quintessence - a fifth force from variation of the ...wetterich/debarcelona0706.pdf · potential...
TRANSCRIPT
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Quintessence Quintessence --a fifth force from variation of a fifth force from variation of
the fundamental scalethe fundamental scale
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ΩΩmm + X = 1+ X = 1
ΩΩmm : 25%: 25%
ΩΩhh : 75%: 75%Dark EnergyDark Energy
?
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QuintessenceQuintessence
C.WetterichC.Wetterich
A.Hebecker,M.Doran,M.Lilley,J.SchwindtA.Hebecker,M.Doran,M.Lilley,J.Schwindt,,C.MC.Müüller,G.Schller,G.Schääfer,E.Thommesfer,E.Thommes,,R.Caldwell,M.Bartelmann,K.KarwanR.Caldwell,M.Bartelmann,K.Karwan
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Dark Energy Dark Energy dominates the Universedominates the Universe
Energy Energy -- density in the Universedensity in the Universe==
Matter + Dark EnergyMatter + Dark Energy
25 % + 75 %25 % + 75 %
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Abell 2255 Cluster~300 Mpc
Matter : Everything that clumpsMatter : Everything that clumps
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gravitational lens , HST
ΩΩmm= 0.25= 0.25
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ΩΩtottot=1=1
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Dark EnergyDark Energy
ΩΩmm + X = 1+ X = 1
ΩΩmm : 25%: 25%
ΩΩhh : 75% : 75% Dark EnergyDark Energy
h : homogenous , often ΩΛ instead of Ωh
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Space between clumpsSpace between clumpsis not empty :is not empty :
Dark Energy !Dark Energy !
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Dark Energy density isDark Energy density isthe same at every point of space the same at every point of space
““ homogeneous homogeneous ““
ΩΩhh
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Predictions for dark energy cosmologiesPredictions for dark energy cosmologies
The expansion of the Universeaccelerates today !
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What is Dark Energy ?
Cosmological Constant or
Quintessence ?
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Cosmological ConstantCosmological Constant-- Einstein Einstein --
Constant Constant λλ compatible with all symmetriescompatible with all symmetriesNo 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--120120
Why important just today ?Why important just today ?
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Cosm. Const. | Quintessencestatic | dynamical
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Quintessence and solution of Quintessence and solution of cosmological constant cosmological constant
problem should be related !problem should be related !
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Cosmological mass scalesCosmological mass scales
Energy densityEnergy density
ρρ ~ ( 2.4~ ( 2.4××10 10 --33 eVeV ))-- 4
Reduced Planck massReduced Planck massM=2.44M=2.44××10101818GeVGeVNewtonNewton’’s constants constantGGNN=(8=(8ππMM²²)
4
)
Only ratios of mass scales are observable !Only ratios of mass scales are observable !
homogeneous dark energy: homogeneous dark energy: ρρhh/M/M44 = 6.5 = 6.5 1010¯¹²¹¹²¹
matter: matter: ρρmm/M/M4= 3.5 10= 3.5 10¯¹²¹¹²¹
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Time evolutionTime evolution
ρρmm/M/M4 4 ~ a~ a¯³³ ~~
ρρrr/M/M4 4 ~ a~ a¯44 ~ ~ t t --22 radiation dominated universeradiation dominated universe
Huge age small ratioHuge age small ratioSame explanation for small dark energy Same explanation for small dark energy ??
t¯² matter dominated universe
t¯3/2 radiation dominated universe
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Time dependent Dark Energy :Time dependent Dark Energy :QuintessenceQuintessence
What changes in time ?What changes in time ?
Only dimensionless ratios of mass scales Only dimensionless ratios of mass scales are observable !are observable !
