Roles of $a_0(980)$ and $a_0(1710)$ in Cabibbo-suppressed process $D^+\to Ï^0Ï^+η$
Roles of $a_0(980)$ and $a_0(1710)$ in Cabibbo-suppressed process $D^+\to Ï^0Ï^+η$
Motivated by the BESIII amplitude analysis of the single Cabibbo-suppressed process $D^+\to Ï^0Ï^+η$, we investigate this reaction by taking into account the contributions from the $a_0(980)$, $Ï$, 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 $Ï^0η$, $Ï^+η$, and $Ï^+Ï^0$ invariant mass distributions are in agreement with the BESIII measurements, especially the clear peaks around 1~GeV in the $Ï^0η$ and $Ï^+η$ 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 $Ï^{0/+}η$ 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 $a_0(1710)$.
Xiao-Hui Zhang、Jing-Yu Zhu、Li-Juan Liu、En Wang
物理学
Xiao-Hui Zhang,Jing-Yu Zhu,Li-Juan Liu,En Wang.Roles of $a_0(980)$ and $a_0(1710)$ in Cabibbo-suppressed process $D^+\to Ï^0Ï^+η$[EB/OL].(2025-08-05)[2025-08-16].https://arxiv.org/abs/2508.03493.点此复制
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