NLO effects for $\Omega_{QQQ}$ Baryons in QCD Sum Rules

We study the triply heavy baryons $\Omega_{QQQ}$ $(Q=c, b)$ in the QCD Sum Rules by calculating the next-to-leading order (NLO) contribution in the perturbative QCD part of the correlation functions. Compared with the leading order (LO) result, the NLO contribution is found to be very important to the $\Omega_{QQQ}$, for it not only leads to a large correction, but also reduces the parameters dependence and makes the Borel platform more distinct, especially for the $\Omega_{bbb}$ in the $\overline{\rm{MS}}$ scheme, where the platform appears only at NLO but not at LO. In particular, due to the inclusion of the NLO contribution, the renormalization schemes ($\overline{\rm{MS}}$ and On-Shell) dependence and scale dependence are significantly improved. As a result, after including the NLO contribution of the perturbative part in QCD sum rules, the masses are predicted to be $4.53^{+0.26}_{-0.11}$ GeV for $\Omega_{ccc}$ and $14.27^{+0.33}_{-0.32}$ GeV for $\Omega_{bbb}$, where the results are obtained at $\mu=M_B$ with errors including that from the variation of the renormalization scale $\mu$ in the range $(0.8-1.2) M_B$. A careful study for the $\mu$ dependence in a wider range is further performed, which shows that the LO results are very sensitive to the choice of $\mu$ whereas the NLO results are much better. In addition to the $\mu=M_B$ result, a quite stable value, (4.75-4.80) GeV, for the $\Omega_{ccc}$ mass is found in the range of $\mu=(1.2-2.0) M_B$.