V : potential energy of scalar field or cosmological constantV : potential energy of scalar field or cosmological constantV/MV/M4 4 is observableis observable
Imagine the Planck mass M increases Imagine the Planck mass M increases ……
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Quintessence Quintessence from time evolution of from time evolution of
fundamental mass scalefundamental mass scale
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Fundamental mass scaleFundamental mass scale
Unification fixes parameters with dimensionsUnification fixes parameters with dimensions
Special relativity : cSpecial relativity : cQuantum theory : hQuantum theory : hUnification with gravity : Unification with gravity :
fundamental mass scalefundamental mass scale( Planck mass , string tension , ( Planck mass , string tension , ……))
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Fundamental mass scaleFundamental mass scale
Fixed parameter or dynamical scale ?Fixed parameter or dynamical scale ?Dynamical scale FieldDynamical scale FieldDynamical scale compared to what ?Dynamical scale compared to what ?momentum versus mass momentum versus mass ( or other parameter with dimension )( or other parameter with dimension )
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CosmonCosmon and and fundamental mass scalefundamental mass scale
Assume all mass parameters are proportional to Assume all mass parameters are proportional to scalar field scalar field χχ ((GUTsGUTs, superstrings,, superstrings,……))MMpp~ ~ χχ , , mmprotonproton~ ~ χχ , , ΛΛQCDQCD~ ~ χχ , M, MWW~ ~ χχ ,,……
χχ may evolve with time : may evolve with time : cosmoncosmonmmnn/M : ( almost ) constant /M : ( almost ) constant -- observationobservation !!
Only ratios of mass scales are observableOnly ratios of mass scales are observable
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Example :Example :
Field Field χχ denotes scale of transitiondenotes scale of transitionfrom higher dimensional physicsfrom higher dimensional physicsto effective four dimensional descriptionto effective four dimensional descriptionin theory without fundamental mass parameterin theory without fundamental mass parameter
(except for running of dimensionless couplings(except for running of dimensionless couplings……))
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Dilatation symmetryDilatation symmetry
Lagrange density:Lagrange density:
Dilatation symmetry forDilatation symmetry for
Conformal symmetry for Conformal symmetry for δδ=0=0
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Dilatation anomalyDilatation anomaly
Quantum fluctuations responsible forQuantum fluctuations responsible fordilatation anomalydilatation anomalyRunning couplings: Running couplings: hypothesishypothesis
Renormalization scale Renormalization scale µµ : ( momentum scale ): ( momentum scale )λλ~(~(χχ//µµ) ) ––AA
E > 0 : crossover QuintessenceE > 0 : crossover Quintessence
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Dilatation anomaly and Dilatation anomaly and quantum fluctuationsquantum fluctuations
Computation of running couplings ( beta Computation of running couplings ( beta functions ) needs unified theory !functions ) needs unified theory !Dominant contribution from modes with Dominant contribution from modes with momentamomenta ~~χχ !!No prejudice on No prejudice on ““natural value natural value ““ of anomalous of anomalous dimension should be inferred from tiny dimension should be inferred from tiny contributions at QCDcontributions at QCD-- momentum scale !momentum scale !
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CosmologyCosmology
Cosmology : Cosmology : χχ increases with time !increases with time !( due to coupling of ( due to coupling of χχ to curvature scalar )to curvature scalar )
for large for large χχ the ratio V/Mthe ratio V/M4 4 decreases to zerodecreases to zero
Effective cosmological constant vanishes Effective cosmological constant vanishes asymptotically for large t !asymptotically for large t !
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Asymptotically vanishing effective Asymptotically vanishing effective ““cosmological constantcosmological constant””
Effective cosmological constant ~ V/MEffective cosmological constant ~ V/M4 4
λλ ~ (~ (χχ//µµ) ) ––AA
V ~ (V ~ (χχ//µµ) ) ––A A χχ44
M = M = χχ
V/MV/M4 4 ~(~(χχ//µµ) ) ––A A
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WeylWeyl scalingscaling
WeylWeyl scaling : gscaling : gµνµν→→ (M/(M/χχ))2 2 ggµνµν ,,
φφ/M = /M = lnln ((χχ 44/V(/V(χχ))))
Exponential potential : V = MExponential potential : V = M44 exp(exp(--φφ/M)/M)
No additional constant !No additional constant !
