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First Observation and Dynamical Study of the $D^+_s\to f_{0}(980) \mu^+\nu_\mu$ Decay

Besiii Collaboration M. Ablikim M. N. Achasov P. Adlarson X. Ai C. Akondi R. Aliberti A. Amoroso Q. An Y. An M. Anderson Y. Bai O. Bakina H.-R. Bao X. Bao M. Barbagiovanni V. Batozskaya K. Begzsuren N. Berger M. Berlowski M. Bertani D. Bettoni F. Bianchi E. Bianco A. Bortone I. Boyko R. Briere A. Brueggemann D. Cabiati H. Cai M.-H. Cai X. Cai A. Calcaterra Gui Cao N. Cao S. Cetin X.-Y. Chai J. Chang T. Chang G.-R. Che Y.-Z. Che C.-H. Chen Chao Chen G. Chen H.-S. Chen H.-Y. Chen M.-L. Chen S.-J. Chen S.-M. Chen T. Chen W. Chen X.-R. Chen X.-T. Chen X.-Y. Chen Y.-B. Chen Y.-Q. Chen Z.-K. Chen J. Cheng L.-N. Cheng S. Choi X. Chu G. Cibinetto F. Cossio J. Cottee-Meldrum Hua-Ming Dai J.-P. Dai X.-C. Dai A. Dbeyssi R. E. de Boer D. Dedovich Chi Deng Z.-Y. Deng A. Denig I. Denisenko M. Destefanis F. De Mori E. Di Fiore X.-X. Ding Y. Ding Y.-X. Ding J. Dong L.-Y. Dong Mei Dong X. Dong Z.-J. Dong M.-C. Du Shao-Xu Du Shao-Xu Du X.-L. Du Y.-Q. Du Y.-Y. Duan Zhu-Ding Duan P. Egorov Gao Fan J.-J. Fan Y.-H. Fan J. Fang Jin Fang S.-S. Fang W.-X. Fang Y.-Q. Fang L. Fava F. Feldbauer G. Felici C.-Q. Feng J.-H. Feng Q.-X. Feng Y.-T. Feng M. Fritsch C. Fu J.-L. Fu Y.-W. Fu H. Gao Xu-Yang Gao Y. Gao Y.-N. Gao Y.-Y. Gao Yu-Nong Gao Z. Gao S. Garbolino I. Garzia L. Ge P.-T. Ge Z.-W. Ge C. Geng A. Gilman K. Goetzen J. Gollub J. Gong J. Gong L. Gong W. Gong W. Gradl M. Greco M. Gu M. Gu C. Guan Alin Guo H. Guo J.-N. Guo L.-B. Guo M.-J. Guo R. Guo X. Guo Y.-P. Guo Z. Guo A. Guskov J. Gutierrez J. Han T. Han X. Han F. Hanisch Ke-Yu Hao Xuan Hao F. Harris C.-Z. He K. He K. He F. H. Heinsius C. H. Heinz Y. Heng C. Herold P. Hong G.-Y. Hou X.-T. Hou Y.-R. Hou Z. Hou H.-M. Hu J.-F. Hu Q.-P. Hu S.-L. Hu T. Hu Y. Hu Y.-X. Hu Z.-M. Hu G.-S. Huang K.-X. Huang L.-Q. Huang P. Huang X.-T. Huang Y.-P. Huang Y.-S. Huang T. Hussain N. Hüsken N. D. der Wiesche J. Jackson Q. Ji Q. Ji W. Ji X.-B. Ji X.-L. Ji Y.-Y. Ji L. Jia X.-Q. Jia D. Jiang S.-J. Jiang X.-S. Jiang Y. Jiang J.-B. Jiao J. Jiao Z. Jiao L.-C. Jin S. Jin Y. Jin M.-Q. Jing X.-M. Jing T. Johansson S. Kabana X. Kang X. Kang Bin Ke V. Khachatryan A. Khoukaz O. B. Kolcu B. Kopf L. Kröger L. Krümmel Yi-Xing Kuang X. Kui N. Kumar A. Kupsc W. Kühn Q. Lan W.-N. Lan T. Lei M. Lellmann T. Lenz C. Li C.-H. Li C.-K. Li Chun-Kai Li Cong Li D.-M. Li F. Li G. Li H.-B. Li H.-J. Li H.-L. Li H.-N. Li H.-P. Li Hui Li J.-N. Li J.-S. Li J.-W. Li K. Li K.-L. Li L.-J. Li L.-K. Li Lei Li M.-H. Li M.-R. Li M.-T. Li P.-L. Li P.-R. Li Q.-M. Li Q.-X. Li R. Li S. Li S.-X. Li S.-Y. Li Shan-Shan Li T. Li T.-Y. Li W.-D. Li W.-G. Li X. Li X.-H. Li X.-K. Li X.-L. Li X.-Y. Li X.-Z. Li Y. Li Y.-H. Li Y.-B. Li Y.-C. Li Y.-G. Li Y.-P. Li Z.-H. Li Z.-J. Li Z.-L. Li Z.-X. Li Z.-Y. Li C. Liang H. Liang Y.-F. Liang Y.-T. Liang Z.-Z. Liang Guo-Ya Liao Li-Dan Liao M. Liao Y.-P. Liao J. Libby A. Limphirat C. Lin C. Lin D. Lin T. Lin B.-J. Liu B.-X. Liu C. Liu C.-X. Liu F. Liu F.-H. Liu Feng Liu G.-M. Liu H. Liu H.-B. Liu H.-M. Liu Hui-Hui Liu J.-B. Liu J.-J. Liu K. Liu K.-Y. Liu Ke Liu Kun Liu L. Liu L.-C. Liu Lu Liu M.-H. Liu Li-Yu Daisy Liu Q. Liu S.-B. Liu T. Liu W.-M. Liu W.-T. Liu X. Liu X.-K. Liu X.-L. Liu X.-P. Liu X.-T. Liu X.-Y. Liu Y. Liu Y.-B. Liu Yi Liu Z.-A. Liu Z.-D. Liu Z.-L. Liu Z.-Q. Liu Z.-X. Liu Z.-Y. Liu X. Lou H.-J. Lu J.-G. Lu X.-L. Lu Y. Lu Y.-H. Lu Y.-P. Lu Z.-H. Lu C.-L. Luo J.-R. Luo J.-S. Luo Mi Luo T. Luo X.-L. Luo Z.-Y. Lv X. Lyu Y. Lyu Y. Lyu F.-C. Ma H.-L. Ma Heng Ma J.-L. Ma L.-L. Ma L.-R. Ma Q.-M. Ma R. Ma R. Ma T. Ma X.-T. Ma X.-Y. Ma F. Maas I. Mackay M. Maggiora S. Maity S. Malde L. M. Mansur Y.-J. Mao Z.-P. Mao S. Marcello A. Marshall F. M. Melendi Y.-H. Meng Zhen Meng G. Mezzadri H. Miao Tai-Shan Min R. Mitchell Xiang-Jun Mo B. Moses N. Muchnoi J. Muskalla Y. Nefedov F. Nerling H. Neuwirth Z. Ning S. Nisar Q. Niu W.-D. Niu Y. Niu C. Normand S. L. Olsen Q. Ouyang I. Ovtin S. Pacetti Y. Pan A. Pathak Y.-P. Pei M. Pelizaeus Ge Peng H.-P. Peng X.-J. Peng Y.-Y. Peng K. Peters K. Petridis Jing-Jing Ping R. Ping S. Plura V. Prasad L. Pöpping Fang-Zheng Qi H. Qi S. Qian W.-B. Qian Chloe Qiao J.-H. Qiao Jin Qin Jin Qin L. Qin L. Qin P.-B. Qin Xuan Qin Xuan Qin Z.-H. Qin J.-F. Qiu Zhao-Bo Qu J. Rademacker K. Ravindran C. F. Redmer A. Rivetti M. Rolo G. Rong S.-S. Rong F. Rosini Ch. Rosner Megan Ruan W. Ruangyoo N. Salone A. Sarantsev Y. Schelhaas M. Schernau K. Schoenning M. Scodeggio W. Shan X. Shan Z.-J. Shang J. Shangguan L. Shao M. Shao C.-P. Shen H.-F. Shen Wei Shen X.-Y. Shen B. Shi Chen Shi H. Shi J.-L. Shi J.-Y. Shi M.-H. Shi S. Shi X. Shi H. L. Song J. Song M. Song T. Song W. Song Y. Song Zi-Rong Song S. Sosio S. Spataro S. Stansilaus F. Stieler M. Stolte S.-S. Su G.-B. Sun G.-X. Sun H. Sun H.-K. Sun J.-F. Sun K. Sun L. Sun R. Sun S.-S. Sun T. Sun W.-Y. Sun Y.-C. Sun Y.-H. Sun Y.-J. Sun Y.-Z. Sun Z.-Q. Sun Z.-T. Sun H. Tabaharizato
Sep 2026 · 0 citations · 5 references
Physics

