点击选择搜索分类
首页 - 励志与成功- 正文
☆☆☆☆☆
||
[德] 马克翰维 著
出版社: 世界图书出版公司 ISBN:9787506292740 版次:1 商品编码:10096503 包装:平装 外文名称:Physical Foundations of COSMOLOGY 开本:16开 出版时间:2009-01-01 用纸:胶版纸 页数:421 正文语种:中文,英语
Acknowledgements
Units and conventions
Part I Homogeneous isotropic universe
1 Kinematics and dynamics of an expanding universe
1.1 Hubble law
1.2 Dynamics of dust in Newtonian cosmology
1.2.1 Continuity equation
1.2.2 Acceleration equation
1.2.3 Newtonian solutions
1.3 From Newtonian to relativistic cosmology
lForeword by Professor Andrei Linde Preface
Acknowledgements
Units and conventions
Part I Homogeneous isotropic universe
1 Kinematics and dynamics of an expanding universe
1.1 Hubble law
1.2 Dynamics of dust in Newtonian cosmology
1.2.1 Continuity equation
1.2.2 Acceleration equation
1.2.3 Newtonian solutions
1.3 From Newtonian to relativistic cosmology
1.3.1 Geometry of an homogeneous,isotropic space
1.3.2 The Einstein equations and cosmic evolution
1.3.3 Friedmann equations
1.3.4 Conformal time and relativistic solutions
1.3.5 Milne universe
1.3.6 De Sitter universe
2 Propagation of light and horizons
2.1 Light geodesics
2.2 Horizons
2.3 Conformal diagrams
2.4 Redshifl
2.4.1 Redshifl as a measure of time and distance
2.5 Kinematic tests
2.5.1 Angular diameter-redshift relation
2.5.2 Luminosity—redshifl relation
2.5.3 Number counts
2.5.4 Redshift evolution
3 The hot universe
3.1 The composition of the universe
3.2 Brief thermal history
3.3 Rudiments of thermodynamics
3.3.1 Maximal entropy state,thermal spectrum, conservation laws and chemical potentials
3.3.2 Energy density,pressure and the equation of state
3.3.3 Calculating integrals
3.3.4 Ultra—relativistic particles
3.3.5 Nonrelativistic particles
3.4 Lepton era
3.4.1 ChemicaI potentials
3.4.2 Neutrino decoupling and electrOn—pOsitrOn annihilation
3.5 NucleOsvnthesis
3.5.1 Freeze—OUt of neutrons
3.5.2“Deuterium bottleneck”
