点击选择搜索分类
首页 - 历史- 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
- 我们应该吃肉吗?无肉不欢的世界 9787121309830 (加)VACLAV SMIL(
- 玩儿这本书
- 树的智慧 麦克斯·亚当斯 约翰·伊夫林 绘
- 画·大师 静物篇
- 科技发展五十年 波澜壮阔的史前世界
- 写实手绘彩铅插画技法精讲
- 经典物理三巨匠 松鹰著
- 名画之谜:希腊神话篇 中信出版社
- 生态文明新论/生态文明决策者X读丛书 卢风
- 画坛名师大讲堂:苏百钧讲工笔花鸟画(下 格局)
- 科学探索系列 大自然的礼物 关于空气和水的科学之旅 (法)勒内·莫罗著;王晓东
- 世界艺术巨匠 名画家全集外国艺术画册 油画书籍 毕沙罗绘画+西斯莱共2本 世界艺术巨匠
- 探秘贝加尔湖 畅销书籍 户外旅游 正版 毛国强
- 少有人走的路3(白金升级版):与心灵对话
- 皇帝新脑-推动系列