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Without dilatation – anomaly :V= const. Massless Goldstone boson = dilaton
Dilatation – anomaly :V (φ )Scalar with tiny time dependent mass : cosmon
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Crossover QuintessenceCrossover Quintessence
( like QCD gauge coupling)( like QCD gauge coupling)
critical critical χχ where where δδ grows largegrows largecritical critical φφ where k grows large kwhere k grows large k²²((φφ )=)=δδ((χχ)/4 )/4
kk²²((φφ )= )= ““1/(2E(1/(2E(φφcc –– φφ)/M))/M)””
ifif ϕ ϕ cc ≈≈ 276/M (276/M ( tuningtuning ! ) :! ) :
this will be responsible for relative increase of dark this will be responsible for relative increase of dark energy in energy in presentpresent cosmological epochcosmological epoch
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Realistic cosmologyRealistic cosmology
Hypothesis on running couplings Hypothesis on running couplings yields realistic cosmology yields realistic cosmology for suitable values of A , E , for suitable values of A , E , φφcc
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Quintessence cosmologyQuintessence cosmology
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QuintessenceQuintessenceDynamical dark energy ,Dynamical dark energy ,generated by scalar generated by scalar fieldfield
((cosmoncosmon))C.Wetterich,Nucl.Phys.B302(1988)668, 24.9.87C.Wetterich,Nucl.Phys.B302(1988)668, 24.9.87P.J.E.Peebles,B.Ratra,ApJ.Lett.325(1988)L17, 20.10.87P.J.E.Peebles,B.Ratra,ApJ.Lett.325(1988)L17, 20.10.87
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Prediction :Prediction :
homogeneous dark energyhomogeneous dark energyinfluences recent cosmologyinfluences recent cosmology
-- of same order as dark matter of same order as dark matter --
Original models do not fit the present observationsOriginal models do not fit the present observations……. Modifications ( . Modifications ( i.e. E > 0 )i.e. E > 0 )
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QuintessenceQuintessence
CosmonCosmon –– Field Field φφ((x,y,z,tx,y,z,t))
Homogeneous und isotropic Universe : Homogeneous und isotropic Universe : φφ((x,y,z,tx,y,z,t)=)=φφ(t)(t)
Potential und kinetic energy of the Potential und kinetic energy of the cosmoncosmon --fieldfieldcontribute to a dynamical energy density of the Universe ! contribute to a dynamical energy density of the Universe !
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““FundamentalFundamental”” InteractionsInteractions
Strong, electromagnetic, weakinteractions
gravitation cosmodynamics
On astronomical length scales:
graviton
+
cosmon
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Dynamics of quintessenceDynamics of quintessence
CosmonCosmon ϕϕ : scalar singlet field: scalar singlet field
Lagrange density L = V + Lagrange density L = V + ½½ k(k(φφ)) ∂∂ϕ ϕ ∂∂ϕϕ(units: reduced Planck mass M=1)(units: reduced Planck mass M=1)
Potential : V=exp[Potential : V=exp[--ϕ]ϕ]
““Natural initial valueNatural initial value”” in Planck era in Planck era ϕ=0ϕ=0
today: today: ϕϕ=276=276
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QuintessenceQuintessence modelsmodels
Kinetic function Kinetic function k(k(φφ)) : parameterizes the : parameterizes the details of the model details of the model -- ““kinetialkinetial””
k(k(φφ) = k=const. Exponential Q.) = k=const. Exponential Q.k(k(φφ ) = exp (() = exp ((φφ –– φφ11)/)/αα) Inverse power law Q.) Inverse power law Q.kk²²((φφ )= )= ““1/(2E(1/(2E(φφcc –– φφ))))”” Crossover Q.Crossover Q.
possible naturalness criterion:possible naturalness criterion:
k(k(φφ=0)/ k(=0)/ k(φφtodaytoday) : not tiny or huge !) : not tiny or huge !
-- else: explanation needed else: explanation needed --
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CosmonCosmon
Scalar field changes its value even in the Scalar field changes its value even in the presentpresent cosmological epochcosmological epochPotential und kinetic energy of Potential und kinetic energy of cosmoncosmoncontribute to the energy density of the Universecontribute to the energy density of the UniverseTime Time -- variable dark energy : variable dark energy : ρρhh(t(t) decreases with time ! ) decreases with time !
