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E-grāmata: First Galaxies in the Universe

  • Formāts: 560 pages
  • Sērija : Princeton Series in Astrophysics
  • Izdošanas datums: 15-Jan-2013
  • Izdevniecība: Princeton University Press
  • Valoda: eng
  • ISBN-13: 9781400845606
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  • Formāts: 560 pages
  • Sērija : Princeton Series in Astrophysics
  • Izdošanas datums: 15-Jan-2013
  • Izdevniecība: Princeton University Press
  • Valoda: eng
  • ISBN-13: 9781400845606
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This book provides a comprehensive, self-contained introduction to one of the most exciting frontiers in astrophysics today: the quest to understand how the oldest and most distant galaxies in our universe first formed. Until now, most research on this question has been theoretical, but the next few years will bring about a new generation of large telescopes that promise to supply a flood of data about the infant universe during its first billion years after the big bang. This book bridges the gap between theory and observation. It is an invaluable reference for students and researchers on early galaxies.

The First Galaxies in the Universe starts from basic physical principles before moving on to more advanced material. Topics include the gravitational growth of structure, the intergalactic medium, the formation and evolution of the first stars and black holes, feedback and galaxy evolution, reionization, 21-cm cosmology, and more.

  • Provides a comprehensive introduction to this exciting frontier in astrophysics
  • Begins from first principles
  • Covers advanced topics such as the first stars and 21-cm cosmology
  • Prepares students for research using the next generation of large telescopes
  • Discusses many open questions to be explored in the coming decade

Recenzijas

"Loeb and Furlanetto, highly respected experts in the field, have written an up-to-date book that explores the early stages of the universe from the big bang through the formation of the first stars and galaxies."--Choice "[ R]eaders who are genuinely into the subject will take pleasure in reading this book, even if they already know some of the analyses presented in the more basic chapters."--B. Ishak, Contemporary Physics "Everybody who is interested in the topics such as formation and evolution of the first Galaxies, black Holes, Sun and Earth in the Universe will benefit from this book."--Gasanbek T. Arazov, Zentralblatt MATH "[ G]raduate students or senior undergraduates will find The First Galaxies in the Universe a thorough introduction to the topic. Interested professionals will find it a helpful entry point to the specialist literature on one of the most exciting frontiers in astrophysics."--Jason Tumlinson, Physics Today

