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9789812388407

Dark Matter in the Universe : The Jerusalem Winter School for Theoretical Physics

by ; ;
  • ISBN13:

    9789812388407

  • ISBN10:

    9812388400

  • Edition: 2nd
  • Format: Hardcover
  • Copyright: 2004-09-30
  • Publisher: WORLD SCIENTIFIC PUB CO INC
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Summary

If standard gravitational theory is correct, then most of the matter in the universe is in an unidentified form which does not emit enough light to have been detected by current instrumentation. This review volume is the extended editon of the lectures given in the 4th Jerusalem Winter School of Theoretical Physics, with new materials added in. It devoted to the discussion of the so-called "missing matter" problem in the universe - dark matter and dark energy. The goal of this volume is to make current research work on unseen matter accessible to students of faculties without prior experience in this area. Due to the pedagogical nature of the notes and the intense discussions between students and the lecturers, the written lectures included in this volume often contain techniques and explanations not found in more formal journal publications.

Table of Contents

Foreword to the First Edition v
Chapter 1. Introduction 1(6)
John N. Bahcall
Chapter 2. Distribution of Dark Matter in the Spiral Galaxy NGC 3198 7(18)
T.S. van Albada, K. Begeman, R. Sanscisi and J.N. Bahcall
1 Introduction
7(4)
2 Distribution of Light
11(1)
3 Rotation Curve
12(2)
4 Mass Models
14(5)
4.1 Choice of Components
14(1)
4.2 Fits with Exponential Disk and Halo
14(4)
4.3 An Upper Limit for the Mass of the Spheroidal Component
18(1)
5 Discussion
19(2)
Appendix: Dark Matter and the Tully-Fisher Relation
21(1)
References
22(3)
Chapter 3. Some Possible Regularities in Missing Mass 25(10)
John N. Bahcall and Stefano Casertano
1 Introduction
25(1)
2 The Simplicity
25(2)
3 The Numerical Characteristics
27(3)
4 The Local Missing Mass
30(1)
5 Implications
30(2)
References
32(3)
Chapter 4. Evolution of Globular Clusters and the Globular Cluster System - I 35(22)
J.P. Ostriker and C. Thompson
1 Globular Clusters
35(1)
2 Basic Properties of Globular Clusters
36(1)
3 Equilibrium Structure of Globular Clusters
37(5)
4 Methods of Computing the Evolution of a Globular Cluster
42(1)
5 Early Evolution of an Isolated Globular Cluster
42(2)
6 Effects of Finite Stellar Size: Heating and Core Bounce
44(5)
7 External Effects on the Evolution of a Globular Cluster
49(2)
8 Evolution of the Globular Cluster System: Destruction of Clusters
51(1)
9 Outstanding Issues
52(1)
10 Nature of the Dark Halo of Our Galaxy
53(2)
References
55(2)
Chapter 5. Positive Energy Perturbations in Cosmology - II 57(14)
J.P. Ostriker and C. Thompson
1 Hydrodynamics in a Cosmological Setting
57(3)
2 Various Self-Similar Solutions for Blast Waves
60(4)
3 Shell Structure
64(1)
4 Equation of Motion of a Thin Shell
65(3)
5 Gravitational Instabilily in a Shell
68(1)
6 Interactions between Cosmological Blasts
69(1)
References
70(1)
Chapter 6. Dark Matter in Galaxies and Galaxy Systems 71(32)
Scott Tremaine and Hyung Mok Lee
1 Introduction
71(8)
1.1 Virial Theorem
72(1)
1.2 History of Dark Matter
73(2)
1.3 A Quick Review of Cosmology
75(3)
1.4 Mass-to-light Ratio in the Solar Neighbourhood
78(1)
1.5 Classification Scheme of Dark Matter
78(1)
2 Theory of Stellar Dynamics
79(7)
2.1 Collisionless Boltzmann Equation
79(3)
2.2 The Jeans Theorem
82(1)
2.3 Examples of Distribution Functions
83(1)
2.3.1 Plummer model
83(1)
2.3.2 Isothermal sphere
84(1)
2.4 Moments of the Collisionless Boltzmann Equation
85(1)
3 Elliptical Cores and Dwarf Spheroidal Galaxies
86(4)
4 The Extent of the Galactic Halo
90(5)
4.1 Local Escape Speed
90(1)
4.2 Magellanic Stream
91(1)
4.3 Local Group Timing
91(1)
4.4 Kinematics of Satellite Galaxies
92(3)
4.5 Summary
95(1)
5 Binary Galaxies
95(2)
6 Masses of Groups and Clusters of Galaxies
97(3)
6.1 Groups of Galaxies
97(1)
6.2 Rich Clusters: Coma Cluster
98(2)
7 Summary
100(1)
References
101(2)
Chapter 7. Gravitational Lenses 103(56)
Roger D. Blandford and Christopher S. Kochanek
1 Introduction
103(5)
1.1 History
103(1)