3.5.3 Helium一4
3.5.4 Deuterium
3.5.5 The other light elements
3.6 Recombination
3.6.1 Helium recombination
3.6.2 Hydrogen recombination:equilibrium consideration
3.6.3 Hydrogen recombination:the kinetic approach
4 The very early universe
4.1 Basics
4.1.1 Local gauge invariance
4.1.2 Non—Abelian gauge theories
4.2 Quantum chromodynamics and quark-gluon plasma
4.2.1 Running coupling constant and asymptotic freedom
4.2.2 Cosmological quark-gluon phase transition
4.3 Electroweak theory
4.3.1 Fermion content
4.3.2“Spontaneous breaking”of U(1)symmetry
4.3.3 Gauge bosons
4.3.4 Fermion interactions
4.3.5 Fermion masses
4.3.6 CP violation
4.4 “Symmetry restoration”and phase transitions
4.4.1 Effective potential
4.4.2 U(l)model
4.4.3 Symmetry restoration at high temperature
4.4.4 Phase transitions
4.4.5 Electroweak phase transition
4.5 Instantons.sphalerons and the early universe
4.5.1 Particle escape from a potential well
4.5.2 Decay of the metastable vacuum
4.5.3 The vacuum structure of gauge theories
4.5.4 Chiral anomaly and nonconservation of the fermion number
4.6 Beyond the Standard Model
4.6.1 Dark matter candidates
4.6.2 Baryogenesis
4.6.3 Topological defects
5 Inflation I:homogeneous limit
5.1 Problem of initial conditions
5.2 Inflation:main idea
5.3 How can gravity become“repulsive”?
5.4 How to realize the equation of state P≈一#####
5.4.1 Simple example:V=m2#4#####
5.4.2 General potential:slow—roll approximation
5.5 Preheating and reheating
5.5.1 Elementary theory
5.5.2 Narrow resonance
5.5.3 Broad resonance
5.5.4 Implications
5.6 “Menu”of scenarios
Part II Inhomogeneous universe
6 Gravitational instability in Newtonian theory
6.1 Basic equations
6.2 Jeans theory
6.2.1 Adiabatic perturbations
6.2.2 Vector perturbations
6.2.3 Entropy perturbations
6.3 Instability in an expanding universe
6.3.1 Adiabatic perturbations
6.3.2 Vector perturbations
6.3.3 Self-similar solution
6.3.4 Cold matter in the presence of radiation or dark energy
6.4 Beyond linear approximation
6.4.1 Tolman solution
6.4.2 Zel’dovich solution
6.4.3 Cosmic web
7 Gravitational instability in General Relativity
7.1 Perturbations and gauge—invariant variables
7.1.1 Classification of perturbations
7.1.2 Gauge transformations and gauge—invariant variables
7.1.3 COOrdinate systems
7.2 Equations for cosmological perturbations
7.3 Hydrodynamical perturbations
7.3.1 Scalar perturbations
7.3.2 Vector and tensor perturbations
7.4 Baryon-radiation plasma and cold dark matter
7.4.1 Equations
7.4.2 Evolution of perturbations and transfer functions
8 Inflation II:origin of the primordial inhomogeneities
8.1 Characterizing perturbations
8.2 Perturbations on inflation(slow—roll approximation)
8.2.1 Inside the Hubble scale
8.2.2 The spectrum of generated perturbations
8.2.3 Why dO we need inflation?
8.3 Quantum cosmological perturbations
8.3.1 Equations
8.3.2 Classical solutions
8.3.3 Quantizing perturbations
8.4 Gravitationa waves from inflation
8.5 Self_reDroductiOn of the universe
8.6 Infation as a theory with predictive power
9 Cosmic microwave background anisotropies
9.1 Basics
9.2 Sachs-Wolfe eflfect
9.3 Initial conditions
9.4 Correlation function and multipoles
9.5 Anisotropies on large angular scales
9.6 Delayed recombination and the finite thickness effect
9.7 Anisotropies on small angular scales
9.7.1 Transfer functions
9.7.2 Multipole moments
9.7.3 Parameters
9.7.4 Calculating the spectrum
9.8 Determining cosmic parameters
9.9 Gravitational waves
9.10 Polarization of the cosmic microwave background
9.10.1 Polarization tensor
9.10.2 Thomson scattering and polarization
9.10.3 Delayed recombination and polarization
9.10.4 E and B polarization modes and correlation functions
9.1l Reionization
Bibliography
Expanding universe(Chapters 1 and 2)
Hot universe and nucleosvnthesis(Chapter 3)
Particle physics and early universe(Chapter 4)
Inflation (Chapters 5 and 8)
Gravitational instability(Chapters 6 and 7)
CMB fluctuations(Chapter 9)
lndex
3.1 Geometry of an homogeneous,isotropic space
1.3.2 The Einstein equations and cosmic evolution
1.3.3 Friedmann equations
1.3.4 Conformal time and relativistic solutions
1.3.5 Milne universe
1.3.6 De Sitter universe
2 Propagation of light and horizons