Abstract

Using 7.33 fb$^{-1}$ of $e^+e^-$ annihilation data recorded with the BESIII detector at center-of-mass energies from 4.128 to 4.226 GeV, we report the first observation and dynamical study of the semileptonic decay $D^+_s\to f_{0}(980) \mu^+\nu_\mu$. The absolute branching fraction of $D^+_s\to f_{0}(980) \mu^+\nu_\mu$ with $ f_{0}(980)\to \pi^+ \pi^-$ is $(1.59 \pm 0.18_{\rm stat} \pm 0.11_{\rm syst}) \times10^{-3}$. Combining this result with our earlier BESIII measurement of ${\mathcal B}(D^+_s\to f_{0}(980) e^+\nu_e)$, their ratio is found to be $\frac{{\mathcal B}(D^+_s\to f_{0}(980) \mu^+\nu_\mu)}{{\mathcal B}(D^+_s\to f_{0}(980)e^+\nu_e)} = 0.92\pm0.13_{\rm stat}\pm0.08_{\rm syst}$, in agreement with the Standard Model expectation of lepton flavor universality. From a dynamical analysis of the $D_{s}^{+} \to f_{0}(980)\mu^+\nu_\mu$ decay with a simple pole parametrization for the hadronic transition form factor, the product of the form factor $f^{f_{0}(980)}_{+}(0)$ and the $c\to s$ Cabibbo-Kobayashi-Maskawa matrix element $|V_{cs}|$ is determined to be $f^{f_{0}(980)}_{+}(0)|V_{cs}|=0.490\pm0.059_{\rm stat}\pm0.025_{\rm syst}$. Averaging with our previously reported result for the $D_{s}^{+} \to f_{0}(980)e^+\nu_e$ decay, we obtain $f^{f_{0}(980)}_{+}(0)|V_{cs}|=0.500\pm0.016_{\rm stat}\pm0.020_{\rm syst}$. Using $|V_{cs}|$ from the CKMfitter group, we extract $f^{f_{0}(980)}_{+}(0)=0.514\pm0.017_{\rm stat}\pm0.021_{\rm syst}$. This represents the most precise determination of the $D_{s} \to f_{0}(980)$ transition form factor to date, and provides stringent tests of various theoretical models.

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