無R超對稱標準模型中輕子的輻射衰變

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陳建溢(Chien-Yi Chen) 查詢紙本館藏

畢業系所

物理學系

論文名稱

無R超對稱標準模型中輕子的輻射衰變
(Leptonic Radiative decay inSupersymmetry without R-parity)

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摘要(中)

我們在無R超對稱標準模型中利用數值方法計算 one loop Feynman圖對 μ and τ 的輻射衰變，即 μ → eγ ，τ → eγ ，和 τ → μγ 的貢獻，並對結果做定性的分析。在目前實驗數據的限制下，R 宇稱破缺參數空間的允許範圍已經可以藉由數值上的計算精確地得到。
Ref.[7] 也曾做過類似的研究，但因為其在計算中對 mass eigenstate couplings 做近似，所以得到的結果並不完全精確。本論文則利用精確的mass eigenstate couplings 來做計算，並對兩者的結果加以比較。我們發現在μ*B 的參數空間中，兩者所得到的結果有明顯的差異。

摘要(英)

We present a detail analysis together with exact numerical calculations on one loop contributions
to the branching ratio of the radiative decay of μ and τ , namely μ → e γ, τ → e γ,
and τ → μγ from supersymmtry without R-parity. An exact numerical study is performed
to obtain explicit bounds on the parameters under the present experimental limit. A similar
work has been performed in the Ref.[7], which used electroweak states as an approximation
to the physical particles for the external legs to the loop. However, we use the formula
for exact mass eigenstate couplings to calculate the one loop diagrams. We compare the
results obtained by using these two approaches in the R-parity violating parameter spaces
and discover that they have a sizable difference in the resulted constraints on some μ*B
combinations.

關鍵字(中)

★ 超對稱

關鍵字(英)

★ supersymmetry
★ R-parity
★ leptonic radiative decay

論文目次

1 Introduction ...........................................................1
2 Generic Supersymmetric Standard Model ..................................4
2.1 Notes on the scalar potential . . . . . . . . . . . . . . . . . . . . 6
2.2 Charged fermions . . . . . . . . . . . . . . . . . . . . . . . . . . 8
2.3 Neutral fermions . . . . . . . . . . . . . . . . . . . . . . . . . . 10
2.4 The neutral scalars . . . . . . . . . . . . . . . . .. . . . . . . . 12
2.5 The charged scalars . . . . . . . . . . . . . . . .... . . . . . . . 16
3 Leptonic Radiative Decay ..............................................19
3.1 ”Standard Model Results” . . . . . . . . . . . . . . . . . . . . . 19
3.2 Charged scalar-neutral lepton vertices . . . . . . . . . . . . . . . 20
3.3 Neutral scalar-charged lepton vertices . . . . . . . . ..... . . . . 22
3.4 The decay amplitude . . . . . . . . . . . . . ........ . . . . . . . 23
4 Numerical Results and Discussions..................................... 26
4.1 Combinations without new contributions . . . . . . . . . ..... . . . 26
4.2 The mu^*-lambda or mu-lambda^* contributions . . . . . . . . . . . . 27
4.3 The B^*-mu or B-mu^* contributions . . . . . . . . . . . . . . . . 29
4.4 Parameter variations . . . . . . . . . . . . . . . . . . . . . . . . 31
5 Conclusion ............................................................42
Bibliography.............................................................43

參考文獻

[1] B. Aubert et al. [BABAR Collaboration], “Search for lepton flavor violation in the decay
tau → mu gamma,” Phys. Rev. Lett. 95, 041802 (2005) [arXiv:hep-ex/0502032].
[2] B. Aubert et al. [BABAR Collaboration], “Search for lepton flavor violation in the decay
tau+- → e+- gamma,” Phys. Rev. Lett. 96, 041801 (2006) [arXiv:hep-ex/0508012].
[3] M. L. Brooks et al. [MEGA Collaboration], “New limit for the family-number nonconserving
decay mu+ → e+ gamma,” Phys. Rev. Lett. 83, 1521 (1999) [arXiv:hepex/
9905013].
[4] M. Bisset, O. C. W. Kong, C. Macesanu and L. H. Orr, Phys. Lett. B 430, 274 (1998)
[arXiv:hep-ph/9804282].
[5] M. Bisset, O. C. W. Kong, C. Macesanu and L. H. Orr, Phys. Rev. D 62, 035001 (2000)
[arXiv:hep-ph/9811498].
[6] O. C. W. Kong, Int. J. Mod. Phys. A 19, 1863 (2004) [arXiv:hep-ph/0205205].
[7] K. m. Cheung and O. C. W. Kong, Phys. Rev. D 64, 095007 (2001) [arXiv:hepph/
0101347].
[8] S. Eidelman et al. [Particle Data Group], Phys. Lett. B 592, 1 (2004).
[9] L. E. Ibanez and G. G. Ross, Nucl. Phys. B 368, 3 (1992).
[10] There has been some possible indication from the recent result for the muon anomalous
magnetic moment. See, for examples, J. Feng and K. Matchev, Phys. Rev. Lett. 86, 3480
(2001); U. Chattopadhyay and P. Nath, ibid. 86, 5854 (2001); K. Cheung, C.-H. Chou,
and O.C.W. Kong, Phys. Rev. D 64 , 111301(R) (2001). Also, some updated reviews
43
from talks by P. Nath and by K. Hagiwara given at NCTS workshop on Supersymmetry,
Chung-li, Taiwan.
[11] O.C.W. Kong, JHEP 0009, 037 (2000).
[12] SNO Collaboration, B. Aharmim et al., Phys. Rev. C 72, 055502 (2005) [arXiv:nuclex/
0502021]; Super-Kamiokande Collaboration, Y. Ashie et al., Phys. Rev. D 71,
112005 (2005) [arXiv:hep-ex/0501064]. GNO Collaboration, M. Altmann et al. Phys.
Lett. B 616, 174 (2005) [arXiv:hep-ex/0504037]. KamLAND Collaboration, T. Araki
et al. Phys. Rev. Lett. 94, 081801 (2005) [arXiv:hep-ex/0406035]. K2K Collaboration,
E. Aliu et al. Phys. Rev. Lett. 94, 081802 (2005) [arXiv:hep-ex/0411038]. MACRO
Collaboration, M. Ambrosio et al. Eur. Phys. J. C 36, 323 (2004). Soudan 2 Collaboration,
M. C. Sanchez et al. Phys. Rev. D 68, 113004 (2003) [arXiv:hep-ex/0307069].
CHOOZ Collaboraton, M. Apollonio et al., Eur. Phys. J. C 27, 331 (2003) [arXiv:hepex/
0301017].
[13] O. C. W. Kong and R. D. Vaidya, Phys. Rev. D 71, 055003 (2005) [arXiv:hepph/
0403148].
[14] J. Hisano, T. Moroi, K. Tobe and M. Yamaguchi, Phys. Rev. D 53, 2442 (1996)
[arXiv:hep-ph/9510309].

指導教授

江祖永(Otto C. W. Kong)

審核日期

2006-7-21

推文