$\Omega_c$ excited states with heavy-quark spin symmetry

L. Tolos, R. Pavão, J. Nieves
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引用次数: 0

Abstract

We study the $C=1$, $S=-2$, $I=0$ sector, where five excited $\Omega_c$ states have been recently observed by the LHCb Collaboration. We start from a recently developed unitarized baryon-meson model that takes, as bare baryon-meson interaction, an extended Weinberg-Tomozawa kernel consistent with both chiral and heavy-quark spin symmetries. This ${\rm SU(6)} \times {\rm HQSS}$ scheme leads to a successful description of the observed lowest-lying odd parity charmed $\Lambda_c$(2595) and $\Lambda_c$(2625) states, and bottomed $\Lambda_b$(5912) and $\Lambda_b$(5920) resonances. Within this model, five odd-parity $\Omega_c$ states are dynamically generated, but with masses below 3 GeV, not allowing for an identification with the observed LHCb resonances. We revise this model and explore two different scenarios for the renormalization scheme, that is, using a modified common energy scale to perform the subtractions or utilizing a common ultraviolet cutoff to render finite the ultraviolet divergent loop functions in all channels. In both cases, we show that some (at least three) of the dynamically generated states can be identified with the experimental $\Omega_c$, while having odd parity and $J=1/2$ or $J=3/2$. Two of these states turn out to be part of the same ${\rm SU(6)} \times {\rm HQSS}$ multiplets as the charmed and bottomed $\Lambda$ baryons.
具有重夸克自旋对称的激发态
我们研究了$C=1$, $S=-2$, $I=0$部门,其中五个激发态最近被LHCb合作观察到$\Omega_c$。我们从最近发展的统一重子-介子模型开始,作为裸重子-介子相互作用,扩展Weinberg-Tomozawa核与手性和重夸克自旋对称一致。这个${\rm SU(6)} \times {\rm HQSS}$方案成功地描述了观测到的最低奇宇称粲$\Lambda_c$(2595)和$\Lambda_c$(2625)态,以及最低$\Lambda_b$(5912)和$\Lambda_b$(5920)共振。在这个模型中,五个奇宇称$\Omega_c$状态是动态生成的,但质量低于3 GeV,不允许与观测到的LHCb共振相识别。我们修改了该模型,并探索了重整化方案的两种不同方案,即使用修改的公共能量标度来执行减法或使用公共紫外线截止来在所有通道中呈现有限的紫外线发散回路函数。在这两种情况下,我们证明了一些(至少三个)动态生成的状态可以用实验$\Omega_c$识别,同时具有奇宇称和$J=1/2$或$J=3/2$。结果证明,其中两个态是与被吸引的和底部的$\Lambda$重子相同的${\rm SU(6)} \times {\rm HQSS}$多重子的一部分。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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