Coupled Dark Energy and Dark Matter from dilatation symmetry
Cosmological ConstantCosmological Constant- Einstein -- Einstein -
Constant Constant λλ compatible with all symmetries compatible with all symmetries Constant Constant λλ compatible with all compatible with all
observationsobservations No time variation in contribution to energy No time variation in contribution to energy
densitydensity
Why so small ? Why so small ? λλ/M/M44 = 10 = 10-120-120
Why important just today ?Why important just today ?
Cosmological mass scalesCosmological mass scales Energy densityEnergy density
ρρ ~ ( 2.4×10 ~ ( 2.4×10 -3-3 eV eV ))- 4- 4
Reduced Planck Reduced Planck massmass
M=2.44M=2.44×10×101818GeVGeV Newton’s constantNewton’s constant
GGNN=(8=(8ππM²)M²)
Only ratios of mass scales are observable !Only ratios of mass scales are observable !
homogeneous dark energy: homogeneous dark energy: ρρhh/M/M44 = 7 · = 7 · 10ˉ¹²¹10ˉ¹²¹
matter: matter: ρρmm/M/M4= 3 · 10ˉ¹²¹= 3 · 10ˉ¹²¹
QuintessenceQuintessenceDynamical dark Dynamical dark
energy ,energy ,
generated by scalargenerated by scalar
field field (cosmon)(cosmon)
C.Wetterich,Nucl.Phys.B302(1988)668, C.Wetterich,Nucl.Phys.B302(1988)668, 24.9.87 24.9.87P.J.E.Peebles,B.Ratra,ApJ.Lett.325(1988)LP.J.E.Peebles,B.Ratra,ApJ.Lett.325(1988)L17, 20.10.8717, 20.10.87
CosmonCosmon Scalar field changes its value even Scalar field changes its value even
in the in the present present cosmological epochcosmological epoch Potential und kinetic energy of Potential und kinetic energy of
cosmon contribute to the energy cosmon contribute to the energy density of the Universedensity of the Universe
Time - variable dark energy : Time - variable dark energy : ρρhh(t) decreases with time !(t) decreases with time !
V(V(φφ) =M) =M44 exp( - exp( - αφαφ/M )/M )
Two key features Two key features for realistic cosmologyfor realistic cosmology
1 ) Exponential cosmon potential and 1 ) Exponential cosmon potential and
scaling solutionscaling solution
V(V(φφ) =M) =M44 exp( - exp( - αφαφ/M ) /M )
V(V(φφ →→ ∞ ) → 0 ! ∞ ) → 0 !
2 ) Stop of cosmon evolution by 2 ) Stop of cosmon evolution by
cosmological triggercosmological trigger
e.g. growing neutrino quintessencee.g. growing neutrino quintessence
Evolution of cosmon fieldEvolution of cosmon field
Field equationsField equations
Potential V(Potential V(φφ) determines details of the ) determines details of the modelmodel
V(V(φφ) =M) =M4 4 exp( - exp( - αφαφ/M )/M )
for increasing for increasing φφ the potential the potential decreases towards zero !decreases towards zero !
exponential potentialexponential potentialconstant fraction in dark constant fraction in dark
energyenergy
can explain order of can explain order of magnitude magnitude
of dark energy !of dark energy !
ΩΩh h = 3(4)/= 3(4)/αα22
Asymptotic solutionAsymptotic solution
explain V( explain V( φφ → ∞ ) = 0 ! → ∞ ) = 0 !