1.2 Simple Estimates
104(3)
1.3 Uses
107(1)
1.4 Organization of Lectures
107(1)
References
108(1)
2 The Optics of Gravitational Lenses
108(9)
2.1 Vector Formalism
109(1)
2.1.1 The lens equation
109(1)
2.1.2 Image amplification and parity
110(1)
2.1.3 Distance measures
111(1)
2.2 Scalar Formalism: Fermat's Principle
112(3)
2.3 Propagation Formalism: The Optical Scalar Equations
115(1)
References
116(1)
3 Gravitational Potential Wells
117(7)
3.1 Uniform Sheet
117(1)
3.2 Point Mass (Black Hole)
117(1)
3.3 Singular Isothermal Sphere
118(1)
3.4 Isothermal Sphere with Finite Core
118(3)
3.5 Elliptical Potentials
121(1)
3.6 Irregular Potentials
122(1)
3.7 Cosmic Strings
122(2)
References
124(1)
4 Generic Features of Images
124(9)
4.1 Arrival Time Surfaces
124(3)
4.2 Caustics and Catastrophes
127(1)
4.2.1 Structural stability of images
127(1)
4.2.2 Isolated image
128(1)
4.2.3 Fold catastrophe
129(1)
4.2.4 Cusp catastrophe
130(1)
4.2.5 Higher order catastrophes
131(1)
4.3 Caustics as Conjugate Points of Ray Congruences
132(1)
References
133(1)
5 Microlensing
133(5)
5.1 Order of Magnitude Estimates
133(2)
5.2 The Character of Microimages: Low Optical Depth
135(1)
5.3 The Character of Microimages: Moderate Optical Depth
135(2)
5.4 The Character of Microimages: Large Optical Depth
137(1)
References
137(1)
6 Compound Lenses
138(3)
References
140(1)
7 The Observational Position
141(11)
7.1 A Reprise of Existing Candidates
141(1)
7.1.1 The double QSO: 0957 + 561
141(1)
7.1.2 PG 1115 + 080
141(1)
7.1.3 2016 + 112
142(1)
7.1.4 2237 + 0305
142(1)
7.1.5 3C324
143(1)
7.1.6 1042 + 178
143(1)
7.1.7 The dark matter lenses: 2345 + 007, 1635 + 267, and 0023 + 171
143(1)
7.1.8 1146 + 111
144(1)
7.2 Space Density of Sources - Quasars, Galaxies, and Radio Sources
145(1)
7.3 Space Density of Lenses - Galaxies and Clusters
145(1)
7.4 Amplification Bias
146(1)
7.5 Surveys and Future Prospects
146(1)
References
147(5)
8 Lenses as Probes of the Universe
152(5)
8.1 The Hubble Constant
152(1)
8.2 Galactic Masses
153(2)
8.3 Lensing by Dark Matter
155(1)
References
156(1)
9 Concluding Remarks
157(2)
Chapter 8. An Introduction to Inflation 159(10)
William H. Press and David N. Spergel
1 Review of Big Bang Cosmology
159(3)
2 Inflation
162(3)
3 Additional Topics Not Covered Here
165(2)
References
167(2)
Chapter 9. Wimps in the Sun and in the Lab 169(14)
William H. Press and David N. Spergel
1 WIMPS and the Solar Neutrino Problem
169(7)
2 Detecting WIMPS in the Lab
176(3)
References
179(4)
Chapter 10. An Introduction to Cosmic Strings 183(14)
William H. Press and David N. Spergel
1 Birth of Cosmic Strings
183(3)
2 The Motion of a Cosmic String Loop
186(3)
3 Cosmic Strings and the Formation of Galaxies
189(5)
3.1 Spherical Accretion Model
190(2)
3.2 Competition between Loops
192(1)
3.3 Galaxy Morphology
193(1)
4 Observing Cosmic Strings
194(1)
References
194(3)
Chapter 11. A Departure from Newtonian Dynamics at Low Accelerations as an Explanation of the Mass-Discrepancy in Galactic Systems 197(20)
Mordehai Milgrom
1 Introduction
198(2)
2 Dynamics at Low Accelerations
200(3)
3 A Nonrelativistic Formulation
203(2)
4 Effects of an Ambient Field
205(2)
5 Observational Consequences
207(8)
5.1 Disc Galaxies
208(3)
5.2 Elliptical Galaxies
211(2)
5.3 The General Expression for the "Dark Matter" Density
213(1)
5.4 The Sign of the Phantom Density-Negative "Dark Matter"
214(1)
5.5 Phantom Matter in Galactic Discs
214(1)
References
215(2)
Chapter 12. Dark Matter in Cosmology 217
Anthony Aguirre
1Introduction
217(1)
2 Dark Matter and Structure Formation
218(5)
2.1 Initial Conditions and the Standard Cosmological Model
218(1)
2.2 Evolution of Perturbations
219(4)
3 Tests and Constraints from the Microwave Background
223(2)
4 Tests and Constraints from the Ly-α Forest and Distribution of Galaxies
225(1)
5 Dark Matter and Galaxy Formation
226(6)
5.1 Halo Formation
226(1)
5.2 The Halo Mass Function
227(1)
5.3 Halo Profiles
228(1)
5.4 Angular Momentum
228(1)
5.5 From a Dark Halo to a Galaxy
229(1)
5.6 Current Status of Galaxy Formation Theory
229(1)
5.7 Outstanding Problems. and Alternatives to (Cold) Dark Matter
230(2)
Conclusions
232(1)
References
232

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