在$B \rightarrow D^{(*)}\tau\nu_{\tau}$衰变中寻找对带电标量更敏感的可观测物。

Q2 Physics and Astronomy Letters in High Energy Physics Pub Date : 2017-03-31 DOI:10.31526/LHEP.2.2019.108
L. Dhargyal
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引用次数: 0

摘要

众所周知,$B \rightarrow D^{(*)} \tau \nu_{\tau}$是寻找带电希格斯粒子的良好观测对象。最近Babar、Belle和LHCb在$R(D^{(*)})$观测到的与标准模型偏差近4 $\sigma$,重新唤起了人们对这些模式中带电希格斯粒子存在的可能信号的兴趣。但是如此大的速率偏差,标准模型有树水平的贡献,仅仅来自带电的希格斯粒子是极不可能的。然而,如果我们能够在这些模式中构建敏感的可观测物,这些衰变模式是寻找小荷电希格斯信号的良好探针。在这项工作中,我们想提出四个新的观测值,它们对带电希格斯粒子的存在比通常的观测值(如$A_{\lambda}^{D^{(*)}}$和$A_{\theta}^{D^{(*)}}$)更敏感。这四个可观测值是(1)$\frac{1}{A_{\lambda}^{D}}$, (2) $Y_{1}(q^{2}) = \frac{A^{D}_{\theta}}{A^{D}_{\lambda}}$, (3) $Y_{2}(q^{2}) = \frac{d\Gamma(B \rightarrow D^{*}\tau\nu_{\tau})}{d\Gamma_{D}(\lambda_{\tau}=+1/2) - d\Gamma_{D}(\lambda_{\tau}=-1/2)}$和(4)$Y_{3}(q^{2}) = (\frac{q^{2}}{m^{2}_{\tau}})(A^{D}_{\lambda} + 1)\frac{1}{A^{D}_{\lambda}}$。
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Search for more sensitive observables to charged scalar in $B \rightarrow D^{(*)}\tau\nu_{\tau}$ decays.
It has been known that $B \rightarrow D^{(*)} \tau \nu_{\tau}$ are good observables in the search for the charged Higgs. The recent obervation of deviation from standard-model by almost 4$\sigma$ by Babar, Belle and LHCb in $R(D^{(*)})$ revived the interest in possible signal of presence of charged Higgs in these modes. But such a large deviation in the rates, where standard-model has tree level contribution, coming from a charged Higgs alone is highly unlikely. However these decay modes are good probes to search for small charged Higgs signal if we can construct sensitive observables in these modes. In this work we would like to propose four new observables which shows much more sensitivity to the presence of charged Higgs than the usual observables such as $A_{\lambda}^{D^{(*)}}$ and $A_{\theta}^{D^{(*)}}$. These four observable are (1) $\frac{1}{A_{\lambda}^{D}}$,\ (2) $Y_{1}(q^{2}) = \frac{A^{D}_{\theta}}{A^{D}_{\lambda}}$,\ (3) $Y_{2}(q^{2}) = \frac{d\Gamma(B \rightarrow D^{*}\tau\nu_{\tau})}{d\Gamma_{D}(\lambda_{\tau}=+1/2) - d\Gamma_{D}(\lambda_{\tau}=-1/2)}$ and (4) $Y_{3}(q^{2}) = (\frac{q^{2}}{m^{2}_{\tau}})(A^{D}_{\lambda} + 1)\frac{1}{A^{D}_{\lambda}}$.
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来源期刊
Letters in High Energy Physics
Letters in High Energy Physics Physics and Astronomy-Nuclear and High Energy Physics
CiteScore
1.20
自引率
0.00%
发文量
4
审稿时长
12 weeks
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