Chapter 1 Introduction
Basic Ideas
Isotropic & Homogeneous
Counts of faint galaxies in different directions
CMB ( 99% of photons in the universe ) - low fluctuations ( $10^{-5} \mathrm{K}$ )
Expansion
Hubble (1929) redshift-distance relation
Scatter of galaxies - peculiar motions
Cosmic distance ladder
Cepheids
Ia SN
Fundamental Observers
Fluid (Plasma)
Substratum (相对宇宙静止)——comoving
We are not fundamental observers! (velocity relative to the sun, the Galactic center, M31, Virgo Cluster…) - subtract all the relative velocity - confirmed by highly isotropic CMB
Distances
1 AU = 1.5e13 cm
1 Parsec = 3.26 ly, mostly kpc or Mpc (8.7 kpc away from the Galactic center)
Radius of the Observable Universe (Inside the horizon) $\sim$ 4450 Mpc ( $c/H_0$ )
Masses
Solar mass $M_\odot$ = 2e33 g
Milky Way
Stellar mass $\sim$ 1e11 $M_\odot$
Total mass $\sim$ 1e12 $M_\odot$
Luminosity and Magnitudes
For flux $F$ and apparent magnitude $m$
Absolute magnitude $M$ - a distance of 10 pc
Cosmological Principle
Homogeneous - each point is ordinary
Isotropic - each direction is ordinary
Copernican Principle - humans, on the Earth or in the Solar System, are not privileged observers of the universe
Universal cosmic time
Redshifts
Doppler Redshift is associated with a speed of recession
The SR case is used when, for example, measuring the ejection velocity of gas clouds ejected from AGNs
We will prove that
where $a$ is the scale factor of the universe,$em$ stands for emission
Universal Expansion
1929 Hubble Law - observing Cepheids
Today - Ia SN
Hubble time
Components of the Universe
Non-relativistic $pc\ll mc^2$
Baryons
Proton + Neutron + Electron
None relativistic
0.5% stars
4% Hydrogen/Helium
0.03% heavy elements
0.3% Neutrinos
mass > 0
Relativistic
Radiation
$E=h\nu=hc/\lambda$, 0 mass
21% Dark Matter
Evidence
Rotation velocity of galaxies
Cluster
Gravitational lensing
74% Dark Energy
Accelerate universal expansion after z = 1
Critical Density
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