MEASURING THE MASS DISTRIBUTION OF DARK MATTER WITHIN GALAXY CLUSTERSTHROUGH WEAK GRAVITATIONAL LENSING

MEASURING THE MASS DISTRIBUTION OF DARK MATTER WITHIN GALAXY CLUSTERSTHROUGH WEAK GRAVITATIONAL LENSING

碩士 === 國立臺灣大學 === 物理研究所 === 96 === For the light rays are deflected by dark matter engendering the gravitational lensing effect in the universe, the galaxies become deformed as we observe. Utilizing the measure of distortion, the variation of its ellipticity, is capable to estimate the mass of dark...

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Main Authors: Hung-Hsu Chan, 詹弘旭
Other Authors: Tzihong Chiueh
Format: Others
Language:en_US
Published: 2008
Online Access:http://ndltd.ncl.edu.tw/handle/55326676758600899845
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spelling ndltd-TW-096NTU051980712015-11-25T04:04:37Z http://ndltd.ncl.edu.tw/handle/55326676758600899845 MEASURING THE MASS DISTRIBUTION OF DARK MATTER WITHIN GALAXY CLUSTERSTHROUGH WEAK GRAVITATIONAL LENSING 利用弱重力透鏡效應測量星系團內暗物質的質量分佈 Hung-Hsu Chan 詹弘旭 碩士 國立臺灣大學 物理研究所 96 For the light rays are deflected by dark matter engendering the gravitational lensing effect in the universe, the galaxies become deformed as we observe. Utilizing the measure of distortion, the variation of its ellipticity, is capable to estimate the mass of dark matter clusters. In this work, we investigate the accuracy of halo mass measurement through weak gravitational lensing, and the lower bound of mass detection on the sky survey. Tzihong Chiueh 闕志鴻 2008 學位論文 ; thesis 27 en_US
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description 碩士 === 國立臺灣大學 === 物理研究所 === 96 === For the light rays are deflected by dark matter engendering the gravitational lensing effect in the universe, the galaxies become deformed as we observe. Utilizing the measure of distortion, the variation of its ellipticity, is capable to estimate the mass of dark matter clusters. In this work, we investigate the accuracy of halo mass measurement through weak gravitational lensing, and the lower bound of mass detection on the sky survey.
author2 Tzihong Chiueh
author_facet Tzihong Chiueh
Hung-Hsu Chan
詹弘旭
author Hung-Hsu Chan
詹弘旭
spellingShingle Hung-Hsu Chan
詹弘旭
MEASURING THE MASS DISTRIBUTION OF DARK MATTER WITHIN GALAXY CLUSTERSTHROUGH WEAK GRAVITATIONAL LENSING
author_sort Hung-Hsu Chan
title MEASURING THE MASS DISTRIBUTION OF DARK MATTER WITHIN GALAXY CLUSTERSTHROUGH WEAK GRAVITATIONAL LENSING
title_short MEASURING THE MASS DISTRIBUTION OF DARK MATTER WITHIN GALAXY CLUSTERSTHROUGH WEAK GRAVITATIONAL LENSING
title_full MEASURING THE MASS DISTRIBUTION OF DARK MATTER WITHIN GALAXY CLUSTERSTHROUGH WEAK GRAVITATIONAL LENSING
title_fullStr MEASURING THE MASS DISTRIBUTION OF DARK MATTER WITHIN GALAXY CLUSTERSTHROUGH WEAK GRAVITATIONAL LENSING
title_full_unstemmed MEASURING THE MASS DISTRIBUTION OF DARK MATTER WITHIN GALAXY CLUSTERSTHROUGH WEAK GRAVITATIONAL LENSING
title_sort measuring the mass distribution of dark matter within galaxy clustersthrough weak gravitational lensing
publishDate 2008
url http://ndltd.ncl.edu.tw/handle/55326676758600899845
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