Roles of $a_0(980)$ and $a_0(1710)$ in Cabibbo-suppressed process $D^+\to π^0π^+η$
Xiao-Hui Zhang, Jing-Yu Zhu, Li-Juan Liu, En Wang
TL;DR
The paper investigates the Cabibbo-suppressed decay $D^+ \to \pi^0\pi^+\eta$, incorporating a dynamically generated $a_0(980)$ through the chiral unitary approach and including $\rho$ and $a_0(1710)$ intermediate states. It develops a hadronization and final-state-interaction framework, solving a coupled-channel Bethe-Salpeter equation to obtain $a_0(980)$ amplitudes and uses Breit–Wigner forms for $a_0(1710)$, all combined with interference phases to predict invariant-mass distributions. Fits to BESIII data show that $a_0(980)$ dynamics reproduce the $~1\ \mathrm{GeV}$ peaks in $π^0η$ and $π^+η$, while $a_0(1710)$ is essential to describe the $1.6\ \mathrm{GeV}$ enhancement; the results support a mixed interpretation of these scalars and motivate further high-precision measurements. The work provides a quantitative link between light scalar meson structure and charmed-hadron decays, with potential implications for understanding scalar meson spectroscopy.
Abstract
Motivated by the BESIII amplitude analysis of the single Cabibbo-suppressed process $D^+\to π^0π^+η$, we investigate this reaction by taking into account the contributions from the $a_0(980)$, $ρ$, and $a_0(1710)$, where the scalar meson $a_0(980)$ could be dynamically generated from the $S$-wave pseudoscalar meson-pseudoscalar meson interaction within the chiral unitary approach. Our theoretical predictions for the $π^0η$, $π^+η$, and $π^+π^0$ invariant mass distributions are in agreement with the BESIII measurements, especially the clear peaks around 1~GeV in the $π^0η$ and $π^+η$ invariant mass distributions could be associated with the dynamically generated state $a_0(980)$. Furthermore, we demonstrate that the intermediate $a_0(1710)$ is also necessary to describe the enhancement structure around $1.6\sim 1.7$~GeV in the $π^{0/+}η$ invariant mass distribution. More precise experimental measurements of this process could provide deeper insights into the nature of the scalar mesons $a_0(980)$ and $a_0(1710)$.
