Production of $\eta_c(1S,2S)$ in $\e^+ e^-$ and $p p$ collisions

I. Babiarz, W. Schafer, A. Szczurek
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引用次数: 1

Abstract

We derive the light-front wave function (LFWF) representation of the $\gamma^{\star} \gamma^{\star} \to \eta_{c} (1S),\eta_{c}(2S)$ transition form factor $F(Q^2_1,Q^2_2)$ for two virtual photons in the initial state. For the LFWF, we use different models obtained from the solution of the Schrodinger equation for a variety of $c\bar{c}$ potentials. We compare our results to the BaBar experimental data for the $\eta_{c}(1S)$ transition form factor, for one real and one virtual photon. We observe that the onset of the asymptotic behaviour is strongly delayed and discuss applicability of the collinear and/or massless limit. In addition, we present a thorough analysis of $\eta_{c}(1S,2S)$ quarkonia hadroproduction in $k_{\perp}$-factorisation in the framework of the light-front potential approach for the quarkonium wave function. The off-shell matrix elements for the $g^{\star} g^{\star} \to \eta_{c} (1S,2S)$ vertices are derived. We discuss the importance of taking into account the gluon virtualities. We present the transverse momentum distributions of $\eta_c$ for several models of the unintegrated gluon distributions. Our calculations are performed for four distinct parametrizations for the $c\bar{c}$ interaction potential consistent with the meson spectra. We compare our results for $\eta_{c}(1S)$ to measurements by the LHCb collaboration and present predictions for $\eta_{c}(2S)$ production.
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在$\e^+ e^-$和$p p$碰撞中$\eta_c(1S,2S)$的产生
我们推导了初始状态下两个虚光子的$\gamma^{\star} \gamma^{\star} \to \eta_{c} (1S),\eta_{c}(2S)$跃迁形状因子$F(Q^2_1,Q^2_2)$的光前波函数(LFWF)表示。对于LFWF,我们使用从薛定谔方程解中得到的不同模型来计算各种$c\bar{c}$势。我们比较了我们的结果与BaBar实验数据的$\eta_{c}(1S)$跃迁形状因子,一个实光子和一个虚光子。我们观察到渐近行为的开始是强延迟的,并讨论了共线和/或无质量极限的适用性。此外,我们在夸克子波函数的光锋势方法的框架下,对$k_{\perp}$分解过程中$\eta_{c}(1S,2S)$夸克子的产氢进行了深入的分析。推导了$g^{\star} g^{\star} \to \eta_{c} (1S,2S)$顶点的离壳矩阵元素。我们讨论了考虑胶子虚性的重要性。我们给出了几种未积分胶子分布模型$\eta_c$的横向动量分布。我们对与介子谱一致的$c\bar{c}$相互作用势进行了四种不同的参数化计算。我们将$\eta_{c}(1S)$的结果与LHCb合作的测量结果进行了比较,并对$\eta_{c}(2S)$的产量进行了预测。
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