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Quintessence. Dunkle Energie – Ein kosmisches Raetsel. Dark energy – a cosmic mystery. C.Wetterich. A.Hebecker,M.Doran,M.Lilley,J.Schwindt, C.M ü ller,G.Sch ä fer,E.Thommes, R.Caldwell. What is our Universe made of ?. Quintessence !. fire , air, water, soil !. critical density.
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Quintessence Dunkle Energie – Ein kosmisches Raetsel
Dark energy –a cosmic mystery C.Wetterich A.Hebecker,M.Doran,M.Lilley,J.Schwindt, C.Müller,G.Schäfer,E.Thommes, R.Caldwell
Quintessence ! fire , air, water, soil !
critical density • ρc =3 H² M² critical energy density of the universe ( M : reduced Planck-mass , H : Hubble parameter ) • Ωb=ρb/ρc fraction in baryons energy density in baryons over critical energy density
Composition of the universe Ωb = 0.045 Ωdm= 0.225 Ωh = 0.73
Ωm≈0.3 gravitational lens , HST
spatially flat universe Ωtot = 1 • theory (inflationary universe ) Ωtot =1.0000……….x • observation ( Boomerang,WMAP ) Ωtot =1.02 (0.02)
mean values Ωtot =1.02 Ωm =0.27 Ωb =0.045 Ωdm =0.225
Dark Energy Ωm + X = 1 Ωm : 30% Ωh : 70% Dark Energy h : homogenous , often ΩΛ instead of Ωh
Dark Energy : homogeneously distributed
What is Dark Energy ? Cosmological Constant or Quintessence ?
Cosmological Constant- Einstein - • Constant λ compatible with all symmetries • No time variation in contribution to energy density • Why so small ? λ/M4 = 10-120 • Why important just today ?
Cosm. Const. | Quintessence static | dynamical
Energy density ρ ~ ( 2.4×10 -3 eV )- 4 Reduced Planck mass M=2.44×1018GeV Newton’s constant GN=(8πM²) Cosmological mass scales Only ratios of mass scales are observable ! homogeneous dark energy: ρh/M4 = 6.5 10ˉ¹²¹ matter: ρm/M4= 3.5 10ˉ¹²¹
Time evolution tˉ² matter dominated universe tˉ3/2 radiation dominated universe • ρm/M4 ~ aˉ³ ~ • ρr/M4 ~ aˉ4~ t -2radiation dominated universe Huge age small ratio Same explanation for small dark energy?
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
Prediction : homogeneous dark energyinfluences recent cosmology- of same order as dark matter - Original models do not fit the present observations …. modifications
Cosmon • 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 • Time - variable dark energy : ρh(t) decreases with time !
Cosmon • Tiny mass • mc ~ H • New long - range interaction
“Fundamental” Interactions Strong, electromagnetic, weak interactions On astronomical length scales: graviton + cosmon gravitation cosmodynamics
Evolution of cosmon field Field equations Potential V(φ) determines details of the model e.g. V(φ) =M4 exp( - φ/M ) for increasing φ the potential decreases towards zero !
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
Equation of state p=T-V pressure kinetic energy ρ=T+V energy density Equation of state Depends on specific evolution of the scalar field
Negative pressure • w < 0 Ωh increases (with decreasing z ) • w < -1/3 expansion of the Universe is accelerating • w = -1 cosmological constant late universe with small radiation component :
small early and large presentdark energy fraction in dark energy has substantially increased since end of structure formation expansion of universe accelerates in present epoch
How can quintessence be distinguished from a cosmological constant ?
Time dependence of dark energy cosmological constant : Ωh ~ t² ~ (1+z)-3 M.Doran,…
Early dark energy A few percent in the early Universe Not possible for a cosmological constant
Quintessence and time variation of fundamental constants Generic prediction Strength unknown Strong, electromagnetic, weak interactions C.Wetterich , Nucl.Phys.B302,645(1988) gravitation cosmodynamics
Are fundamental “constants”time dependent ? Fine structure constant α (electric charge) Ratio nucleon mass to Planck mass
Quintessence and time dependence of “fundamental constants” • Fine structure constant depends on value of cosmon field : α(φ) (similar in standard model: couplings depend on value of Higgs scalar field) • Time evolution of φ Time evolution of α Jordan,…
Field dependent gauge coupling( gauge invariance maintained ) for GUT : C.Hill ; Q.Shafi , CW
GUT : running of electromagneticand strong gauge coupling related strong effect from variation of nucleon mass for time dependent couplings ! X.Calmet , H.Fritzsch
Where to look for time variation of fundamental couplings ? • Nucleosynthesis • Molecular absorption lines in the light of distant Quasars • Oklo natural reactor • Atomic clocks • CMB
Abundancies of primordial light elements from nucleosynthesis A.Coc
if present 2-sigma deviation of He –abundance from CMB/nucleosynthesis prediction would be confirmed : Δα/α ( z=1010 ) = -1.0 10-3 GUT 1 Δα/α ( z=1010 ) = -2.7 10-4 GUT 2 C.Mueller,G.Schaefer,…
Variation of fine structure constant as function of redshift Webb et al Srianand et al
Variation of fine structure constant Three independent data sets from Keck/HIRES Δα/α = - 0.54 (12) 10-5 Murphy,Webb,Flammbaum, june 2003 VLT Δα/α = - 0.06 (6) 10-5 Srianand,Chand,Petitjean,Aracil, feb.2004 z ≈ 2
Crossover quintessence andtime variation of fundamental “constants” Upper bounds for relative variation of the fine structure constant • Oklo natural reactor Δα/α < 10 -7 z=0.13 • Meteorites ( Re-decay ) Δα/α < 3 10 -7 z=0.45 • Crossover Quintessence compatible with QSO and upper bounds !
Time evolution of fundamental couplings traces time evolution of quintessence • todaywh close to -1 : • Small kinetic energy • Slow change of φ • Slow change of α • Very small Δα/αfor low z !
Variation of fine structure constant as function of redshift Webb et al
Atomic clocks and OKLO assumes that both effects are dominated by change of fine structure constant
Time variation of coupling constants must be tiny – would be of very high significance ! Possible signal for Quintessence
Πανταρει everything flows
Cosmodynamics Cosmon mediates new long-range interaction Range : size of the Universe – horizon Strength : weaker than gravity photon electrodynamics graviton gravity cosmon cosmodynamics Small correction to Newton’s law
Violation of equivalence principle Different couplings of cosmon to proton and neutron Differential acceleration Violation of equivalence principle p,n earth cosmon p,n