Lecture 8 Observational Cosmology Parameters of Our Universe The Concordance Model AS 4022 Cosmology Time and Distance vs Redshift d R −dx x = 1+ z = 0 → dt = dt R x H(x) R Friedmann : H(x) = H 0 ΩM x 3 + ΩΛ + (1− Ω0 ) x 2 Ω0 ≡ΩM + ΩΛ look - back time : t0 t(z) = 1+z ∫ dt = te ∫ 1 χ ( ΩR = 0) dx 1 1+z = ∫ x H(x) H 0 1 x € dx ΩM x 3 + ΩΛ + (1− Ω0 ) x 2 radial distance : t0 D0(z) = R0 χ = ∫ te 1+z R0 x c dx c 1+z c dt = ∫ = ∫ R(t) x H(x) H 0 1 1 dx ΩM x 3 + ΩΛ + (1− Ω0 ) x 2 1/ 2 c k circumferencial distance : r0 = R0 Sk ( χ ) R0 = H 0 Ω0 −1 angular diameter distance : DA = r0 (1+ z ) luminosity distance : DL = (1+ z ) r0 AS 4022 Cosmology r D Angular Diameter Distance ΩΛ ΩM € ΩM + ΩΛ = 1 € ΩΛ = 0 € € AS 4022 Cosmology r(z) DA (z) = 1+ z DL (z) = (1+ z) r(z) € € r(z) = R0 Sk ( χ (z)) r(z) H0 / c € AS 4022 Cosmology “Concordance Model” Parameters km/s km/s H 0 ≡ 100 h ≈ 70 Mpc Mpc h ≈ 0.7 ΩR ≈ 4.2 ×10−5 h −2 ≈ 8.4 ×10−5 (CMB photons + neutrinos) ΩB ~ 0.02 h −2 ~ 0.04 (baryons) ΩM ~ 0.3 (Dark Matter) ΩΛ ~ 0.7 (Dark Energy) Ω0 ≡ ΩR + ΩM + ΩΛ = 1.0 → Flat Geometry AS 4022 Cosmology Our (Crazy?) Universe Vacuum Dominated accelerating decelerating km/s H 0 ≈ 70 Mpc ΩM ~ 0.3 ΩΛ ~ 0.7 −5 ΩR ~ 8 ×10 Ω0 = 1.0 AS 4022 Cosmology Critical Empty Sub-Critical Cycloid Evolution of Ω Density at a past/future epoch in units of ρ c = 3 H 0 2 /8π G ρ Ω≡ = ∑ Ωw x 3(1+w) = ΩR x 4 + ΩM x 3 + ΩΛ x ≡ 1+ z = R0 /R ρc w in units of critical density 3 H 2 /8π G at the past/future epoch : H02 ΩM x 3 3 ΩM (x) = 2 ΩM x = H ΩM x 3 + ΩΛ + (1− Ω0 )x 2 H02 ΩΛ ΩΛ (x) = 2 ΩΛ = H ΩM x 3 + ΩΛ + (1− Ω0 )x 2 Do we live at a special time ? ΩM ΩΛ log x AS 4022 Cosmology Evolution of Ω ΩM x 3 ΩM (x) = ΩR x 4 + ΩM x 3 + ΩΛ + (1− Ω0 )x 2 ΩΛ ΩΛ (x) = ΩR x 4 + ΩM x 3 + ΩΛ + (1− Ω0 )x 2 € AS 4022 Cosmology “Concordance” Model Three main constraints: 1. Supernova Hubble Diagram 2. Galaxy Counts + M/L ratios ΩM ~ 0.3 3. Flat Geometry ( inflation, CMB fluctuations) Ω0 = ΩM + ΩΛ = 1 2 1 3 concordance model H 0 ≈ 72 ΩM ≈ 0.3 ΩΛ ≈ 0.7 AS 4022 Cosmology HST Key Project -1 H 0 ≈ 72 ± 3 ± 7 km s Mpc Freedman, et al. 2001 ApJ 553, 47. AS 4022 Cosmology −1 Hubble time and radius Hubble constant : R˙ R˙ km/s km/s H≡ H 0 ≡ = 100 h ≈ 70 R Mpc Mpc R 0 Hubble time : 1 tH ≡ = 1010 h −1 yr ≈ 14 ×10 9 yr H0 ~ age of Universe Hubble radius : c RH ≡ = 3000 h −1 Mpc ≈ 4 ×10 9 pc H0 = distance light travels in a Hubble time. ~ distance to the Horizon. AS 4022 Cosmology Age vs Hubble time R˙ H= R R˙ H= R t=t 0 deceleration decreases age acceleration increases age e.g. matter dominated 2R 2/3 ˙ R∝t ⇒ R= 3 t R˙ 2 1 2 1 2 H= = ⇒ t0 = = tH R 3t 3 H0 3 AS 4022 Cosmology tH = 1 H 0 Age = t0 Beyond H0 • Globular cluster ages: t < t0 --> acceleration • Radio jet lengths: DA(z) --> deceleration • Hi-Redshift Supernovae: DL(z) --> acceleration • Dark Matter estimates ---> ΩM ~ 0.3 • Inflation ---> Flat Geometry • CMB power spectra Ω0 ≈ 1.0 € • “Concordance Model” € AS 4022 Cosmology ΩM ~ 0.3 ΩΛ ~ 0.7 Ω0 = ΩM + ΩΛ ≈ 1.0 Age Constraints • Nuclear decay ( U, Th -> Pb ) – – – – Decay times for (232Th,235U,238U) = (20.3, 1.02, 6.45) Gyr 3.7 Gyr = oldest Earth rocks 4.57 Gyr = meteorites ~10 Gyr = time since supernova produced U, Th – ( 235U / 238U = 1.3 --> 0.33, 232Th / 238U = 1.7 --> 2.3 ) • Stellar evolution – 13-17 Gyr = oldest globular clusters • White dwarf cooling – ~13 Gyr = coolest white dwarfs in M4 AS 4022 Cosmology Nuclear Decay Chronology • P=parent D=daughter S=stable isotope of D • Chemical fractionation changes P/S but not D/S: e.g. concentrate D+S in crystals • Samples have same D0 / S0 various P0 / S0 • P decays to D: D/S D0/S0 P(t) = P0 e−t / τ D(t) = D0 + P0 (1− e−t / τ ) = D0 + P(t) (e t / τ −1) D(t) D0 P(t) t / τ = + e −1) ( S(t) S0 S0 AS 4022 Cosmology S(t) = S0 P/S Observed slope = (e t / τ −1) gives age t / τ , typically to ~ 1% Globular Cluster Ages AS 4022 Cosmology Coolest White Dwarfs 12.7± 0.7 Gyr Hansen et al. 2002 ApJ 574,155 € White dwarf cooling ages --> star formation at z > 5. AS 4022 Cosmology Cooling times have been measured using “ZZ Ceti” oscillation period changes. Age Crisis (~1995) ∞ H 0 t0 = ∫ 1 dx ΩM x 3 + ΩΛ + (1− Ω0 ) x 2 x observations : −1 −1 H 0 = 72 ± 8 km s Mpc t 0 ≥ 14 ± 2 Gyr old globular clusters H 0 t 0 ≥ 1.0 ± 0.15 Globular clusters older than the Universe ? Inconsistent with critical-density matter-only model : 2 H 0 t0 = 3 for (ΩM ,ΩΛ ) = (1,0) ( ) Strong theoretical prejudice for inflation. Ω 0 = 1 Doubts about stellar evolution therory (e.g. convection). AS 4022 Cosmology