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作者(中文):詹政勳
作者(外文):Chan, Chen Hsun
論文名稱(中文):太陽與超新星微中子的暗物質米赫耶夫-斯米爾夫-沃芬斯坦效應
論文名稱(外文):Dark Matter Induced Mikheyev-Smirnov-Wolfenstain Effect in The Sun And Core-Collapse Supernovae
指導教授(中文):張維甫
指導教授(外文):Chang, We Fu
口試委員(中文):徐百嫻
張敬民
口試委員(外文):Hsu, Pai Hsien
Cheung, Kingman
學位類別:碩士
校院名稱:國立清華大學
系所名稱:物理系
學號:102022544
出版年(民國):104
畢業學年度:103
語文別:英文
論文頁數:64
中文關鍵詞:微中子MSW效應暗物質太陽微中子超新星
外文關鍵詞:neutrino oscillationMSW effectdark matterasymmetric dark mattersolar neutrino problemcore-collapse supernova
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我們計算了在太陽與超新星微中子受到暗物質的米赫耶夫-斯米爾夫-沃芬斯坦效應。然而,若暗物質不會自我湮滅,例如,不對稱暗物質,才會有足夠大的效應。從太陽微中子觀測實驗的數據,在暗物質質量小於四十百萬電子伏特的範圍,我們得到一個很強的對於微中子與暗物質之間作用力大小的限制條件。在核塌陷超新星中,我們發現只有在超新星的位置很靠近銀河系中心或暗物質與微中子作用力夠強才有機會偵測到這個額外的效應。
We studied the dark matter induced Mikheyev-Smirnov-Wolfenstein e ect on neutrino oscillations in the Sun and the core-collapse supernovae. However, to have sizable e ect, we found that the dark matter cannot self-annihilate, for instance, the asymmetric dark matter. From the solar neutrino data, we found strong constraint on the interaction between dark matter and neutrino for asymmetric dark matter with mass less than 40 GeV. For supernovae, we found that the additional e ect would be detectable only if the supernova sits close to the Galactic center or the interaction between dark matter and neutrinos is strong enough.
Contents i
List of Tables iii
List of Figures vi
1 Introduction 1
2 Brief Review on Neutrino Oscillation 3
2.1 Neutrino Mass, Mixing, And PMNS Matrix . . . . . . . . . . . . . 3
2.2 Neutrino Oscillations in Vacuum.................... 4
2.3 Matter effect on neutrino oscillations ................. 6
2.3.1 Oscillations of solar neutrinos ................. 8
2.4 Experiments and Measurements.................... 9
2.4.1 Solar neutrino oscillations ................... 10
2.4.2 Atmospheric neutrino experiment ............... 11
2.4.3 Experiments of reactor..................... 11
2.4.4 Accelerator neutrino ...................... 11
2.4.5 Short summary ......................... 12
3 MSW Effect on Solar Neutrinos Through Accumulated Dark Matter 14
3.1 MSW Effect of Electrons........................ 14
3.2 Accumulation of Dark Matter in the Sun . . . . . . . . . . . . . . . 15
3.3 Distribution of Accumulated Dark Matter . . . . . . . . . . . . . . 20
3.4 Dark matter MSW Effect in the Sun ................. 21
4 MSW Effect on Neutrino Oscillations in Core-collapse Supernovae 30
4.1 Core-collapse Supernovae........................ 30
4.1.1 Sn1987A............................. 34
4.2 Accumulation of Dark Matter in Core-collapse Supernovae . . . . . 35
4.3 Dark Matter Density Distribution................... 38
4.4 Additional MSW Effect with DarkMatter . . . . . . . . . . . . . . 38
4.4.1 MSW effect of electron only .................. 41
4.4.2 Additional MSW effect of DM................. 44
5 Summary and Conclusion..............48
Reference.........49
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