Sign of φ-ω Mixing and the OZI Rule

碩士 === 國立臺灣大學 === 物理學系 === 85 === We try to understand the dynamical origin of OZI violation. The earlier works including gluonic annihilation and meson rescattering pictures are reviewed. With the rising value of the vector glueball(O) mas...

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Main Authors: Ko, Cheng-Ying, 柯澄瑛
Other Authors: Hou Wei-Shu
Format: Others
Language:zh-TW
Published: 1997
Online Access:http://ndltd.ncl.edu.tw/handle/46525501588047294921
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spelling ndltd-TW-085NTU001980182016-07-01T04:15:35Z http://ndltd.ncl.edu.tw/handle/46525501588047294921 Sign of φ-ω Mixing and the OZI Rule φ-ω介子混合的符號與OZI法則 Ko, Cheng-Ying 柯澄瑛 碩士 國立臺灣大學 物理學系 85 We try to understand the dynamical origin of OZI violation. The earlier works including gluonic annihilation and meson rescattering pictures are reviewed. With the rising value of the vector glueball(O) mass, we find that a new viewpoint could be taken: the smallness of $\phi-\omega$ mixing is related to the heaviness of O! A difficulty arises with the sign of the $\phi- \omega$ mixing fromthis model when comparing to experiments. This is solved by redefining the $\phi_0$ state from $s\bar s \rightarrow-s\bar s$ and modifying the mass matrix. We find that Nature chooses this relative sign of $-s\bar s$ for $\phi$ as compared to$\omega\cong(u\bar u+d\bar d)/\sqrt{2}$, if the O dominance pictureis correct. There is a leftover problem with $\rho-\omega$ mass difference, but no other mechanism seems to give any appropriate solution. Perhaps it could be explained by tuning of meson rescattering. Hou Wei-Shu 侯維恕 1997 學位論文 ; thesis 39 zh-TW
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language zh-TW
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description 碩士 === 國立臺灣大學 === 物理學系 === 85 === We try to understand the dynamical origin of OZI violation. The earlier works including gluonic annihilation and meson rescattering pictures are reviewed. With the rising value of the vector glueball(O) mass, we find that a new viewpoint could be taken: the smallness of $\phi-\omega$ mixing is related to the heaviness of O! A difficulty arises with the sign of the $\phi- \omega$ mixing fromthis model when comparing to experiments. This is solved by redefining the $\phi_0$ state from $s\bar s \rightarrow-s\bar s$ and modifying the mass matrix. We find that Nature chooses this relative sign of $-s\bar s$ for $\phi$ as compared to$\omega\cong(u\bar u+d\bar d)/\sqrt{2}$, if the O dominance pictureis correct. There is a leftover problem with $\rho-\omega$ mass difference, but no other mechanism seems to give any appropriate solution. Perhaps it could be explained by tuning of meson rescattering.
author2 Hou Wei-Shu
author_facet Hou Wei-Shu
Ko, Cheng-Ying
柯澄瑛
author Ko, Cheng-Ying
柯澄瑛
spellingShingle Ko, Cheng-Ying
柯澄瑛
Sign of φ-ω Mixing and the OZI Rule
author_sort Ko, Cheng-Ying
title Sign of φ-ω Mixing and the OZI Rule
title_short Sign of φ-ω Mixing and the OZI Rule
title_full Sign of φ-ω Mixing and the OZI Rule
title_fullStr Sign of φ-ω Mixing and the OZI Rule
title_full_unstemmed Sign of φ-ω Mixing and the OZI Rule
title_sort sign of φ-ω mixing and the ozi rule
publishDate 1997
url http://ndltd.ncl.edu.tw/handle/46525501588047294921
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AT kēchéngyīng phōjièzihùnhédefúhàoyǔozifǎzé
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