effective field equations should effective field equations should have generic solution of this typehave generic solution of this type
setting : quantum effective action , setting : quantum effective action , all quantum fluctuations included:all quantum fluctuations included:investigate generic forminvestigate generic form
realized by fixed point realized by fixed point of runaway solutionof runaway solution
in higher dimensions :in higher dimensions :
dilatation symmetrydilatation symmetry
Cosmon and Cosmon and bolonbolon
Two scalar fields : common Two scalar fields : common origin from origin from dilatation symmetric fixed dilatation symmetric fixed point of point of higher dimensional theoryhigher dimensional theory
Two characteristic Two characteristic behaviorsbehaviors
Bolon oscillates - Bolon oscillates -
if mass larger than H if mass larger than H
Bolon is frozen -Bolon is frozen -
if mass smaller that Hif mass smaller that H
Early scaling solutionEarly scaling solution
dominated by cosmondominated by cosmonbolon frozen and negligiblebolon frozen and negligiblebolon mass increases during bolon mass increases during scaling solutionscaling solution
Bolon oscillationsBolon oscillations
ratio bolon mass / H increasesratio bolon mass / H increases bolon starts oscillating once mass bolon starts oscillating once mass
larger than Hlarger than H subsequently bolon behaves as Dark subsequently bolon behaves as Dark
MatterMatter matter radiation equality around matter radiation equality around
beginning of oscillationsbeginning of oscillations
Transition to matter Transition to matter dominationdomination
precise timing depends at this stage on initial precise timing depends at this stage on initial value of bolonvalue of bolon
Effective coupling betweenEffective coupling betweenDark Energy and Dark Dark Energy and Dark
mattermatter
Realistic quintessence needs late Realistic quintessence needs late modificationmodification
modification of cosmon – bolon potential modification of cosmon – bolon potential or growing neutrinos or …or growing neutrinos or …
Modification of potential for Modification of potential for large large χχ : :
independence of initial independence of initial conditionsconditions
matter - radiation equality depends now on matter - radiation equality depends now on parameters of potentialparameters of potential
Present bolon mass Present bolon mass corresponds to range on corresponds to range on
subgalactic scalessubgalactic scales
suppression of small scale Dark Matter suppression of small scale Dark Matter structures ?structures ?
conclusions (1)conclusions (1)
Bolon : new Dark Matter candidateBolon : new Dark Matter candidate
not detectable by local observations –not detectable by local observations –
direct or indirect dark matter direct or indirect dark matter searchessearches
perhaps observation by influence on perhaps observation by influence on subgalactic dark matter structuressubgalactic dark matter structures
Higher –dimensional Higher –dimensional dilatation symmetrydilatation symmetry
solvessolvescosmological constant cosmological constant
problemproblem
graviton and dilatongraviton and dilaton
dilatation symmetric effective actiondilatation symmetric effective action
simple examplesimple example
in general : in general : many dimensionless many dimensionless parameters characterize effective parameters characterize effective actionaction
flat phaseflat phase
generic existence of solutions of generic existence of solutions of
higher dimensional field equations higher dimensional field equations withwith
effective effective four –dimensional gravityfour –dimensional gravity andand
vanishing cosmological constantvanishing cosmological constant
torus solutiontorus solutionexample : example : Minkowski space Minkowski space xx D-dimensional torus D-dimensional torus ξξ = const = const solves higher dimensional field equationssolves higher dimensional field equations extremum of effective actionextremum of effective action
finite four- dimensional gauge couplingsfinite four- dimensional gauge couplings dilatation symmetry spontaneously brokendilatation symmetry spontaneously broken
generically many more solutions in flat phase !generically many more solutions in flat phase !
massless scalars
dilaton
geometrical scalars ( moduli ) variation of circumference of tori change of volume of internal space bolon is associated to one such
scalar
Higher dimensional Higher dimensional dilatation symmetrydilatation symmetry
for arbitrary values of effective couplings within a certain for arbitrary values of effective couplings within a certain range :range :
higher dimensional dilatation symmetry implies existence higher dimensional dilatation symmetry implies existence of of
a large class of solutions with vanishing four –dimensionala 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 equations , which admit a finite four-dimensional
gravitationalgravitational constant and non-zero value for the dilaton , have V=0constant and non-zero value for the dilaton , have V=0
self-tuning mechanismself-tuning mechanism
look for extrema of effective actionlook for extrema of effective actionfor general field configurationsfor general field configurations
warpingwarping
most general metric with maximal most general metric with maximal four – dimensional symmetryfour – dimensional symmetry
general form of quasi – static solutionsgeneral form of quasi – static solutions( non-zero or zero cosmological constant )( non-zero or zero cosmological constant )
effective four – dimensional effective four – dimensional actionaction
flat phase : flat phase : extrema of Wextrema of Win higher dimensions , those exist generically !in higher dimensions , those exist generically !
