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PHY 4460 RELATIVITY

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3. Galaxies are receding from us. Redshift velocity. V. 4. Velocity distance s ... But light from distant galaxies came from long time ago. If earlier H is larger ... – PowerPoint PPT presentation

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Title: PHY 4460 RELATIVITY


1
PHY 4460RELATIVITY
  • K Young, Physics Department, CUHK
  • ?The Chinese University of Hong Kong

2
CHAPTER 11POOR MAN'S COSMOLOGY
3
Objectives
  • The problem of cosmology
  • Observational evidence
  • Kinematics
  • Dynamics
  • Belief in 1920s, 1960s, 21st century

4
Observational Evidence
5
Observational evidence
  • Isotropic
  • Principle of cosmology
  • Homogeneous
  • Expansion

6
1. Universe is isotropic
YES
NO
7
2. Our position is not special
8
2. Our position is not special
NO
YES
Would not be isotropic from another observational
point
9
Universe is homogeneous!
10
3. Galaxies are receding from us
11
4. Velocity ? distance s (for small distances)
12
Hubble constantis not constant
  • Although
  • it does not mean velocity is uniform
  • and in fact H is changing
  • Present values denoted by subscript0

13
Unit of H
  • v km s-1
  • s Mpc
  • 1 pc 3.26 ly
  • H km s-1 Mpc-1
  • H v / s s-1
  • H-1 s Gyr

14
Value of H0
  • Hubble 1930s 500 units
  • Recent decades 50-100 units
  • 2001 70 units (/- 10)
  • WL Freedman et al

15
Problem
  • Determine s?
  • Determine v?

16
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17
Determine s
L 100 W
  • "Standard" sources Cepheids Know L
  • Measure l
  • Determine s

18
Determine v
19
Uniform motion? T age of universe?
NO !
20
Kinematics
21
Kinematics
  • Co-expansion
  • factorization
  • Single parameter a(t)
  • Expansion
  • H(t)
  • Deceleration
  • q

22
Co-expansion
Factorized
23
v ? s does not imply uniform motion H?1 ? age of
universe
24
Key Equations
25
?
26
If earlier H is larger, then decelerating (to be
qualified)
27
(No Transcript)
28
How to express deceleration
  • Dimensionless

29
Example inNewtonian Gravity
30
Stone
31
  • Escape KE gt PE q lt 1/2

Marginal KE PE q 1/2 Not escape KE lt PE q
gt 1/2
32
Deceleration parameter
  • How do we know whether expansion is

33
In principle
  • Measure H or T
  • now
  • 0.1 Gyr ago
  • Find difference

34
In practice?
  • We do not have data from long time ago
  • But light from distant galaxies
    came from long time ago

35
  • If earlier H is larger
  • Then amount of deviation is a measure (q) of how
    much larger

36
In practice?
  • Slope of each part
  • Tells us H at some time in past
  • Can trace H(t)
  • Actually dynamical model with a few parameters
  • Fit diagram to determine parameters

37
  • Model

38
Homogeneous and Isotropic Spatial Geometries
39
Homogeneous and isotropic spatial geometries
  • Flat
  • Closed sphere

40
Homogeneous and isotropic spatial geometries
  • Open
  • like a saddle

All described by a(t) ???
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