醉染图书Dark Energy(暗能量)9787301210383

Part I Preliminaries in a Nutshell
1 Gravitation．
1．1 The Curved Spacetime
1．2 The Curved Spacetime：an Example
1．3 TheEinstein Equation
2 Matter Components
2. 1 The StressTensor
2．2 Perfect Fluid
. Observers and Energy Conditions
2．4 TheVacuum
2．5 Particles．
2．6 Homogeneous Field Configurations
3 Cosmology
3．1 The Cosmological Principle
3．2 Newtonian Cosmology
3．3 FRW Cosmology
Part II Theoretical Aspects
4 Introduction to Dark Energy
4．1 The Cosmological Constant Reloaded
4．2 TheTheoretical ChallengeReferences
5 Weinbergs Classification
5.1 Supersymmetry
5.2 Anthropic Principle
5.3 Tuning Mechanism
5.4 Modifying Gravity
5.5 ntum Cosmology
References
6 Symmetry
6.1 Supersymmetry in 21 Dimensions
6.2 t HooftNobhenhuis Symmetry
6.3 KaplanSunu Symmetry
6.4 Symmetry of Reversing Sign of the Metric
6.5 Sealing Invariance in D > 4
References
7 Anthropic Principle
7.1 BoussoPolchinski Scenario
7.2 KKLT Scenario
7.3 Populating the Landscape and Anthropic Interpretations.
References
8 Tuning Mechanisms
8.1 Brane versus Bulk Mechanism
8.2 Black Hole SelfAdjustment
References
9 Modified Gravity
9.1 f(R) Models
9.2 MOND and TeVeS Theories
9.3 DGP Model
9.4 Other Modified Gravity Theories
References
10 ntum Cosmology
10.1 Cosmological Constant Seesaw
10.2 Wave Function through the Landscape
References
11 Holographic Principle
11.1 The Holographic Principle
11.2 Holographic Dark Energy
11.3 Complementary Motivations
11.4 Agegraphic Dark Energy
11.5 Ricci Dark Energy
References
12 cRaction
12.1 SubHubble Inhomogeneities
12.2 SuperHubble Inhomogeneities
References
13 Phenomenological Models
13.1 intessence, Phantom and intom
13.2 KEssense, Custuton, Braiding and Ghost Condensation
13.3 Higher Spin Fields
13.4 Chaplygin Gas and Viscous Fluid
13.5 Particle Physics Models
13.6 Dark Energy Perturbations
References
14 The Theoretical Challenge Revisited
References
Part III Observational Aspects
15 Basis of Statistics
15.1 X2 Analysis
15.2 Algorithms for the BestFit Analysis
15.3 The Markov Chain Monte Carlo Algorithm
15.4 The Fisher Matrix Techniques
References
16 Cosmic Probes of Dark Energy
16.1 Type Ia Supernovae
16.2 Cosmic Microwave Background
16.3 Baryon Acoustic Oscillations
16.4 Weak Lensing
16.5 Galaxy Clusters
16.6 GammaPay Burst
16.7 XRay Observations
16.8 Hubble Parameter Measurements
16.9 Cosmic Age Tests
16.10 Growth Factor
16.11 Other Cosmological Probes
References
17 Dark Energy Projects
17.1 OnGoing Projects
17.2 IntermediateScale, NearFuture Projects
17.3 LargerScale, LongerTerm Future Projects
References
18 Observational Constraints on Specific Theoretical Models
18.1 Scalar Field Models
18.2 Chaplygin Gas Models
18.3 Holographic Dark Energy Models
18.4 DvaliGabadadzePorrati Model
18.5 f(R) Models
18.6 Other Modified Gravity Models
18.7 Inhomogeneous LTB and cRartion Models
18.8 Comparison of Dark Energy Models
References
19 Dark Energy Reconstructions from Observational Data
19.1 Specific Ansatz
19.2 Binned Parametrization
19.3 Polynomial Fitting
19.4 Gaussian Process Modeling
References
Index

李淼，1990年于丹麦哥本哈根大学玻尔研究所获博士，研究量子场论、超弦理论以及宇宙学。先后在美国加州大学圣巴巴拉分校、布朗大学以及芝加哥大学做博士后研究员和研究理教授。1999年回国，是杰出人才入选者、委杰出青年获得者、新世纪百千万人工程入选者，曾任台湾大学客座教授。现为理论物理研究所研究员、交叉学科理论研究中心成员、中国科学技术大学客座教授。在超弦理论中的研究有一定的国际影响，特别是二维刘维尔理论、D膜以及黑洞的量子物理。近致力于研究超弦中的黑洞物理、超弦宇宙学以及暗能量。