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CosmonCosmon
Tiny massTiny mass
mmcc ~ H~ H
New long New long -- range interactionrange interaction
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cosmoncosmon mass changes with time !mass changes with time !
for standard kinetic termfor standard kinetic termmmcc
22 = V= V””
for standard exponential potential , k for standard exponential potential , k ≈≈ const.const.mmcc
22 = V= V””/ k/ k22 = V/( k= V/( k2 2 MM22 ) ) = 3 = 3 ΩΩh h (1 (1 -- wwhh ) H) H2 2 /( 2 k/( 2 k2 2 ) )
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Cosmological equationsCosmological equations
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Cosmic Attractors Cosmic Attractors
Solutions independent of initial conditions
typically V~t -2
φ ~ ln ( t )
Ωh ~ const.
details depend on V(φ)or kinetic term
early cosmology
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Quintessence becomes important Quintessence becomes important ““todaytoday””
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Equation of stateEquation of state
p=Tp=T--V pressure V pressure kinetic energykinetic energy
ρρ=T+V energy density=T+V energy density
Equation of stateEquation of state
Depends on specific evolution of the scalar fieldDepends on specific evolution of the scalar field
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Negative pressureNegative pressure
w < 0 w < 0 ΩΩh h increases increases (with decreasing z )(with decreasing z )
w < w < --1/3 expansion of the Universe is1/3 expansion of the Universe isacceleratingaccelerating
w = w = --1 cosmological constant1 cosmological constant
late universe withlate universe withsmall radiation component :small radiation component :
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Quintessence becomes important Quintessence becomes important ““todaytoday””
No reason why w shouldNo reason why w shouldbe constant in time !be constant in time !
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How can quintessence be How can quintessence be distinguished from a distinguished from a
cosmological constant ?cosmological constant ?
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Time dependence of dark energyTime dependence of dark energy
cosmological constant : Ωh ~ t² ~ (1+z)-3
M.Doran,…
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small early and large presentsmall early and large presentdark energydark energy
fraction in dark energy has substantially fraction in dark energy has substantially increased since end of structure formationincreased since end of structure formation
expansion of universe accelerates in present expansion of universe accelerates in present epochepoch
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Early dark energyEarly dark energy
A few percent in the early UniverseA few percent in the early Universe
Not possible for a cosmological constantNot possible for a cosmological constant
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A few percent Early Dark EnergyA few percent Early Dark Energy
If linear power spectrum fixed today ( If linear power spectrum fixed today ( σσ8 8 ) :) :
More Structure at high z !More Structure at high z !
Bartelmann,DoranBartelmann,Doran,,……
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Early Dark EnergyEarly Dark Energy
A few percent in the A few percent in the early Universeearly Universe
Not possible for a Not possible for a cosmological cosmological constant
1σ and 2σ limits
Doran,Karwan,..constant
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Measure Measure ΩΩhh(z(z) !) !
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How to distinguish Q from How to distinguish Q from ΛΛ ??
A) Measurement A) Measurement ΩΩhh(z(z) ) H(zH(z))
i) i) ΩΩhh(z(z) at the time of) at the time ofstructure formation , CMB structure formation , CMB -- emissionemissionor or nucleosynthesisnucleosynthesis
ii) equation of state ii) equation of state wwhh((todaytoday) > ) > --11
B) Time variation of fundamental B) Time variation of fundamental ““constantsconstants””C) Apparent violation of equivalence principleC) Apparent violation of equivalence principle
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Quintessence and time variation of Quintessence and time variation of fundamental constantsfundamental constants
Strong, electromagnetic, weakinteractions
gravitation cosmodynamics
Generic prediction
Strengthunknown
C.WetterichC.Wetterich , , Nucl.Phys.B302,645(1988Nucl.Phys.B302,645(1988))
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Time varying constantsTime varying constants
It is not difficult to obtain quintessence It is not difficult to obtain quintessence potentials from higher dimensional or string potentials from higher dimensional or string theoriestheoriesExponential form rather generic Exponential form rather generic ( after ( after WeylWeyl scaling)scaling)But most models show too strong time But most models show too strong time dependence of constants !dependence of constants !