2.1 Light geodesics
2.2 Horizons
2.3 Conformal diagrams
2.4 Redshifl
2.4.1 Redshifl as a measure of time and distance
2.5 Kinematic tests
2.5.1 Angular diameter-redshift relation
2.5.2 Luminosity—redshifl relation
2.5.3 Number counts
2.5.4 Redshift evolution
3 The hot universe
3.1 The composition of the universe
3.2 Brief thermal history
3.3 Rudiments of thermodynamics
3.3.1 Maximal entropy state,thermal spectrum, conservation laws and chemical potentials
3.3.2 Energy density,pressure and the equation of state
3.3.3 Calculating integrals
3.3.4 Ultra—relativistic particles
3.3.5 Nonrelativistic particles
3.4 Lepton era
3.4.1 ChemicaI potentials
3.4.2 Neutrino decoupling and electrOn—pOsitrOn annihilation
3.5 NucleOsvnthesis
3.5.1 Freeze—OUt of neutrons
3.5.2“Deuterium bottleneck”
3.5.3 Helium一4
3.5.4 Deuterium
3.5.5 The other light elements
3.6 Recombination
3.6.1 Helium recombination
3.6.2 Hydrogen recombination:equilibrium consideration
3.6.3 Hydrogen recombination:the kinetic approach
4 The very early universe
4.1 Basics
4.1.1 Local gauge invariance
4.1.2 Non—Abelian gauge theories
4.2 Quantum chromodynamics and quark-gluon plasma
4.2.1 Running coupling constant and asymptotic freedom
4.2.2 Cosmological quark-gluon phase transition
4.3 Electroweak theory
4.3.1 Fermion content
4.3.2“Spontaneous breaking”of U(1)symmetry
4.3.3 Gauge bosons
4.3.4 Fermion interactions
4.3.5 Fermion masses
4.3.6 CP vi 经典英文物理教材系列:宇宙学的物理基础 [Physical Foundations of COSMOLOGY] 电子书 下载 mobi epub pdf txt
经典英文物理教材系列:宇宙学的物理基础 [Physical Foundations of COSMOLOGY]-so88
经典英文物理教材系列:宇宙学的物理基础 [Physical Foundations of COSMOLOGY] pdf epub mobi txt 电子书 下载 2022
图书介绍
☆☆☆☆☆
||
[德] 马克翰维 著
出版社: 世界图书出版公司 ISBN:9787506292740 版次:1 商品编码:10096503 包装:平装 外文名称:Physical Foundations of COSMOLOGY 开本:16开 出版时间:2009-01-01 用纸:胶版纸 页数:421 正文语种:中文,英语
内容简介
This book is meant to be neither encyclopedic nor a sourcebook for the most recent observational data. In fact, I avoid altogether the presentation of data; after all the data change very quickly and are easily accessible from numerous available monographs as well as on the Intemet. Furthermore, I have intentionally restricted the discussion in this book to results that have a solid basis. I believe it is premature to present detailed mathematical consideration of controversial topics in a book on the foundations of cosmology and, therefore, such topics are covered only at a very elementary level.内页插图
目录
Foreword by Professor Andrei Linde PrefaceAcknowledgements
Units and conventions
Part I Homogeneous isotropic universe
1 Kinematics and dynamics of an expanding universe
1.1 Hubble law
1.2 Dynamics of dust in Newtonian cosmology
1.2.1 Continuity equation
1.2.2 Acceleration equation
1.2.3 Newtonian solutions
1.3 From Newtonian to relativistic cosmology
lForeword by Professor Andrei Linde Preface
Acknowledgements
Units and conventions
Part I Homogeneous isotropic universe
1 Kinematics and dynamics of an expanding universe
1.1 Hubble law
1.2 Dynamics of dust in Newtonian cosmology
1.2.1 Continuity equation
1.2.2 Acceleration equation
1.2.3 Newtonian solutions
1.3 From Newtonian to relativistic cosmology
1.3.1 Geometry of an homogeneous,isotropic space
1.3.2 The Einstein equations and cosmic evolution
1.3.3 Friedmann equations
1.3.4 Conformal time and relativistic solutions
1.3.5 Milne universe
1.3.6 De Sitter universe
2 Propagation of light and horizons
2.1 Light geodesics
2.2 Horizons
2.3 Conformal diagrams
2.4 Redshifl
2.4.1 Redshifl as a measure of time and distance
2.5 Kinematic tests
2.5.1 Angular diameter-redshift relation
2.5.2 Luminosity—redshifl relation
2.5.3 Number counts
2.5.4 Redshift evolution
3 The hot universe
3.1 The composition of the universe
3.2 Brief thermal history
3.3 Rudiments of thermodynamics
3.3.1 Maximal entropy state,thermal spectrum, conservation laws and chemical potentials
3.3.2 Energy density,pressure and the equation of state
3.3.3 Calculating integrals
3.3.4 Ultra—relativistic particles
3.3.5 Nonrelativistic particles
3.4 Lepton era
3.4.1 ChemicaI potentials
3.4.2 Neutrino decoupling and electrOn—pOsitrOn annihilation
3.5 NucleOsvnthesis
3.5.1 Freeze—OUt of neutrons
3.5.2“Deuterium bottleneck”