Preface xi
PART I Fundamentals Of Structure Formation
1(130)
Chapter 1 Introduction and Cosmological Background
3(22)
1.1 Preliminary Remarks
3(2)
1.2 Standard Cosmological Model
5(10)
1.3 Milestones in Cosmic Evolution
15(5)
1.4 Most Matter Is Dark
20(5)
Chapter 2 Linear Growth of Cosmological Perturbations
25(16)
2.1 Growth of Linear Perturbations
25(10)
2.2 The Thermal History during the Dark Ages
35(6)
Chapter 3 Nonlinear Structure and Halo Formation
41(51)
3.1 Spherical Collapse
41(4)
3.2 Cosmological Jeans Mass
45(6)
3.3 Halo Properties
51(5)
3.4 Abundance of Dark Matter Halos
56(9)
3.5 Halo Clustering in Linear Theory
65(3)
3.6 The Nonlinear Power Spectra of Dark Matter and Galaxies
68(10)
3.7 Numerical Simulations of Structure Formation
78(14)
Chapter 4 The Intergalactic Medium
92(39)
4.1 The Cosmic Web
92(3)
4.2 Lyman-α Absorption in the Intergalactic Medium
95(5)
4.3 Theoretical Models of the Lyman-α Forest
100(14)
4.4 The Metagalactic Ionizing Background
114(6)
4.5 The Helium-Ionizing Background
120(1)
4.6 Metal-Line Systems
121(4)
4.7 The Lyman-α Forest at z > 5
125(6)
PART II The First Structures
131(204)
Chapter 5 The First Stars
133(41)
5.1 From Virialized Halos to Protostars
136(8)
5.2 From Protostars to Stars
144(13)
5.3 The Second Generation of Stars: "Population III.2"
157(6)
5.4 Properties of the First Stars
163(5)
5.5 The End States of Population III Stars
168(2)
5.6 Gamma-Ray Bursts: The Brightest Explosions
170(4)
Chapter 6 Stellar Feedback and Galaxy Formation
174(43)
6.1 The Ultraviolet Background and H2 Photodissociation
174(10)
6.2 The X-ray Background: Positive Feedback
184(2)
6.3 Radiative Feedback: Mechanical Effects
186(6)
6.4 Galactic Superwinds and Mechanical Feedback
192(9)
6.5 Metal Enrichment and the Transition to Population II Star Formation
201(10)
6.6 The First Galaxies
211(6)
Chapter 7 Supermassive Black Holes
217(34)
7.1 Quasars and Black Holes: An Overview
217(5)
7.2 Basic Principles of Astrophysical Black Holes
222(3)
7.3 Accretion of Gas onto Black Holes
225(7)
7.4 The First Black Holes and Quasars
232(5)
7.5 Black Holes and Galaxies
237(7)
7.6 Black Hole Binaries
244(3)
7.7 Gravitational Waves from Black Hole Mergers
247(4)
Chapter 8 Physics of Galaxy Evolution
251(32)
8.1 High-Redshift Galaxies
251(2)
8.2 Gas Accretion
253(2)
8.3 Halo Mergers
255(1)
8.4 Disk Formation
256(2)
8.5 Star Formation in Galaxies
258(5)
8.6 Black Hole Growth in Galaxies
263(1)
8.7 Feedback and Galaxy Evolution
264(2)
8.8 From Galaxy Model to Stellar Spectra
266(3)
8.9 Signatures of the Interstellar Medium
269(6)
8.10 Gravitational Lensing
275(8)
Chapter 9 The Reionization of Intergalactic Hydrogen
283(52)
9.1 Propagation of Ionization Fronts
283(5)
9.2 Global Ionization History
288(3)
9.3 The Phases of Hydrogen Reionization
291(2)
9.4 The Morphology of Reionization
293(9)
9.5 Recombinations inside Ionized Regions
302(6)
9.6 Simulations of Reionization
308(7)
9.7 Statistical Properties of the Ionization Field
315(4)
9.8 Reionization by Quasars and Other Exotic Sources
319(7)
9.9 Feedback from Reionization: Photoheating
326(9)
PART III Observations Of The Cosmic Dawn
335(160)
Chapter 10 Surveys of High-Redshift Galaxies
337(30)
10.1 Telescopes for Observing High-Redshift Galaxies
337(3)
10.2 Methods for Identifying High-Redshift Galaxies
340(10)
10.3 Luminosity and Mass Functions
350(7)
10.4 The Statistics of Galaxy Surveys
357(10)
Chapter 11 The Lyman-α Line as a Probe of the Early Universe
367(41)
11.1 Lyman-α Emission from Galaxies
367(8)
11.2 The Gunn-Peterson Trough
375(1)
11.3 IGM Scattering in the Blue Wing of the Lyman-α Line
376(6)
11.4 The Red Damping Wing
382(6)
11.5 The Lyman-α Forest as a Probe of the Reionization Topology
388(2)
11.6 Lyman-α halos around Distant Sources
390(6)
11.7 Lyman-α Emitters during the Reionization Era
396(12)
Chapter 12 The 21-cm Line
408(51)
12.1 Radiative Transfer of the 21-cm Line
410(2)
12.2 The Spin Temperature
412(8)
12.3 The Brightness Temperature of the Spin-Flip Background
420(8)
12.4 The Monopole of the Brightness Temperature
428(4)
12.5 Statistical Fluctuations in the Spin-Flip Background
432(7)
12.6 Spin-Flip Fluctuations during the Cosmic Dawn
439(7)
12.7 Mapping the Spin-Flip Background
446(13)
Chapter 13 Other Probes of the First Galaxies
459(36)
13.1 Secondary Cosmic Microwave Background Anisotropies from the Cosmic Dawn
459(11)
13.2 Diffuse Backgrounds from the Cosmic Dawn
470(14)
13.3 The Cross-Correlation of Different Probes
484(4)
13.4 The Fossil Record of the Local Group
488(7)
Appendix A Useful Numbers 495(2)
Appendix B Cosmological Parameters 497(2)
Notes 499(10)
Further Reading 509(4)
Index 513
Abraham Loeb is Frank B. Baird, Jr. Professor of Science, chair of the Astronomy Department, and director of the Institute for Theory and Computation at Harvard University. Loeb is a member of the American Academy of Arts and Sciences. He is the author of How Did the First Stars and Galaxies Form? (Princeton). Steven R. Furlanetto is associate professor of physics and astronomy at the University of California, Los Angeles.