extrema of Wextrema of W
provide large class of solutions with provide large class of solutions with vanishing four – dimensional constantvanishing four – dimensional constant
dilatation transformationdilatation transformation
extremum of W must occur for W=0 !extremum of W must occur for W=0 ! effective cosmological constant is effective cosmological constant is
given by Wgiven by W
extremum of W must occur extremum of W must occur for W = 0for W = 0
for any given solution : rescaled metric and for any given solution : rescaled metric and dilaton is again a solutiondilaton is again a solution
for rescaled solution :for rescaled solution :
useuse
extremum condition :extremum condition :
effective four – dimensional effective four – dimensional cosmological constant cosmological constant
vanishes for extrema of Wvanishes for extrema of W
expand effective 4 – d - actionexpand effective 4 – d - action
in derivatives :in derivatives :
4 - d - field 4 - d - field equationequation
Quasi-static solutionsQuasi-static solutions
for arbitrary parameters of dilatation for arbitrary parameters of dilatation symmetric effective action :symmetric effective action :
large classes of solutions with extremum of large classes of solutions with extremum of W and WW and Wext ext = 0 are explicitly known ( = 0 are explicitly known ( flat flat phasephase ) )
example : example : Minkowski space Minkowski space xx D-dimensional D-dimensional torustorus
only for certain parameter regions : further only for certain parameter regions : further solutions without extremum of W exist : solutions without extremum of W exist :
( ( non-flat phasenon-flat phase ) )
sufficient condition for sufficient condition for vanishing cosmological vanishing cosmological
constantconstant
extremum of W extremum of W existsexists
self tuning in higher self tuning in higher dimensionsdimensions
involves infinitely many degrees of freedom !involves infinitely many degrees of freedom !
for arbitrary parameters in effective action : for arbitrary parameters in effective action : flat phase solutions are flat phase solutions are presentpresent
extrema of W existextrema 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 solve field equations for internal metric and σσ and and ξξ
Dark energyDark energy
if cosmic runaway solution has not yet if cosmic runaway solution has not yet reached fixed point :reached fixed point :
dilatation symmetry of field equations dilatation symmetry of field equations
not yet exactnot yet exact
“ “ dilatation anomaly “dilatation anomaly “
non-vanishing effective potential V in non-vanishing effective potential V in reduced four –dimensional theoryreduced four –dimensional theory
conclusions (2)conclusions (2)
cosmic runaway towards fixed point cosmic runaway towards fixed point maymay
solve the cosmological constant solve the cosmological constant problemproblem
andand
account for dynamical Dark Energyaccount for dynamical Dark Energy
effective dilatation effective dilatation symmetry insymmetry in
full quantum theoryfull quantum theory
realized for fixed pointsrealized for fixed points
Cosmic runawayCosmic runaway large class of cosmological solutions which never large class of cosmological solutions which never
reach a static state : runaway solutionsreach a static state : runaway solutions
some characteristic scale some characteristic scale χχ changes with time changes with time
effective dimensionless couplings flow with effective dimensionless couplings flow with χχ ( similar to renormalization group )( similar to renormalization group )
couplings either diverge or reach fixed pointcouplings either diverge or reach fixed point
for fixed point : for fixed point : exact dilatation symmetry exact dilatation symmetry of full of full quantum field equations and corresponding quantum field equations and corresponding quantum effective actionquantum effective action
approach to fixed pointapproach to fixed point
dilatation symmetry not yet realizeddilatation symmetry not yet realized dilatation anomalydilatation anomaly effective potential effective potential V(φ)V(φ) exponential potential reflects exponential potential reflects
anomalous dimension for vicinity of anomalous dimension for vicinity of fixed pointfixed point
V(V(φφ) =M) =M4 4 exp( - exp( - αφαφ/M )/M )
cosmic runaway and the cosmic runaway and the problem of time varying problem of time varying
constantsconstants It is not difficult to obtain quintessence It is not difficult to obtain quintessence
potentials from higher dimensional ( or potentials from higher dimensional ( or string ? ) theoriesstring ? ) theories
Exponential form rather generic Exponential form rather generic
( after Weyl scaling)( after Weyl scaling) Potential goes to zero for Potential goes to zero for φφ →→ ∞∞ But most models show too strong time But most models show too strong time
dependence of constants !dependence of constants !
