Search for the radiative decay $D^+_s \to γρ(770)^+$

BESIII Collaboration
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Abstract

Using 7.33 fb$^{-1}$ of $e^+e^-$ collision data samples collected with the BESIII detector at center-of-mass energies between 4.128 and 4.226 GeV, we search for the radiative decay $D_s^+\to\gamma\rho(770)^+$ for the first time. A hint of $D_s^+\to\gamma\rho(770)^+$ is observed with a statistical significance of 2.5$\sigma$. %Our data contains a signal of this decay with a statistical significance of 2.5$\sigma$. %No obvious signals are found with the current statistics. The upper limits of the branching fraction for $D_s^+\to\gamma\rho(770)^+$ is set to be $\mathcal{B}(D^+_s\to \gamma\rho(770)^+) < 6.1\times$10$^{-4}$. The branching fraction of $D_s^+\to\gamma\rho(770)^+$ is measured to be $(2.2\pm0.9_{\rm stat.}\pm0.2_{\rm syst.})\times10^{-4}$, corresponding to an upper limit of $6.1\times$10$^{-4}$ at the $90\%$ confidence level.
寻找辐射衰变 $D^+_s 到 γρ(770)^+$
利用BESIII探测器在4.128和4.226 GeV之间的质心能量上收集的7.33 fb$^{-1}$的$e^+e^-$碰撞数据样本,我们首次寻找到了辐射衰变$D_s^+to\\gamma\rho(770)^+$。我们的数据包含了这一衰变的信号,统计意义为 2.5 美元/西格玛。$D_s^+\to\gamma\rho(770)^+$的分支分数上限设定为$\mathcal{B}(D^+_s\to\gamma\rho(770)^+) < 6.1\times$10$^{-4}$。测得$D_s^+to\\gamma\rho(770)^+$的分支分数为$(2.2\pm0.9_{\rmstat.}\pm0.2_{\rm syst.})\times10^{-4}$,对应于置信度为90%$的上限$6.1\times$10^{-4}$。
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