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The $\rho \gamma^* \to \pi (\rho)$ transition form factors in the Perturbative QCD factorization approach

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arxiv 1510.05108 v1 pith:ELIDOXQA submitted 2015-10-17 hep-ph hep-ex

classification hep-phhep-ex
keywords formgammatransitionpqcdfactorfactorsruleagree
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

In this paper, we studied the $\rho \gamma^* \to \pi$ and $\rho\gamma^*\to \rho$ transition processes and made the calculations for the $\rho\pi$ transition form factor $Q^4 F_{\rho\pi}(Q^2)$ and the $\rho$ meson electromagnetic form factors, $F_{\rm LL, LT,TT}(Q^2)$ and $F_{1,2,3}(Q^2)$, by employing the perturbative QCD (PQCD) factorization approach. For the $\rho \gamma^* \to \pi$ transition, we found that the contribution to form factor $Q^4 F_{\rho\pi}(Q)$ from the term proportional to the distribution amplitude combination $\phi^T_{\rho}(x_1)\phi^P_{\pi}(x_2)$ is absolutely dominant, and the PQCD predictions for both the size and the $Q^2$-dependence of this form factor $Q^4 F_{\rho\pi}(Q^2)$ agree well with those from the extended ADS/QCD models or the light-cone QCD sum rule. For the $\rho \gamma^* \to \rho$ transition and in the region of $Q^2\geq 3$ GeV$^2$, further more, we found that the PQCD predictions for the magnitude and their $Q^2$-dependence of the $F_1(Q^2)$ and $F_2(Q^2)$ form factors agree well with those from the QCD sum rule, while the PQCD prediction for $F_3(Q^2)$ is much larger than the one from the QCD sum rule.

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Cited by 2 Pith papers

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  1. Radiative Decays of Vector Mesons with Light-Cone Sum Rules

    hep-ph 2025-11 unverdicted novelty 5.0 of 10

    Light-cone sum rules yield radiative decay widths for ground-state vector mesons that match data where available and exhibit a universal linear dependence on a function A(x) in log coordinates arising from decay-const...

  2. Next-to-leading-order time-like rho electromagnetic form factors in ${k_{\rm T}}$ factorization

    hep-ph 2025-01 conditional novelty 5.0 of 10

    The NLO time-like rho meson electromagnetic form factors are obtained by analytic continuation of space-like NLO results, with twist-3 contributions dominating and predictions consistent with BABAR.

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