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Constraining dark energy models with cosmic microwave background data =: 微波背景幅射數據對暗能量模型的規範. / 微波背景幅射數據對暗能量模型的規範 / Constraining dark energy models with cosmic microwave background data =: Wei bo bei jing fu she shu ju dui an neng liang mo xing de gui fan. / Wei bo bei jing fu she shu ju dui an neng liang mo xing de gui fan

Chan, Wing Hang. / Thesis (M.Phil.)--Chinese University of Hong Kong, 2008. / Includes bibliographical references (leaves 76-78). / Abstracts in English and Chinese. / Chan, Wing Hang. / Chapter 1 --- Review of Cosmology --- p.1 / Chapter 1.1 --- Background Evolution of Universe --- p.1 / Chapter 1.1.1 --- The Cosmological Principle --- p.1 / Chapter 1.1.2 --- The Non-static Universe --- p.3 / Chapter 1.1.3 --- Robertson-Walker metric --- p.3 / Chapter 1.1.4 --- Scale Factor and Cosmological Redshift --- p.3 / Chapter 1.1.5 --- Hubble Constant --- p.4 / Chapter 1.1.6 --- The Einstein Field Equations --- p.4 / Chapter 1.1.7 --- The Cosmological Constant --- p.6 / Chapter 1.1.8 --- Time Evolution --- p.6 / Chapter 1.1.9 --- Continuity Equation --- p.7 / Chapter 1.1.10 --- Conformal Distance --- p.8 / Chapter 1.2 --- Observational Data --- p.8 / Chapter 1.2.1 --- Type Ia Supernovae --- p.9 / Chapter 1.2.2 --- Cosmic Microwave Background --- p.9 / Chapter 2 --- Review of Dark Energy Models --- p.11 / Chapter 2.1 --- The Cosmological Constant --- p.11 / Chapter 2.2 --- Quintessence --- p.11 / Chapter 2.3 --- Extra Dimension Models --- p.12 / Chapter 2.3.1 --- Kaluza-Klein --- p.12 / Chapter 2.3.2 --- Generalized Homogeneous and Isotropic Extra Dimensions --- p.12 / Chapter 3 --- Review of CMB and Type Ia Supernovae --- p.17 / Chapter 3.1 --- Type Ia Supernovae --- p.17 / Chapter 3.1.1 --- Comparison of cosmological models with recent SNIa data --- p.18 / Chapter 3.2 --- Cosmic Microwave Background Radiation --- p.18 / Chapter 3.2.1 --- Power Spectrum of CMBA --- p.18 / Chapter 3.2.2 --- Photon Baryon Oscillation --- p.21 / Chapter 3.2.3 --- Acoustic Peaks --- p.23 / Chapter 3.2.4 --- Matter Perturbation --- p.24 / Chapter 3.2.5 --- Baryon Loading --- p.24 / Chapter 3.2.6 --- Photons Driving --- p.25 / Chapter 3.2.7 --- Initial Conditions --- p.25 / Chapter 3.2.8 --- Reionization --- p.26 / Chapter 3.2.9 --- The Vanilla ACDM Model --- p.26 / Chapter 3.2.10 --- Summary of CMBA --- p.26 / Chapter 4 --- Constraining Dark Energy Models --- p.27 / Chapter 4.1 --- Constraining Dark Energy Density Using SN Ia data --- p.27 / Chapter 4.1.1 --- Direct Calculation of Dark Energy Density --- p.27 / Chapter 4.2 --- Constraining Dark Energy Density Using CMB data --- p.31 / Chapter 4.2.1 --- Dark Energy Evolution for time varying EOS --- p.31 / Chapter 4.2.2 --- Dark Energy Density Perturbation --- p.32 / Chapter 4.2.3 --- Parameterization of Time Varying Dark Energy --- p.32 / Chapter 4.2.4 --- Effect of Dark Energy Density on CMBA power spectrum --- p.33 / Chapter 4.2.5 --- Limitations and Difficulties Constraining Dark Energy Equation of State --- p.41 / Chapter 4.2.6 --- Constraining the Evolution of Dark Energy Density with a polynomial model --- p.54 / Chapter 4.2.7 --- Constraining Evolution of Dark Energy Density with Gaussian-type EOS --- p.59 / Chapter 4.2.8 --- Constraining Evolution of Dark Energy Step Function EOS with CMB Acoustic Peaks --- p.66 / Chapter 5 --- Summary --- p.73 / Bibliography --- p.76

Identiferoai:union.ndltd.org:cuhk.edu.hk/oai:cuhk-dr:cuhk_326551
Date January 2008
ContributorsChan, Wing Hang., Chinese University of Hong Kong Graduate School. Division of Physics.
Source SetsThe Chinese University of Hong Kong
LanguageEnglish, Chinese
Detected LanguageEnglish
TypeText, bibliography
Formatprint, xiv, 78 leaves : ill. ; 30 cm.
RightsUse of this resource is governed by the terms and conditions of the Creative Commons “Attribution-NonCommercial-NoDerivatives 4.0 International” License (http://creativecommons.org/licenses/by-nc-nd/4.0/)

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