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Quintessence from Quintessence from higher dimensionshigher dimensions
work with J. work with J. SchwindtSchwindt
hephep--th/0501049th/0501049
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Quintessence Quintessence from higher dimensionsfrom higher dimensions
An instructive example:An instructive example:
Einstein Einstein –– Maxwell theory in six dimensionsMaxwell theory in six dimensions
Warning : not scale Warning : not scale -- free !free !Dilatation anomaly replaced by explicit mass scales.Dilatation anomaly replaced by explicit mass scales.
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MetricMetric
AnsatzAnsatz with particular metric ( not most general ! )with particular metric ( not most general ! )which is consistent withwhich is consistent with
d=4 homogeneous and isotropic Universed=4 homogeneous and isotropic Universeand internal and internal U(1) x ZU(1) x Z22 isometryisometry
B B ≠≠ 1 : football shaped internal geometry1 : football shaped internal geometry
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Exact solutionExact solution
m : monopole number ( integer)m : monopole number ( integer)
cosmology with scalarcosmology with scalar
and potential V :and potential V :
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Asymptotic solution for large tAsymptotic solution for large t
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NaturalnessNaturalness
No tuning of parameters or integration No tuning of parameters or integration constantsconstantsRadiation and matter can be implementedRadiation and matter can be implementedAsymptotic solution depends on details of Asymptotic solution depends on details of model, e.g. solutions with constant model, e.g. solutions with constant ΩΩhh ≠≠ 11
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problem :problem :
time variation of fundamental constantstime variation of fundamental constants
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Are fundamental Are fundamental ““constantsconstants””time dependent ?time dependent ?
Fine structure constant Fine structure constant αα (electric charge)(electric charge)
Ratio electron to proton massRatio electron to proton mass
Ratio nucleon mass to Planck massRatio nucleon mass to Planck mass
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Quintessence and Quintessence and Time dependence of Time dependence of
““fundamental constantsfundamental constants””
Fine structure constant depends on value ofFine structure constant depends on value ofcosmoncosmon field : field : αα((φφ))
(similar in standard model: couplings depend on (similar in standard model: couplings depend on value of Higgs scalar field)value of Higgs scalar field)
Time evolution of Time evolution of φφTime evolution of Time evolution of αα
Jordan,Jordan,……
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Standard Standard –– Model of Model of electroweak interactions :electroweak interactions :
Higgs Higgs -- mechanismmechanism
The masses of all fermions and gauge bosons are The masses of all fermions and gauge bosons are proportional to the ( vacuum expectation ) value of a proportional to the ( vacuum expectation ) value of a scalar field scalar field φφHH ( Higgs scalar )( Higgs scalar )For electron, quarks , WFor electron, quarks , W-- and Zand Z-- bosons :bosons :
mmelectronelectron = = hhelectronelectron * * φφHH etc.etc.
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Restoration of symmetryRestoration of symmetryat high temperature at high temperature in the early Universein the early Universe
Low TLow TSSBSSB<<φφHH>=>=φφ00 ≠≠ 00
High THigh TSYM SYM <<φφHH>=0>=0
high T :high T :less orderless ordermore symmetrymore symmetry
example:example:magnetsmagnets
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In the hot plasma In the hot plasma of the early Universe :of the early Universe :
No difference in mass for No difference in mass for electron and electron and muonmuon !!
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Quintessence :Quintessence :Couplings are still varying Couplings are still varying nownow !!
Strong bounds on Strong bounds on the variation of couplings the variation of couplings --interesting perspectives for interesting perspectives for
observation !observation !
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Where to look for time variation of Where to look for time variation of fundamental couplings ?fundamental couplings ?