3.5.3 Helium一4
3.5.4 Deuterium
3.5.5 The other light elements
3.6 Recombination
3.6.1 Helium recombination
3.6.2 Hydrogen recombination:equilibrium consideration
3.6.3 Hydrogen recombination:the kinetic approach
4 The very early universe
4.1 Basics
4.1.1 Local gauge invariance
4.1.2 Non—Abelian gauge theories
4.2 Quantum chromodynamics and quark-gluon plasma
4.2.1 Running coupling constant and asymptotic freedom
4.2.2 Cosmological quark-gluon phase transition
4.3 Electroweak theory
4.3.1 Fermion content
4.3.2“Spontaneous breaking”of U(1)symmetry
4.3.3 Gauge bosons
4.3.4 Fermion interactions
4.3.5 Fermion masses
4.3.6 CP violation
4.4 “Symmetry restoration”and phase transitions
4.4.1 Effective potential
4.4.2 U(l)model
4.4.3 Symmetry restoration at high temperature
4.4.4 Phase transitions
4.4.5 Electroweak phase transition
4.5 Instantons.sphalerons and the early universe
4.5.1 Particle escape from a potential well
4.5.2 Decay of the metastable vacuum
4.5.3 The vacuum structure of gauge theories
4.5.4 Chiral anomaly and nonconservation of the fermion number
4.6 Beyond the Standard Model
4.6.1 Dark matter candidates
4.6.2 Baryogenesis
4.6.3 Topological defects
5 Inflation I:homogeneous limit
5.1 Problem of initial conditions
5.2 Inflation:main idea
5.3 How can gravity become“repulsive”?
5.4 How to realize the equation of state P≈一#####
5.4.1 Simple example:V=m2#4#####
5.4.2 General potential:slow—roll approximation
5.5 Preheating and reheating
5.5.1 Elementary theory
5.5.2 Narrow resonance
5.5.3 Broad resonance
5.5.4 Implications
5.6 “Menu”of scenarios
Part II Inhomogeneous universe
6 Gravitational instability in Newtonian theory
6.1 Basic equations
6.2 Jeans theory
6.2.1 Adiabatic perturbations
6.2.2 Vector perturbations
6.2.3 Entropy perturbations
6.3 Instability in an expanding universe
6.3.1 Adiabatic perturbations
6.3.2 Vector perturbations
6.3.3 Self-similar solution
6.3.4 Cold matter in the presence of radiation or dark energy
6.4 Beyond linear approximation
6.4.1 Tolman solution
6.4.2 Zel’dovich solution
6.4.3 Cosmic web
7 Gravitational instability in General Relativity
7.1 Perturbations and gauge—invariant variables
7.1.1 Classification of perturbations
7.1.2 Gauge transformations and gauge—invariant variables
7.1.3 COOrdinate systems
7.2 Equations for cosmological perturbations
7.3 Hydrodynamical perturbations
7.3.1 Scalar perturbations
7.3.2 Vector and tensor perturbations
7.4 Baryon-radiation plasma and cold dark matter
7.4.1 Equations
7.4.2 Evolution of perturbations and transfer functions
8 Inflation II:origin of the primordial inhomogeneities
8.1 Characterizing perturbations
8.2 Perturbations on inflation(slow—roll approximation)
8.2.1 Inside the Hubble scale
8.2.2 The spectrum of generated perturbations
8.2.3 Why dO we need inflation?
8.3 Quantum cosmological perturbations
8.3.1 Equations
8.3.2 Classical solutions
8.3.3 Quantizing perturbations
8.4 Gravitationa waves from inflation
8.5 Self_reDroductiOn of the universe
8.6 Infation as a theory with predictive power
9 Cosmic microwave background anisotropies
9.1 Basics
9.2 Sachs-Wolfe eflfect
9.3 Initial conditions
9.4 Correlation function and multipoles
