Authors' preface |
|
ix | |
|
|
xi | |
Prologue: the quest for darkness |
|
xiii | |
|
|
1 | (10) |
|
|
1 | (1) |
|
|
2 | (1) |
|
Newtonian gravitation and finding the invisible |
|
|
2 | (2) |
|
How to measure stellar motions |
|
|
4 | (2) |
|
How galaxies stay inflated |
|
|
6 | (1) |
|
|
7 | (1) |
|
|
7 | (1) |
|
|
7 | (2) |
|
Mass-luminosity relationship |
|
|
9 | (1) |
|
Gravitational versus luminous mass |
|
|
10 | (1) |
|
|
11 | (10) |
|
|
11 | (1) |
|
|
12 | (2) |
|
Oort discovers differential rotation |
|
|
14 | (1) |
|
Oort 'discovers' disk dark matter |
|
|
15 | (1) |
|
|
16 | (1) |
|
|
17 | (1) |
|
Bahcall and the resurgence of interest in disk dark matter |
|
|
17 | (1) |
|
|
18 | (1) |
|
Not the end of disk dark matter |
|
|
18 | (3) |
|
|
21 | (14) |
|
|
21 | (4) |
|
|
25 | (1) |
|
Zwicky and Abell cluster catalogues |
|
|
25 | (2) |
|
|
27 | (1) |
|
Measuring cluster 'pressure' |
|
|
28 | (1) |
|
|
29 | (1) |
|
Mass-luminosity relationship |
|
|
30 | (1) |
|
Results of studying the Coma and Virgo Clusters |
|
|
31 | (1) |
|
Contrast between Oort and Zwicky |
|
|
32 | (3) |
|
|
35 | (14) |
|
How to measure dark matter halos |
|
|
35 | (1) |
|
Beyond the visible disk: the 21-cm line |
|
|
36 | (1) |
|
The first signs of trouble |
|
|
37 | (1) |
|
How to suppress bar structures |
|
|
38 | (2) |
|
|
40 | (1) |
|
|
41 | (3) |
|
Dark matter in elliptical galaxies |
|
|
44 | (1) |
|
Importance of planetary nebulae |
|
|
45 | (2) |
|
Shape of the dark matter halo |
|
|
47 | (1) |
|
Flaring of the hydrogen disk |
|
|
48 | (1) |
|
|
49 | (10) |
|
Rotation curve of the Milky Way |
|
|
49 | (1) |
|
Escape velocity argument (halo stars) |
|
|
49 | (2) |
|
Objective prism reveals halo stars |
|
|
51 | (1) |
|
Proper motions reveal halo stars |
|
|
52 | (1) |
|
Looking for halo stars in the halo |
|
|
53 | (1) |
|
|
53 | (1) |
|
The Magellanic Clouds and Galactic dark matter |
|
|
54 | (4) |
|
Dark matter in the Large Magellanic Cloud |
|
|
58 | (1) |
|
|
59 | (10) |
|
|
59 | (1) |
|
Aaronson's pioneering work |
|
|
59 | (1) |
|
The density of dark halos: Kormendy and Freeman's work |
|
|
60 | (1) |
|
|
61 | (3) |
|
Dark matter in dwarf galaxies |
|
|
64 | (1) |
|
Why do dwarf galaxies have so much dark matter? |
|
|
64 | (1) |
|
Is there a large population of undiscovered dark galaxies? |
|
|
65 | (1) |
|
|
66 | (1) |
|
Lack of dark matter in globular clusters still a mystery |
|
|
67 | (2) |
|
|
69 | (14) |
|
How gravity deflects starlight |
|
|
69 | (3) |
|
The mechanics of gravitational lensing |
|
|
72 | (1) |
|
|
72 | (1) |
|
Probability of lensing events |
|
|
73 | (2) |
|
Using gravitational lensing to measure dark matter |
|
|
75 | (1) |
|
Strong lensing and the Hubble constant |
|
|
75 | (2) |
|
|
77 | (1) |
|
|
77 | (6) |
|
|
83 | (10) |
|
Ω (omega) as a common unit of measurement |
|
|
83 | (1) |
|
|
84 | (1) |
|
|
84 | (1) |
|
Observing baryonic matter |
|
|
85 | (1) |
|
|
86 | (1) |
|
|
86 | (1) |
|
|
87 | (1) |
|
|
87 | (1) |
|
|
88 | (1) |
|
Baryonic matter in groups and clusters of galaxies |
|
|
88 | (1) |
|
|
89 | (1) |
|
Virgo and Coma baryonic matter compared |
|
|
90 | (3) |
|
|
93 | (12) |
|
|
93 | (3) |
|
The Great Melbourne Telescope |
|
|
96 | (2) |
|
|
98 | (1) |
|
|
98 | (2) |
|
Looking at the centre of the Galaxy |
|
|
100 | (1) |
|
|
100 | (1) |
|
Problems and uncertainties |
|
|
100 | (1) |
|
|
101 | (1) |
|
Variable stars, if nothing else |
|
|
102 | (1) |
|
Searching for extrasolar planets |
|
|
102 | (1) |
|
|
102 | (3) |
|
|
105 | (12) |
|
Baryonic dark matter: why it is suspected |
|
|
105 | (1) |
|
|
105 | (1) |
|
|
106 | (1) |
|
|
106 | (2) |
|
|
108 | (1) |
|
|
109 | (1) |
|
|
110 | (1) |
|
|
110 | (1) |
|
|
111 | (1) |
|
How to find intracluster stars |
|
|
112 | (2) |
|
|
114 | (1) |
|
Milgrom's alternative theory of gravity |
|
|
114 | (3) |
|
Exploring Exotica: Neutrinos |
|
|
117 | (6) |
|
Why non-baryonic dark matter is suspected |
|
|
117 | (2) |
|
Classes of non-baryonic dark matter |
|
|
119 | (1) |
|
|
120 | (3) |
|
Exploring Exotica: Wimps and Axions |
|
|
123 | (8) |
|
|
123 | (1) |
|
Fundamental forces and supersymmetry |
|
|
124 | (1) |
|
|
125 | (1) |
|
|
125 | (1) |
|
|
126 | (5) |
|
|
|
|
131 | (8) |
|
|
131 | (1) |
|
Creation of large-scale structure |
|
|
132 | (1) |
|
Cosmic microwave background |
|
|
133 | (2) |
|
|
135 | (4) |
|
|
139 | (8) |
|
Critical density preferred |
|
|
139 | (1) |
|
An accelerating Universe: dark energy |
|
|
140 | (1) |
|
What is the cosmological constant? |
|
|
141 | (1) |
|
|
141 | (2) |
|
|
143 | (1) |
|
Constraining Ωb, Ωm and ΩΛ |
|
|
143 | (2) |
|
|
145 | (2) |
|
Appendix 1 What is matter? |
|
|
147 | (6) |
|
|
147 | (1) |
|
|
148 | (1) |
|
|
148 | (1) |
|
|
149 | (1) |
|
|
149 | (1) |
|
Structure of the atom: electrons, protons and neutrons |
|
|
149 | (1) |
|
|
150 | (1) |
|
|
150 | (1) |
|
|
150 | (3) |
|
Appendix 2 Expressing mass |
|
|
153 | (2) |
Index |
|
155 | |