higher dimensional higher dimensional dilatation symmetrydilatation symmetry
generic class of solutions with generic class of solutions with
vanishing effective four-dimensional vanishing effective four-dimensional cosmological constantcosmological constant
andand
constant effective dimensionless couplingsconstant effective dimensionless couplings
characteristic length characteristic length scalesscales
ll : scale of internal space : scale of internal space
ξξ : dilaton scale: dilaton scale
effective Planck masseffective Planck mass
dimensionless , dimensionless , depends on internal geometry ,depends on internal geometry ,from expansion of F in Rfrom expansion of F in R
canonical scalar fieldscanonical scalar fields
consider field configurations with rescaledconsider field configurations with rescaledinternal length scale and dilaton valueinternal length scale and dilaton value
potential and effective Planck mass depend on scalar fieldspotential and effective Planck mass depend on scalar fields
phase structure of phase structure of solutionssolutions
solutions in flat phase exist for arbitrary solutions in flat phase exist for arbitrary values of effective parameters of higher values of effective parameters of higher dimensional effective actiondimensional effective action
question : how “big” is flat phase question : how “big” is flat phase ( which internal geometries and warpings ( which internal geometries and warpings
are possible beyond torus solutions )are possible beyond torus solutions )
solutions in non-flat phase only exist for solutions in non-flat phase only exist for restricted parameter rangesrestricted parameter ranges
self tuningself tuning
for all solutions in flat phase : for all solutions in flat phase :
self tuning of cosmological constant self tuning of cosmological constant to zero !to zero !
self tuningself tuning
for simplicity : no contribution of F to for simplicity : no contribution of F to VV
assume Q depends on parameter assume Q depends on parameter αα , , which characterizes internal which characterizes internal geometry:geometry:
tuning required : tuning required : andand
self tuning in higher self tuning in higher dimensionsdimensions
Q depends on higher dimensionalQ depends on higher dimensional
extremum condition extremum condition amounts to field equationsamounts to field equations
typical solutions depend on integration constants typical solutions depend on integration constants γγ
solutions obeying boundary condition exist :solutions obeying boundary condition exist :
fieldsfields
self tuning in higher self tuning in higher dimensionsdimensions
involves infinitely many degrees of freedom !involves infinitely many degrees of freedom !
for arbitrary parameters in effective action : for arbitrary parameters in effective action : flat phase solutions are flat phase solutions are presentpresent
extrema of W existextrema 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 solve field equations for internal metric and σσ and and ξξ
Dark energyDark energy
if cosmic runaway solution has not yet if cosmic runaway solution has not yet reached fixed point :reached fixed point :
dilatation symmetry of field equations dilatation symmetry of field equations
not yet exactnot yet exact
“ “ dilatation anomaly “dilatation anomaly “
non-vanishing effective potential V in non-vanishing effective potential V in reduced four –dimensional theoryreduced four –dimensional theory