Tensor Meson Pole contributions to the HLbL piece of $a_μ$ within R$χ$T
Emilio J. Estrada, Pablo Roig
TL;DR
This work computes tensor-meson pole contributions to the HLbL piece of $a_\mu$ within Resonance Chiral Theory, using the lightest tensor nonet and two vector nonets in the chiral limit. In the minimal setup, only $\mathcal{F}_1^T$ is nonzero and is fixed by short-distance QCD constraints and radiative widths, yielding a negative total $a_\mu^{T\text{-poles}}$ of about $-4.3\times 10^{-11}$. Extending the Lagrangian to generate $\mathcal{F}_3^T$ flips the sign and yields $a_\mu^{T\text{-poles}}=+1.7(4.4)\times 10^{-11}$, broadly compatible with holographic results within uncertainties, though dominated by the uncertain normalization of $\mathcal{F}_3^T(0,0)$. The authors emphasize that a complete $a_\mu^{\rm T-poles}$ within this framework awaits the inclusion of $\mathcal{F}_{2,4,5}^T$ and urgent double-virtual tensor-transition data to constrain $\mathcal{F}_3^T(0,0)$, underscoring the need for targeted measurements of $T\to\gamma^*\gamma^*$.
Abstract
We compute the tensor meson pole contributions to the Hadronic Light-by-Light piece of $a_μ$ in the purely hadronic region, using Resonance Chiral Theory. Given the differences between the dispersive and holographic groups determinations, we consider timely to present an alternative evaluation. In our approach, the lightest tensor meson nonet and two vector meson resonance nonets are considered in the chiral limit. Disregarding operators with derivatives, only the form factor $\mathcal{F}_1^T$ is non-vanishing, as assumed in the dispersive study. All parameters are determined by imposing a set of short-distance QCD constraints, and the radiative decay widths. In this case, we obtain (in units of $10^{-11}$): $ a_2$-pole: $-\left(1.02(10)_{\rm stat}(^{+0.00}_{-0.12})_{\rm syst}\right)$, $f_2$-pole: $-\left(3.2(3)_{\rm stat}(^{+0.0}_{-0.4})_{\rm syst}\right)$ and $f_2^\prime$-pole: $-\left(0.042(13)_{\rm stat}\right)$, which add up to $a_μ^{a_2+f_2+f_2^\prime \rm -pole}=-\left(4.3^{+0.3}_{-0.5}\right)$, in close agreement with the holographic result when truncated to $\mathcal F_1^T$ only. However, with an ad-hoc extended Lagrangian, that also generates $\mathcal F_3^T$, as in the holographic approach, we have found: $ a_2$-pole: $+0.47(1.43)_{\rm norm}(3)_{\rm stat}(^{+0.06}_{-0.00})_{\rm syst}$, $f_2$-pole: $+1.18(4.18)_{\rm norm}(12)_{\rm stat}(^{+0.24}_{-0.00})_{\rm syst}$ and $f_2^\prime$-pole: $+0.040(78)_{\rm norm}(2)_{\rm stat}$, summing to $a_μ^{a_2+f_2+f_2^\prime \rm - pole}=+1.7(4.4)$, which agree with these recent determinations within uncertainties (dominated by the $\mathcal F_3^T$ normalization). We point out that $RχT$ generates all form factors, the contributions to $a_μ$ of $\mathcal F_{2,4,5}$ cannot be evaluated in the current basis, preventing for the moment a complete calculation of $a_μ^{\rm T-poles}$ within our framework.
