Title: COSMOLOGY
1COSMOLOGY
International Meeting of Fundamental
Physics (Winter meeting) Santiago de
Compostela, 2007
Eduard Massó UAB/IFAE
2Program
- The standard cosmological model
- The observed universe
- Inflation. Neutrinos in cosmology
Emphasis on Particles
3Science, vol. 315, 2007
4Our universe is expanding
lights-years ago
co-moving distance
scale
today
redshift
5Co-moving co-ordinates
On top peculiar (real) velocities
6Hubbles law Cosmological principle
Universe homogenous isotropic on large scales
Cosmological principle
Hubble parameter
(today)
Hubbles discovery
Hubbles law
7Expansion (or contraction) is inevitable
Robertson-Walker metric (homogeneity isotropy)
Parameters
Content (matterradiation)
Content too (cosm. const.)
Parameters are related by eqs.
Spatial geometry
8Cosmological equations
Friedmann eqs.
1
2a
12a -gt 2b
9Spatial geometry Light propagation
Open
Closed
FLAT
3D
10Spatial geometry Light propagation
11Luminosity distance
Absolute luminosity E/time in rest frame
Measured flux (E/time/area)
Luminosity distance
12Hubbles law
Exact
Small z
Deceleration parameter
That was kinematics
13Cosmological constant contribution
Negative pressure
any other component
14Solution to cosmological eqs.
Equation of state
Assume i - dominance and
RD universe
MD universe.
CCD universe
15Critical density
Define
Define also (Today)
Not energy-density contribution
16Rewriting Friedmann eqs.
Cosmic sum rule
2a today
Notice signs
17The future
Diff. eq.
Initial conditions taken today
Eternal Expansion OR Recollapse ?
1
2
3
18Distance - Redshift
Co-moving distance to source
Where
Can neglect
Distance-redshift relation is function of
19Age of the universe
look-back time
lifetime
Flat univ.
Our univ.
(Age crisis Open universe gave too low lifetime)
20Which universe ?
21The past universe
nucleosynthesis
rad
recombination
mat
cc
equality
today
next
22The hot universe
Equilibrium thermodynamics
g deg. of freedom
number density
energy density
pressure
distribution
23Decoupling of species
Expansion Interaction
24Phase transitionsSymmetry restoring
2n order
25Phase transitions
1st order
26Conformal time
27Particle Horizon
It is the physical distance photons can travel
until a time t
Defines causal distance at a given time t
28Program
- The standard cosmological model
- The observed universe
- Inflation. Neutrinos in cosmology