Chan Man Ho = 中微子星的形成與特徵 / 陳文豪. / Thesis (M.Phil.)--Chinese University of Hong Kong, 2004. / Includes bibliographical references (leaves 84-87). / Text in English; abstracts in English and Chinese. / Chan Man Ho = Zhong wei zi xing de xing cheng yu te zheng / Chen Wenhao. / Chapter 1 --- Introduction --- p.1 / Chapter 1.1 --- History of dark matter research --- p.1 / Chapter 1.2 --- Method of searching for dark matter --- p.3 / Chapter 1.2.1 --- Observation of dark matter --- p.3 / Chapter 1.2.2 --- N-body simulation --- p.4 / Chapter 1.3 --- Candidates of dark matter --- p.7 / Chapter 1.3.1 --- Properties of neutrinos --- p.8 / Chapter 1.3.2 --- Neutrino oscillation --- p.9 / Chapter 1.3.3 --- Decay of neutrinos --- p.10 / Chapter 1.4 --- Origin of neutrino dark matter --- p.11 / Chapter 2 --- Properties of Neutrino Stars --- p.16 / Chapter 2.1 --- Hydrostatic Equilibrium --- p.16 / Chapter 2.2 --- Ultra-relativistic degenerate neutrino star --- p.17 / Chapter 2.2.1 --- Trajectory inside an ultra-relativistic neutrino star --- p.19 / Chapter 2.2.2 --- Rotation curve of an ultra-relativistic neutrino star --- p.20 / Chapter 2.3 --- Non-relativistic neutrino star --- p.21 / Chapter 2.3.1 --- Trajectories inside a non-relativistic neutrino star --- p.22 / Chapter 2.3.2 --- Rotation curve of non-relativistic neutrino stars --- p.24 / Chapter 2.4 --- Neutrino Mixing correction --- p.24 / Chapter 3 --- Neutrino star in galaxy --- p.26 / Chapter 3.1 --- Neutrino star in galactic center --- p.26 / Chapter 3.1.1 --- The rate of change of mass of neutrino star --- p.27 / Chapter 3.1.2 --- Motion inside the neutrino star in milky way --- p.27 / Chapter 3.2 --- Neutrino star in Milky Way --- p.30 / Chapter 3.2.1 --- Components of Milky Way --- p.32 / Chapter 3.2.2 --- Dark matter component in Milky Way --- p.33 / Chapter 4 --- Hot gas and Neutrino star in cluster --- p.40 / Chapter 4.1 --- Neutrino dark matter model --- p.41 / Chapter 4.1.1 --- Cowsik and McClelland model --- p.41 / Chapter 4.1.2 --- Treumann et al. model --- p.42 / Chapter 4.2 --- NFW universal dark matter profile --- p.43 / Chapter 4.3 --- Probing dark matter distribution --- p.44 / Chapter 4.4 --- Neutrino stars in clusters --- p.48 / Chapter 4.5 --- Heat source of hot gas --- p.52 / Chapter 4.5.1 --- Infall and compressional heating --- p.53 / Chapter 4.5.2 --- Heating by ejection from galaxies --- p.53 / Chapter 4.5.3 --- Heating by galaxy motion --- p.54 / Chapter 4.5.4 --- Heating by relativistic electrons --- p.55 / Chapter 4.5.5 --- Heating by photons from neutrino decay --- p.55 / Chapter 5 --- Formation of neutrino star --- p.58 / Chapter 5.1 --- Hydrodynamic code --- p.58 / Chapter 5.2 --- Hydrodynamic evolution of neutrino star --- p.61 / Chapter 5.2.1 --- Result of the simulation --- p.61 / Chapter 5.2.2 --- Scaling law of neutrino star formation --- p.66 / Chapter 5.2.3 --- Oscillation in neutrino star --- p.67 / Chapter 5.3 --- Expected Observational Results --- p.69 / Chapter 6 --- Discussion and conclusion --- p.72 / Chapter 6.1 --- Conclusion --- p.72 / Chapter 6.2 --- discussion --- p.74 / Chapter A --- Derivation of TOV equation --- p.76 / Chapter B --- Equation of state of degenerate ideal gas --- p.80 / Chapter C --- Derivation of oscillation period --- p.82 / Bibliography --- p.84
| Identifer | oai:union.ndltd.org:cuhk.edu.hk/oai:cuhk-dr:cuhk_324597 |
| Date | January 2004 |
| Contributors | Chan, Man Ho., Chinese University of Hong Kong Graduate School. Division of Physics. |
| Source Sets | The Chinese University of Hong Kong |
| Language | English, Chinese |
| Detected Language | English |
| Type | Text, bibliography |
| Format | print, vi, 87 leaves : ill. ; 30 cm. |
| Rights | Use 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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