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Big Bang 3rd Revised edition [Kietas viršelis]

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  • Formatas: Hardback, 480 pages, aukštis x plotis: 230x150 mm, weight: 837 g, illustrations
  • Išleidimo metai: 06-Dec-2000
  • Leidėjas: W.H.Freeman & Co Ltd
  • ISBN-10: 0716742462
  • ISBN-13: 9780716742463
Kitos knygos pagal šią temą:
  • Formatas: Hardback, 480 pages, aukštis x plotis: 230x150 mm, weight: 837 g, illustrations
  • Išleidimo metai: 06-Dec-2000
  • Leidėjas: W.H.Freeman & Co Ltd
  • ISBN-10: 0716742462
  • ISBN-13: 9780716742463
Kitos knygos pagal šią temą:
The Big Bang theory of the birth of the universe teaches that billions of years ago there was a hot, violent explosion of elementary particles and radiation. What do we know about this ultimate moment of creation, and how do we know it? This is an introduction to scientific cosmology, and the third edition of this book provides a sweeping account of events. New to this edition are: photographs and measurements from the Hubble Space Telescope, Cosmic Background Explorer Satellite and Infrared Space Observatory; new ideas in string and superstring theory; and ideas about black holes, worm holes, quantum foam and multiple universes.
Preface xi
Introduction to Cosmology
1(8)
Cosmological Principles
2(4)
Modern Cosmologies
6(2)
The Big Bang
8(1)
Origins of Modern Cosmology
9(20)
The Giants of Classical Cosmology
10(6)
The Renaissance of Cosmology
16(6)
Issues in Modern Cosmology
22(2)
The Giants of Modern Cosmology
24(5)
Observational Cosmology
29(34)
The Extragalactic Distance Scale
31(7)
The Most Distant Objects
38(8)
The Recession of the Galaxies
46(7)
The Homogeneity of the Universe
53(2)
Olbers' Paradox
55(3)
Mach's Principle: The Concept of Inertia
58(5)
Evidence for the Big Bang
63(22)
The Age of the Universe
63(2)
The Cosmic Time Scale
65(6)
Radio Galaxies
71(4)
The Cosmic Microwave Background Radiation
75(6)
Helium and Deuterium in the Universe
81(4)
Cosmological Models
85(20)
The Curvature of Space
85(3)
Observable Horizons
88(3)
Newtonian Cosmology
91(1)
A Raisin Pudding Model of the Universe
92(4)
Big Bang Models
96(4)
Cosmological Repulsion
100(5)
The First Millisecond
105(34)
The Density of the Universe
107(2)
The Temperature of the Big Bang
109(2)
The Physics of Creation
111(2)
In the Beginning
113(2)
Inflation
115(7)
The Legacy of Inflation
122(1)
Strings
123(3)
The Particle Zoo
126(3)
Probing the Nature of Relics from the Big Bang
129(1)
Mini- Black Holes
130(4)
Matter and Antimatter
134(5)
The Thermonuclear Detonation of the Universe
139(10)
Neutrons
140(1)
Nucleosynthesis
141(1)
Universal Helium Abundance
142(1)
Deuterium Abundance
143(6)
The Primeval Fireball Emerges
149(20)
The Case of the Elusive Neutrinos
150(5)
Characteristics of the Background Radiation
155(2)
The Density of Matter and Radiation
157(1)
Radiation Temperature
158(1)
Scattering
159(2)
Primordial Chaos?
161(1)
The End of the Radiation Era
162(1)
The Cooling of Matter
163(6)
The Origin of the Galaxies
169(18)
The Conservative Approach
170(2)
The Revolutionary Approach
172(4)
A Cosmic Filter
176(7)
The Dominance of Cold Dark Matter
183(4)
The Evolution of the Galaxies
187(34)
Merging
189(1)
The Collapse of a Protogalactic Cloud
189(2)
Rotation
191(1)
The Formation of Protogalaxies
192(2)
The Formation of Galaxies and Galaxy Clusters
194(8)
The Luminosity Function
202(1)
The Formation of the Stars
202(3)
Elliptical and Spiral Galaxies
205(6)
The Archeology of the Milky Way
211(2)
Mergers and Infall
213(2)
The History of Cosmic Star Formation
215(1)
Galaxy Gobbling
216(5)
The Theory of Galaxy Formation
221(12)
Mergers and Fragmentation
222(2)
Dwarf Galaxies and Young Galaxies
224(2)
The Fate of Cold Dark Matter
226(2)
Lyman-Break Galaxies
228(1)
The Cosmic Star-Formation History
229(4)
Giant Clusters of Galaxies
233(26)
Galaxy Clustering
235(4)
Hubble Bubbles
239(1)
Intergalactic Gas
240(5)
Galaxy Collisions
245(2)
Dark Matter
247(8)
Massive Compact Halo Objects: MACHOs
255(1)
Weakly Interacting Massive Particles: WIMPs
256(1)
The Origin of the Giant Clusters
257(2)
Radio Galaxies and Quasars
259(26)
Radio Emission and Radio Galaxies
259(8)
Quasi-Stellar Radio Sources
267(9)
Gravitational Lenses
276(2)
Theories of Quasars and Radio Galaxies
278(7)
The Formation of the Stars
285(24)
The Birth and Death of Stars
285(3)
The First Stars
288(8)
Current Star Formation
296(3)
Molecular Clouds
299(2)
Stellar-Mass Distribution
301(8)
The Morphology of Galaxies
309(20)
Rotation and Density Waves
309(5)
The Role of Magnetic Fields
314(3)
Elliptical Galaxies and Globular Clusters
317(3)
The Colors of Galaxies
320(3)
Morphology and Galaxy Formation
323(6)
The Origin of the Heavy Elements
329(26)
The Nuclear Evolution of Stars
330(1)
White Dwarfs
331(2)
Neutron Stars
333(4)
Black Holes
337(2)
Explosive Nucleosynthesis
339(1)
Elemental Abundances
340(5)
Supernovae and the Solar System
345(2)
The Formation of the Earth and Life
347(3)
Catastrophic Evolution
350(1)
Life in the Universe
351(4)
Into the Infinite Future
355(30)
The Mass Density of the Universe
355(4)
Galaxies as Cosmological Probes
359(2)
Measuring the Curvature of Space
361(7)
The Acceleration of the Universe
368(1)
Quasars as Cosmological Probes
369(1)
Deuterium and Mass Density
370(2)
The Hubble Expansion
372(4)
The Future of Open and Closed Universes
376(9)
Alternatives to the Big Bang
385(24)
Quantum Origins
387(1)
Wormholes
388(1)
Multiple Universes
389(1)
Tired-Light Cosmologies
390(1)
Arpian Objects
391(1)
Steady State Cosmology
392(1)
Galaxies and Antigalaxies
393(2)
Variable Gravitation
395(1)
A Shrinking Universe
396(1)
Avoiding the Singularity
397(2)
Chaos versus Order
399(1)
A Cold Universe
400(1)
Forecasting the Infinite Future
401(1)
The Future of Cosmology
402(1)
New Tests
403(2)
A New Physics
405(4)
Mathematical Notes 409(40)
For Further Reading 449(6)
Glossary 455(24)
Index 479