Search for the massless dark photon with $D^0\to\omega\gamma'$ and $D^0\to\gamma\gamma'

Using $7.9~\rm{fb^{-1}}$ of $e^+e^-$ collision data collected at $\sqrt{s}=3.773$ GeV with the BESIII detector at the BEPCII collider, we search for the massless dark photon with the flavor-changing neutral current processes $D^0\to\omega\gamma'$ and $D^0\to\gamma\gamma'$ for the first tim...

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Hauptverfasser: Ablikim, M, Achasov, M. N, Bai, Y, Berger, N, Chen, C, Chen, M. L, Chen, S. J, Chen, X. T, Cui, J. J, Dai, J. P, Denig, A, Ding, B, Dong, X, Du, S. X, Duan, Y. Y, Fang, J, Feng, J. H, Garbolino, S, Gilman, A, Gradl, W, Guan, C. Y, Guo, M. J, Guskov, A, Hanisch, F, Hu, S. L, Huang, L. Q, Jackson, J, Jeong, J. H, Ji, X. L, Jia, X. Q, Jiang, X. S, Kalantar-Nayestanaki, N, Kolcu, O. B, Kuessner, M, Lenz, T, Li, Cheng, Li, H. B, Li, H. N, Li, J. S, Li, K, Li, M. H, Li, Y. G, Liang, H, Liu, H, Liu, H. H, Liu, S. B, Liu, W. K, Lou, X. C, Lu, F. X, Luo, X. L, Ma, T, Ma, X. Y, Meng, Z. X, Miao, H, Muchnoi, N. Yu, Pan, X, Peng, H. P, Plura, S, Qi, F. Z, Qi, M, Qi, T. Y, Sarantsev, A, Scodeggio, M, Shao, M, Shi, Q. Q, Shi, S. Y, Sun, G. B, Tang, G. Y, Thoren, V, Wang, F, Wang, H. J, Wang, X. F, Wu, C, Wu, L. J, Wu, X. H, Xiao, D, Xiao, G. Y, Xie, Y. H, Xu, Q. N, Xu, Y, Yan, X. Q, Yang, H. X, Yang, Y, Yang, Y. X, Yu, T, Yu, X. D, Yuan, C. Z, Yuan, J, Zafar, A. A, Zeng, F. R, Zhang, G. Y, Zhang, H. C, Zhang, H. Y, Zheng, J. P, Zhou, J. Y, Zhou, S, Zhou, X. Y, Zhu, A. N, Zhu, J, Zhu, K. S
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Zusammenfassung:Using $7.9~\rm{fb^{-1}}$ of $e^+e^-$ collision data collected at $\sqrt{s}=3.773$ GeV with the BESIII detector at the BEPCII collider, we search for the massless dark photon with the flavor-changing neutral current processes $D^0\to\omega\gamma'$ and $D^0\to\gamma\gamma'$ for the first time. No significant signals are observed, and the upper limits at the 90% confidence level on the massless dark photon branching fraction are set to be $1.1\times10^{-5}$ and $2.0\times10^{-6}$ for $D^0\to\omega\gamma'$ and $D^0\to\gamma\gamma'$, respectively. These results provide the most stringent constraint on the new physics energy scale associated with $cu\gamma'$ coupling in the world, with the new physics energy scale related parameter $|\mathbb{C}|^2+|\mathbb{C}_5|^2
DOI:10.48550/arxiv.2409.02578