The FTIR spectra analysis of CO & CH chemical compound production of 15keV H3+ ion bombard on CO & CO2 & CH3OH ice mixed with H2O

碩士 === 國立中央大學 === 物理研究所 === 99 === There are many interstellar ices in the galaxy, and its main composition includes H2O, NH3, CH3OH, CH4, CO, CO2, etc. Under the low temperature (10K -100K), these molecules tend to attach to the surfaces of the interstellar particles or the meteorites, and then bec...

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Main Authors: Chiu Chen-Ning, 邱振寧
Other Authors: C.S. Lee
Format: Others
Language:zh-TW
Published: 2011
Online Access:http://ndltd.ncl.edu.tw/handle/78405595651824168186
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spelling ndltd-TW-099NCU051980052015-10-13T20:23:26Z http://ndltd.ncl.edu.tw/handle/78405595651824168186 The FTIR spectra analysis of CO & CH chemical compound production of 15keV H3+ ion bombard on CO & CO2 & CH3OH ice mixed with H2O 15KeV H3+離子撞擊含CO及CH鍵化合物與水不同比例之冰晶產生CO、CO2、CH3OH的FTIR光譜分析 Chiu Chen-Ning 邱振寧 碩士 國立中央大學 物理研究所 99 There are many interstellar ices in the galaxy, and its main composition includes H2O, NH3, CH3OH, CH4, CO, CO2, etc. Under the low temperature (10K -100K), these molecules tend to attach to the surfaces of the interstellar particles or the meteorites, and then become interstellar ice. Meanwhile, there are also many particles (with energy to some degree) that ejected by other stars in the universe, like the solar wind of the solar system. When bombarded with these energetic particles, the molecule structure of the interstellar ice could be changed and produce organic matters. Those interstellar ices on the surfaces of the meteorite, which had turned into organic matters, may fall on a planet with the meteorite, and bring the organic matters to that planet. This could make a significant change to the evolution of the planet, especially for the planet where the organic matters never exist before. The mechanism of the reaction that produces organic matter out of ice crystal is the main topic that we wanted to probe into in this essay. In our experiment, we utilized the cryogenic technique (24 K) and the ultra-high vacuum (6×10-10 torr) to simulate the environment of outer space. And we used H3+ ions (15keV) to bombard the chemical compounds (the ice crystal) with CH-bonds or CO-bonds. The chemical compounds, including CH4 and CO2, mixed with H2O in various proposition are the controlled variables in the experiment. Finally, we used FTIR to scan the ice crystal, both before and after the bombardment, and then analyze the quantity of the CO、 CO2 and CH3OH bonds produced under the different conditions. C.S. Lee 李敬萱 2011 學位論文 ; thesis 56 zh-TW
collection NDLTD
language zh-TW
format Others
sources NDLTD
description 碩士 === 國立中央大學 === 物理研究所 === 99 === There are many interstellar ices in the galaxy, and its main composition includes H2O, NH3, CH3OH, CH4, CO, CO2, etc. Under the low temperature (10K -100K), these molecules tend to attach to the surfaces of the interstellar particles or the meteorites, and then become interstellar ice. Meanwhile, there are also many particles (with energy to some degree) that ejected by other stars in the universe, like the solar wind of the solar system. When bombarded with these energetic particles, the molecule structure of the interstellar ice could be changed and produce organic matters. Those interstellar ices on the surfaces of the meteorite, which had turned into organic matters, may fall on a planet with the meteorite, and bring the organic matters to that planet. This could make a significant change to the evolution of the planet, especially for the planet where the organic matters never exist before. The mechanism of the reaction that produces organic matter out of ice crystal is the main topic that we wanted to probe into in this essay. In our experiment, we utilized the cryogenic technique (24 K) and the ultra-high vacuum (6×10-10 torr) to simulate the environment of outer space. And we used H3+ ions (15keV) to bombard the chemical compounds (the ice crystal) with CH-bonds or CO-bonds. The chemical compounds, including CH4 and CO2, mixed with H2O in various proposition are the controlled variables in the experiment. Finally, we used FTIR to scan the ice crystal, both before and after the bombardment, and then analyze the quantity of the CO、 CO2 and CH3OH bonds produced under the different conditions.
author2 C.S. Lee
author_facet C.S. Lee
Chiu Chen-Ning
邱振寧
author Chiu Chen-Ning
邱振寧
spellingShingle Chiu Chen-Ning
邱振寧
The FTIR spectra analysis of CO & CH chemical compound production of 15keV H3+ ion bombard on CO & CO2 & CH3OH ice mixed with H2O
author_sort Chiu Chen-Ning
title The FTIR spectra analysis of CO & CH chemical compound production of 15keV H3+ ion bombard on CO & CO2 & CH3OH ice mixed with H2O
title_short The FTIR spectra analysis of CO & CH chemical compound production of 15keV H3+ ion bombard on CO & CO2 & CH3OH ice mixed with H2O
title_full The FTIR spectra analysis of CO & CH chemical compound production of 15keV H3+ ion bombard on CO & CO2 & CH3OH ice mixed with H2O
title_fullStr The FTIR spectra analysis of CO & CH chemical compound production of 15keV H3+ ion bombard on CO & CO2 & CH3OH ice mixed with H2O
title_full_unstemmed The FTIR spectra analysis of CO & CH chemical compound production of 15keV H3+ ion bombard on CO & CO2 & CH3OH ice mixed with H2O
title_sort ftir spectra analysis of co & ch chemical compound production of 15kev h3+ ion bombard on co & co2 & ch3oh ice mixed with h2o
publishDate 2011
url http://ndltd.ncl.edu.tw/handle/78405595651824168186
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