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arxiv: 2012.02538 · v3 · pith:FLZSTYP4new · submitted 2020-12-04 · ✦ hep-ex

Search for the dark photon in B⁰ to A^(prime) A^(prime), A^(prime) to e^+ e^-, μ^+ μ^-, and π^+ π^- decays at Belle

S.-H. Park , Y.-J. Kwon , I. Adachi , H. Aihara , S. Al Said , D. M. Asner , H. Atmacan , T. Aushev
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R. Ayad V. Babu P. Behera J. Bennett M. Bessner V. Bhardwaj B. Bhuyan T. Bilka J. Biswal G. Bonvicini A. Bozek M. Bra\v{c}ko T. E. Browder M. Campajola L. Cao D. \v{C}ervenkov M.-C. Chang P. Chang A. Chen B. G. Cheon K. Chilikin H. E. Cho K. Cho S.-J. Cho S.-K. Choi Y. Choi S. Choudhury D. Cinabro S. Cunliffe S. Das N. Dash G. De Nardo F. Di Capua J. Dingfelder Z. Dole\v{z}al T. V. Dong S. Eidelman D. Epifanov D. Ferlewicz B. G. Fulsom R. Garg V. Gaur A. Garmash A. Giri P. Goldenzweig Y. Guan K. Gudkova C. Hadjivasiliou T. Hara O. Hartbrich K. Hayasaka H. Hayashii M. T. Hedges M. Hernandez Villanueva W.-S. Hou C.-L. Hsu K. Huang T. Iijima K. Inami G. Inguglia A. Ishikawa R. Itoh M. Iwasaki Y. Iwasaki W. W. Jacobs I. Jaegle E.-J. Jang H. B. Jeon S. Jia Y. Jin C. W. Joo K. K. Joo K. H. Kang G. Karyan T. Kawasaki C. Kiesling D. Y. Kim K.-H. Kim S. H. Kim Y.-K. Kim K. Kinoshita P. Kody\v{s} T. Konno S. Korpar D. Kotchetkov P. Kri\v{z}an R. Kroeger P. Krokovny T. Kuhr M. Kumar K. Kumara K. Lalwani I. S. Lee S. C. Lee C. H. Li J. Li L. K. Li Y. B. Li L. Li Gioi J. Libby K. Lieret Z. Liptak D. Liventsev T. Luo J. MacNaughton C. MacQueen M. Masuda T. Matsuda D. Matvienko M. Merola F. Metzner K. Miyabayashi R. Mizuk G. B. Mohanty S. Mohanty T. Mori H.-G. Moser M. Mrvar R. Mussa M. Nakao Z. Natkaniec A. Natochii L. Nayak M. Nayak M. Niiyama N. K. Nisar S. Nishida S. Ogawa H. Ono Y. Onuki P. Oskin P. Pakhlov G. Pakhlova S. Pardi C. W. Park H. Park S. Patra S. Paul T. K. Pedlar R. Pestotnik L. E. Piilonen T. Podobnik V. Popov E. Prencipe M. T. Prim M. Ritter M. R\"ohrken A. Rostomyan N. Rout G. Russo Y. Sakai S. Sandilya A. Sangal L. Santelj T. Sanuki V. Savinov G. Schnell J. Schueler C. Schwanda Y. Seino K. Senyo M. E. Sevior M. Shapkin C. Sharma C. P. Shen J.-G. Shiu A. Sokolov E. Solovieva S. Stani\v{c} M. Stari\v{c} Z. S. Stottler J. F. Strube M. Sumihama K. Sumisawa T. Sumiyoshi W. Sutcliffe M. Takizawa K. Tanida F. Tenchini M. Uchida T. Uglov Y. Unno S. Uno P. Urquijo S. E. Vahsen R. Van Tonder G. Varner K. E. Varvell A. Vinokurova V. Vorobyev E. Waheed C. H. Wang E. Wang M.-Z. Wang P. Wang M. Watanabe S. Watanuki S. Wehle E. Won X. Xu B. D. Yabsley W. Yan S. B. Yang H. Ye J. Yelton J. H. Yin Y. Yusa Z. P. Zhang V. Zhilich V. Zhukova V. Zhulanov (The Belle Collaboration)
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keywords primemathcaldarklimitsmathrmphotondecayshiggs
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We present a search for the dark photon $A^{\prime}$ in the $B^0 \to A^{\prime} A^{\prime}$ decays, where $A^{\prime}$ subsequently decays to $e^+ e^-$, $\mu^+ \mu^-$, and $\pi^+ \pi^-$. The search is performed by analyzing $772 \times 10^6$ $B\overline{B}$ events collected by the Belle detector at the KEKB $e^+ e^-$ energy-asymmetric collider at the $\Upsilon (4S)$ resonance. No signal is found in the dark photon mass range $0.01~\mathrm{GeV}/c^2 \le m_{A^{\prime}} \le 2.62~\mathrm{GeV}/c^2$, and we set upper limits of the branching fraction of $B^0 \to A^{\prime} A^{\prime}$ at the 90\% confidence level. The products of branching fractions, $\mathcal{B}(B^0 \to A^{\prime} A^{\prime}) \times \mathcal{B}(A^{\prime} \to e^+ e^-)^2$ and $\mathcal{B}(B^0 \to A^{\prime} A^{\prime}) \times \mathcal{B}(A^{\prime} \to \mu^+ \mu^-)^2$, have limits of the order of $10^{-8}$ depending on the $A^{\prime}$ mass. Furthermore, considering $A^{\prime}$ decay rate to each pair of charged particles, the upper limits of $\mathcal{B}(B^0 \to A^{\prime} A^{\prime})$ are of the order of $10^{-8}$-$10^{-5}$. From the upper limits of $\mathcal{B}(B^0 \to A^{\prime} A^{\prime})$, we obtain the Higgs portal coupling for each assumed dark photon and dark Higgs mass. The Higgs portal couplings are of the order of $10^{-2}$-$10^{-1}$ at $m_{h'} \simeq m_{B^0} \pm 40~\mathrm{MeV}/c^2$ and $10^{-1}$-$1$ at $m_{h'} \simeq m_{B^0} \pm 3~\mathrm{GeV}/c^2$.

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