The oldest science? One of the most rapidly evolving fields of...
Transcript of The oldest science? One of the most rapidly evolving fields of...
The oldest science?
One of the most rapidly evolving fields of modern research.
Driven by observations and instruments
Intersection of physics (fundamental laws) and astronomy (contents of the universe)
Study of the Universe viewed as a whole (not a very humble field of science! Must coarse-grain and shove some details under the rug.)
general relativity (back bone) astronomy (supporting data) particle physics (evolution at earliest epochs) plasma physics (a physical system; objects) thermodynamics (of an expanding plasma) chemistry (late evolution; individual objects) statistics (large scale description, initial cond’s) mathematical physics (earliest stages) … cosmetology (“kosmos”=“harmony”)
~ 80 years old (external galaxies, expansion) ~ 40 yrs ago: CMB (hot big bang, structures) ~ 10 yrs: Dark Energy (???)
cf. Particle Physics: less rigorously defined open questions, puzzles are more numerous, and more fundamental
• I. Cosmological Principle homogeneous and isotropic on large scales • II. Expansion: kinematics expanding in a way that preserves I. → Hubble • III. Expansion: dynamics obeys general relativity theory • IV. Hot Big Bang hot dense state, dominated by thermal radiation • V. Inflation(*) initial exponential (“superluminal”) expansion • VI. The Dark Sector(**) to account for apparent acceleration + large structures
• Galaxy Counts - follow N(>f) ∝ f -3/2 historical argument; must now disentangle space-time curvature and galaxy evolution - statistics: δN/〈N〉 vs L monotonically decreasing L ~ 30 Mpc gives δN/〈N〉 ~ 0.5 (IRAS) - more elaborate statistics: power spectra (2d,3d) low power on large scales
Distance (1pc = 3 light years)
Velo
city
(km
/s)
• Hubble (1929): redshift vs distance to 20 galaxies (Cepheids) • Linear expansion v=H0d → Hubble length: d=c/H0 ~ 5 Gpc
• Non-linear expansion law can be explained within relativistic theory
• But it requires a lot of “dark energy”:
Dark Energy Dark Matter Neutrinos Ordinary gas and stars
• Hot radiation from the big bang, which has cooled to ~3 Kelvin by present epoch • Predicted in 1948 (Gamow; Alpher & Herman) → expanding universe a background for plasma/nuclear physics prediction (4K) based on light elements (D) • Observed in 1965 (Penzias & Wilson) • Extremely smooth, but seeds of structure discovered by COBE (1992) and WMAP (2003) • Accounts for 3% of the static on your TV screen!
Extremely accurately measured quantity The most precisely measured example of a black-body spectrum
Implies thermal equilibrium Temperature measured to be T=2.725 ± 0.001 K Too cold and dilute to achieve equilibrium today - real puzzle outside the big bang model - natural by-product of hot dense phase
Supports: • Cosmological principle (isotropy) • Laws of nature not varying even over cosmic scales • Universe expanded • Universe was much hotter in the past • A puzzle: horizon problem. Inflation?
CMB angular and frequency structures contain a wealth of cosmological information
Amplitude of the temperature fluctuations is consistent with gravitational structure formation
This wealth of detail (to be discussed in future lectures) is all consistent with the hot big bang + cold dark matter structure formation model
hard feat for alternative to replicate / postdict!
• Paradigm? Model? Picture? Principle? Scenario? Theory? Idea? Mechanism?
[you decide]
• Solves some major problems: - flatness problem - horizon problem - monopole problem
• No compelling competing idea for (i) starting expansion and (ii) producing inhomogeneities
• Flat universe with critical density Ω=1.02 ±0.02
• Scale invariant power spectrum of density fluctuations
n=dlnP/dlnk=0.99±0.04
• Relic gravitational waves from metric perturbation (not yet observed, but future CMB experiments can detect them)
What is the nature of dark matter ? What is the nature of dark energy ? Why is the Universe expanding ? What is the origin of initial fluctuations ? What is the physical cause of inflation ? Is General Relativity correct in early universe ?
Many other unsolved ‘astrophysics’ problems: - where are the baryons ? - how did galaxies form ? - what sets properties of intergalactic gas? - ….