effective action solutions in flat phase exist for arbitrary values of effective parameters of higher dimensional effective action question : how “big” is flat phase question : how “big” is flat phase ( which internal geometries and warpings are possible beyond torus solutions ) ( which internal geometries and warpings are possible beyond torus solutions ) solutions in non-flat phase only exist for restricted parameter ranges solutions in non-flat phase only exist for restricted parameter ranges

58. self tuning for all solutions in flat phase : self tuning of cosmological constant to zero ! self tuning of cosmological constant to zero !

59. self tuning for simplicity : no contribution of F to V assume Q depends on parameter α, which characterizes internal geometry: tuning required : and

60. self tuning in higher dimensions Q depends on higher dimensional extremum condition amounts to field equations typical solutions depend on integration constants γ solutions obeying boundary condition exist : fields

61. self tuning in higher dimensions involves infinitely many degrees of freedom ! involves infinitely many degrees of freedom ! for arbitrary parameters in effective action : flat phase solutions are present for arbitrary parameters in effective action : flat phase solutions are present extrema of W exist extrema of W exist for flat 4-d-space : W is functional for flat 4-d-space : W is functional of internal geometry, independent of x of internal geometry, independent of x solve field equations for internal metric and σ and ξ solve field equations for internal metric and σ and ξ

62. Dark energy if cosmic runaway solution has not yet reached fixed point : dilatation symmetry of field equations dilatation symmetry of field equations not yet exact not yet exact “ dilatation anomaly “ “ dilatation anomaly “ non-vanishing effective potential V in reduced four –dimensional theory non-vanishing effective potential V in reduced four –dimensional theory

63. End