NucleosynthesisNucleosynthesisMolecular absorption lines in the light of Molecular absorption lines in the light of distant Quasarsdistant QuasarsOkloOklo natural reactornatural reactorAtomic clocksAtomic clocksCMBCMB
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baryons :
the matter of stars and humans
ΩΩbb = 0.045= 0.045
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AbundanciesAbundancies of of primordialprimordiallight elementslight elementsfrom from nucleosynthesisnucleosynthesis
A.CocA.Coc
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Allowed values for variation of Allowed values for variation of fine structure constant :fine structure constant :
∆α∆α//αα ( z=10( z=1010 10 ) = ) = --1.0 101.0 10--3 3 GUT 1GUT 1∆α∆α//αα ( z=10( z=1010 10 ) = ) = --2.7 102.7 10--4 4 GUT 2GUT 2
C.Mueller,G.SchaeferC.Mueller,G.Schaefer,,……
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Time variation of coupling constants must be tiny –
would be of very high significance !
Possible signal for Quintessence
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Violation of equivalence principleViolation of equivalence principle
Different couplings of Different couplings of cosmoncosmon to proton and to proton and neutronneutron
Differential accelerationDifferential acceleration
““Violation of Violation of equivalence principleequivalence principle”
p,n
earthcosmon
” p,n
only apparent : new only apparent : new ““fifth forcefifth force”” !!
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Apparent violation of equivalence principle Apparent violation of equivalence principle
andand
time variation of fundamental couplingstime variation of fundamental couplings
measure both themeasure both the
cosmoncosmon –– coupling to ordinary mattercoupling to ordinary matter
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Differential acceleration Differential acceleration ηη
For unified theories ( GUT ) :For unified theories ( GUT ) :
Q : time dependence of other parameters
ηη==∆∆a/2aa/2a
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Link between time variation of α
and violation of equivalence principle
typically : η = 10-14
if time variation of α near Oklo upper bound
to be tested by MICROSCOPE
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SummarySummary
oo ΩΩhh = 0.75= 0.75
oo Q/Q/ΛΛ : dynamical und static dark energy : dynamical und static dark energy will be distinguishablewill be distinguishable
oo Q : time varying fundamental coupling Q : time varying fundamental coupling ““constantsconstants””
violation of equivalence principleviolation of equivalence principle
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????????????????????????????????????????????????Why becomes Quintessence dominant in the Why becomes Quintessence dominant in the
present cosmological epoch ?present cosmological epoch ?Are dark energy and dark matter related ?Are dark energy and dark matter related ?Can Quintessence be explained in a fundamental Can Quintessence be explained in a fundamental
unified theory ?unified theory ?
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EndEnd
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A few referencesA few references
C.WetterichC.Wetterich , Nucl.Phys.B302,668(1988) , received 24.9.1987, Nucl.Phys.B302,668(1988) , received 24.9.1987
P.J.E.Peebles,B.RatraP.J.E.Peebles,B.Ratra , Astrophys.J.Lett.325,L17(1988) , received 20.10.1987, Astrophys.J.Lett.325,L17(1988) , received 20.10.1987
B.Ratra,P.J.E.PeeblesB.Ratra,P.J.E.Peebles , Phys.Rev.D37,3406(1988) , received 16.2.1988, Phys.Rev.D37,3406(1988) , received 16.2.1988
J.Frieman,C.T.Hill,A.Stebbins,I.WagaJ.Frieman,C.T.Hill,A.Stebbins,I.Waga , Phys.Rev.Lett.75,2077(1995), Phys.Rev.Lett.75,2077(1995)
P.FerreiraP.Ferreira, , M.JoyceM.Joyce , Phys.Rev.Lett.79,4740(1997), Phys.Rev.Lett.79,4740(1997)
C.WetterichC.Wetterich , Astron.Astrophys.301,321(1995), Astron.Astrophys.301,321(1995)
P.VianaP.Viana, , A.LiddleA.Liddle , Phys.Rev.D57,674(1998), Phys.Rev.D57,674(1998)
E.Copeland,A.Liddle,D.WandsE.Copeland,A.Liddle,D.Wands , Phys.Rev.D57,4686(1998), Phys.Rev.D57,4686(1998)
R.Caldwell,R.Dave,P.SteinhardtR.Caldwell,R.Dave,P.Steinhardt , Phys.Rev.Lett.80,1582(1998), Phys.Rev.Lett.80,1582(1998)
P.Steinhardt,L.Wang,I.ZlatevP.Steinhardt,L.Wang,I.Zlatev , Phys.Rev.Lett.82,896(1999), Phys.Rev.Lett.82,896(1999)
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CosmodynamicsCosmodynamics
CosmonCosmon mediates new longmediates new long--range interactionrange interactionRange : size of the Universe Range : size of the Universe –– horizonhorizonStrength : weaker than gravityStrength : weaker than gravity
photon electrodynamicsphoton electrodynamicsgraviton gravitygraviton gravitycosmoncosmon cosmodynamicscosmodynamics
Small correction to NewtonSmall correction to Newton’’s laws law
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Time evolution of fundamental Time evolution of fundamental couplings traces time evolution of couplings traces time evolution of quintessencequintessence
today today wwhh close to close to --1 :1 :
•• Small kinetic energySmall kinetic energy•• Slow change of Slow change of φφ•• Slow change of Slow change of αα
Very small Very small ∆α∆α//αα for low z !for low z !