9.5 Anisotropies on large angular scales
9.6 Delayed recombination and the finite thickness effect
9.7 Anisotropies on small angular scales
9.7.1 Transfer functions
9.7.2 Multipole moments
9.7.3 Parameters
9.7.4 Calculating the spectrum
9.8 Determining cosmic parameters
9.9 Gravitational waves
9.10 Polarization of the cosmic microwave background
9.10.1 Polarization tensor
9.10.2 Thomson scattering and polarization
9.10.3 Delayed recombination and polarization
9.10.4 E and B polarization modes and correlation functions
9.1l Reionization
Bibliography
Expanding universe(Chapters 1 and 2)
Hot universe and nucleosvnthesis(Chapter 3)
Particle physics and early universe(Chapter 4)
Inflation (Chapters 5 and 8)
Gravitational instability(Chapters 6 and 7)
CMB fluctuations(Chapter 9)
lndex
3.1 Geometry of an homogeneous,isotropic space
1.3.2 The Einstein equations and cosmic evolution
1.3.3 Friedmann equations
1.3.4 Conformal time and relativistic solutions
1.3.5 Milne universe
1.3.6 De Sitter universe
2 Propagation of light and horizons
2.1 Light geodesics
2.2 Horizons
2.3 Conformal diagrams
2.4 Redshifl
2.4.1 Redshifl as a measure of time and distance
2.5 Kinematic tests
2.5.1 Angular diameter-redshift relation
2.5.2 Luminosity—redshifl relation
2.5.3 Number counts
2.5.4 Redshift evolution
3 The hot universe
3.1 The composition of the universe
3.2 Brief thermal history
3.3 Rudiments of thermodynamics
3.3.1 Maximal entropy state,thermal spectrum, conservation laws and chemical potentials
3.3.2 Energy density,pressure and the equation of state
3.3.3 Calculating integrals
3.3.4 Ultra—relativistic particles
3.3.5 Nonrelativistic particles
3.4 Lepton era
3.4.1 ChemicaI potentials
3.4.2 Neutrino decoupling and electrOn—pOsitrOn annihilation
3.5 NucleOsvnthesis
3.5.1 Freeze—OUt of neutrons
3.5.2“Deuterium bottleneck”
3.5.3 Helium一4
3.5.4 Deuterium
3.5.5 The other light elements
3.6 Recombination
3.6.1 Helium recombination
3.6.2 Hydrogen recombination:equilibrium consideration
3.6.3 Hydrogen recombination:the kinetic approach
4 The very early universe
4.1 Basics
4.1.1 Local gauge invariance
4.1.2 Non—Abelian gauge theories
4.2 Quantum chromodynamics and quark-gluon plasma
4.2.1 Running coupling constant and asymptotic freedom
4.2.2 Cosmological quark-gluon phase transition
4.3 Electroweak theory
4.3.1 Fermion content
4.3.2“Spontaneous breaking”of U(1)symmetry
4.3.3 Gauge bosons
4.3.4 Fermion interactions
4.3.5 Fermion masses
4.3.6 CP vi 经典英文物理教材系列:宇宙学的物理基础 [Physical Foundations of COSMOLOGY] 电子书 下载 mobi epub pdf txt
电子书下载地址:
相关电子书推荐:
- 文件名
- 初级篇-小手学涂色
- HIIT 高强度间歇训练法 [英]史蒂夫巴雷特(Steve Barrett)
- 羚牛的故事(绿野寻踪) 9787503888939 雍严格,孙晋强;蒲春举 摄影-RT
- BF:巴西柔术-BOOK+DVD (加) 德莱·飞利浦 (Drolet Philippe)
- BF-徽州地-中国地理百科-中国地理百科丛书编委会著 世界图书出版公司 978751008
- 正版 象棋高级杀法及其训练测试/象棋阶梯课堂系列 傅宝胜 9787533772109
- 探秘海洋生物(全彩版)/科学眼 (日) 原田雅章著
- 围棋阶梯培训教程:入门教程(零起点到8级) 9787111508168 机械工业出版社
- 古罗马:每天30秒探索恒久文明的50个伟大成就 科普读物 书籍
- 少年足球教学与训练 基础训练98项 11-12岁9787115467638 人民邮电出版社
- {RT}自然界的物质循环-《自然界的物质循环》编写组 世界图书出版公司 978751001
- 9787807428404 图文版 自然科学新导向丛书——文化的传播 百花洲文艺出版社
- 贪玩的人类——那些将我们带进科学的人 9787030271341 李建荣(老多)-RT
- 中国青少年皮划艇训练教学大纲
- 32cm地球仪-(语音)