Vineet Nayyar Learning Resource Centre

Dark Energy.

By: Contributor(s): Material type: TextTextSeries: eBooks on DemandPublication details: Singapore : World Scientific Publishing Company, 2012Description: 254ISSN:
  • 9789814619707
Subject(s): DDC classification:
  • 523.01 MIA
Online resources:
Contents:
Foreword; Preface; Contents; Part I Preliminaries in a Nutshell; 1 Gravitation; 1.1 The Curved Spacetime; 1.2 The Curved Spacetime: An Example; 1.3 The Einstein Equation; 2 Matter Components; 2.1 The Stress Tensor; 2.2 Perfect Fluid; 2.3 Observers and Energy Conditions; 2.4 The Vacuum; 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 The Theoretical Challenge; References; 5 Weinberg's Classification
5.1 Supersymmetry5.2 Anthropic Principle; 5.3 Tuning Mechanism; 5.4 Modifying Gravity; 5.5 Quantum Cosmology; References; 6 Symmetry; 6.1 Supersymmetry in 2 + 1 Dimensions; 6.2 't Hooft-Nobbenhuis Symmetry; 6.3 Kaplan-Sundrum Symmetry; 6.4 Symmetry of Reversing Sign of the Metric; 6.5 Scaling Invariance in D > 4; References; 7 Anthropic Principle; 7.1 Bousso-Polchinski 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 Self-Adjustment; References; 9 Modified Gravity
9.1 f(R) Models9.2 MOND and TeVeS Theories; 9.3 DGP Model; 9.4 Other Modified Gravity Theories; References; 10 Quantum 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 Back-Reaction; 12.1 Sub-Hubble Inhomogeneities; 12.2 Super-Hubble Inhomogeneities; References; 13 Phenomenological Models; 13.1 Quintessence, Phantom and Quintom
13.2 K-Essense, Custuton, Braiding and Ghost Condensation13.3 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 χ2 Analysis; 15.1.1 χ2 Function; 15.1.2 χ2 Analysis; 15.2 Algorithms for the Best-Fit Analysis; 15.2.1 The Gradient Descent Algorithm; 15.2.2 The Newton's Method; 15.2.3 The Random Walk Algorithm; 15.2.4 Summary; 15.3 The Markov Chain Monte Carlo Algorithm
15.3.1 The Metropolis Hastings Algorithm15.3.2 The CosmoMC Code; 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 Gamma-Ray Burst; 16.7 X-Ray 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 On-Going Projects; 17.2 Intermediate-Scale, Near-Future Projects; 17.3 Larger-Scale, Longer-Term Future Projects
References
Summary: This book introduces the current state of research on dark energy. It consists of three parts. The first part is for preliminary knowledge, including general relativity, modern cosmology, etc. The second part reviews major theoretical ideas and models of dark energy. The third part reviews some observational and numerical works. The aim of this book is to provide a sufficient level of understanding of dark energy problems, so that the reader can both get familiar with this area quickly and also be prepared to tackle the scientific literature on this subject. It will be useful for graduate stud
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Reference Reference Mahindra University VNLRC Reference Physics 523.01 MIA (Browse shelf(Opens below)) Not for loan 5026

Foreword; Preface; Contents; Part I Preliminaries in a Nutshell; 1 Gravitation; 1.1 The Curved Spacetime; 1.2 The Curved Spacetime: An Example; 1.3 The Einstein Equation; 2 Matter Components; 2.1 The Stress Tensor; 2.2 Perfect Fluid; 2.3 Observers and Energy Conditions; 2.4 The Vacuum; 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 The Theoretical Challenge; References; 5 Weinberg's Classification

5.1 Supersymmetry5.2 Anthropic Principle; 5.3 Tuning Mechanism; 5.4 Modifying Gravity; 5.5 Quantum Cosmology; References; 6 Symmetry; 6.1 Supersymmetry in 2 + 1 Dimensions; 6.2 't Hooft-Nobbenhuis Symmetry; 6.3 Kaplan-Sundrum Symmetry; 6.4 Symmetry of Reversing Sign of the Metric; 6.5 Scaling Invariance in D > 4; References; 7 Anthropic Principle; 7.1 Bousso-Polchinski 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 Self-Adjustment; References; 9 Modified Gravity

9.1 f(R) Models9.2 MOND and TeVeS Theories; 9.3 DGP Model; 9.4 Other Modified Gravity Theories; References; 10 Quantum 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 Back-Reaction; 12.1 Sub-Hubble Inhomogeneities; 12.2 Super-Hubble Inhomogeneities; References; 13 Phenomenological Models; 13.1 Quintessence, Phantom and Quintom

13.2 K-Essense, Custuton, Braiding and Ghost Condensation13.3 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 χ2 Analysis; 15.1.1 χ2 Function; 15.1.2 χ2 Analysis; 15.2 Algorithms for the Best-Fit Analysis; 15.2.1 The Gradient Descent Algorithm; 15.2.2 The Newton's Method; 15.2.3 The Random Walk Algorithm; 15.2.4 Summary; 15.3 The Markov Chain Monte Carlo Algorithm

15.3.1 The Metropolis Hastings Algorithm15.3.2 The CosmoMC Code; 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 Gamma-Ray Burst; 16.7 X-Ray 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 On-Going Projects; 17.2 Intermediate-Scale, Near-Future Projects; 17.3 Larger-Scale, Longer-Term Future Projects

References

This book introduces the current state of research on dark energy. It consists of three parts. The first part is for preliminary knowledge, including general relativity, modern cosmology, etc. The second part reviews major theoretical ideas and models of dark energy. The third part reviews some observational and numerical works. The aim of this book is to provide a sufficient level of understanding of dark energy problems, so that the reader can both get familiar with this area quickly and also be prepared to tackle the scientific literature on this subject. It will be useful for graduate stud

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