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Crossover quintessence andCrossover quintessence andtime variation of fundamental time variation of fundamental
““constantsconstants””
Upper bounds for relative variation of the Upper bounds for relative variation of the fine structure constantfine structure constantOkloOklo natural reactor natural reactor ∆∆αα//αα < 10 < 10 --7 7 z=0.13z=0.13Meteorites ( ReMeteorites ( Re--decay ) decay ) ∆∆αα//αα < 3 10 < 3 10 --7 7 z=0.45z=0.45
Crossover Quintessence compatible with QSOCrossover Quintessence compatible with QSOand upper bounds !and upper bounds !
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Atomic clocks and OKLOAtomic clocks and OKLO
assumes that both effects are dominated by change of fine structure constant
Observation : |Observation : |∆α∆α//αα | < 2 * 10 | < 2 * 10 --15 15 / yr/ yr
Munich groupMunich group
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Variation of fine structure constant Variation of fine structure constant as function of as function of redshiftredshift
Three independent data sets from Three independent data sets from Keck/HIRESKeck/HIRES
∆∆αα//αα = = -- 0.54 (12) 100.54 (12) 10--55
Murphy,Webb,FlammbaumMurphy,Webb,Flammbaum, , junejune20032003
VLTVLT
∆∆αα//αα = = -- 0.06 (6) 100.06 (6) 10--55
Srianand,Chand,Petitjean,AracilSrianand,Chand,Petitjean,Aracil, , feb.2004feb.2004
z ≈ 2
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CosmonCosmon and time variation of and time variation of couplings : fixed pointscouplings : fixed points
small coupling of small coupling of cosmoncosmon to matter due to fixed to matter due to fixed points behaviorpoints behavior
close to fixed point :small time evolution of couplingscoupling to matter weaker than gravitational strength
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Field equationsField equations
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Energy momentum tensorEnergy momentum tensor
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Free integration constantsFree integration constants
M , B , M , B , ΦΦ(t=0) , (d(t=0) , (dΦΦ//dt)(tdt)(t=0) : continuous=0) : continuous
m : discretem : discrete
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Conical singularitiesConical singularities
deficit angledeficit angle
singularities can be included with singularities can be included with energy momentum tensor on energy momentum tensor on branebrane
bulk point of view : describe everything in terms of bulk bulk point of view : describe everything in terms of bulk geometry ( no modes on geometry ( no modes on branebrane without tail in bulk )without tail in bulk )
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Dimensional reductionDimensional reduction
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Time dependent gauge couplingTime dependent gauge coupling
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Realistic model :Realistic model :Crossover QuintessenceCrossover Quintessence
( like QCD gauge coupling)( like QCD gauge coupling)
critical critical χχ where where δδ grows largegrows largecritical critical φφ where k grows large kwhere k grows large k²²((φφ )=)=δδ((χχ)/4 )/4
kk²²((φφ )= )= ““1/(2E(1/(2E(φφcc –– φφ)/M))/M)””
ifif ϕ ϕ cc ≈≈ 276/M (276/M ( tuningtuning ! )! )
Relative increase of dark energy in present Relative increase of dark energy in present cosmological epochcosmological epoch