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Search for the radiative decay Ds+→γK∗892+. / BESIII Collaboration ; Ачасов, Михаил Николаевич; Мучной, Николай Юрьевич et al.

In: Journal of High Energy Physics, Vol. 2026, No. 7, 266, 28.07.2026.

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BESIII Collaboration, Ачасов МН, Мучной НЮ, Николаев ИБ. Search for the radiative decay Ds+→γK∗892+. Journal of High Energy Physics. 2026 Jul 28;2026(7):266. doi: 10.1007/JHEP07(2026)266

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@article{b18ab040e6794e5e8138e29d3e4c1fd0,
title = "Search for the radiative decay Ds+→γK∗892+",
abstract = "Using 7.33 fb−1 of e+e− collision data samples collected with the BESIII detectorat center-of-mass energies between 4.128 and 4.226 GeV, we perform a search for the radiative decay D+s → γK∗(892)+ via K∗(892)+ → K+π0 and K∗(892)+ → K0Sπ + for the first time. No significant signals are observed. The upper limit on the branching fraction of D+s → γK∗(892)+ is set to be 2.3 × 10−4 at the 90% confidence level.",
keywords = "Branching fraction, Charm Physics, e +-e − Experiments",
author = "{BESIII Collaboration} and Ачасов, {Михаил Николаевич} and Мучной, {Николай Юрьевич} and Николаев, {Иван Борисович}",
note = "The BESIII Collaboration thanks the staff of BEPCII (https://cstr.cn/31109.02.BEPC) and the IHEP computing center for their strong support. This work is supported in part by National Key R&D Program of China under Contracts Nos. 2023YFA1606000, 2023YFA1606704; National Natural Science Foundation of China (NSFC) under Contracts Nos. 12405094, 12275067, 11635010, 11935015, 11935016, 11935018, 12025502, 12035009, 12035013, 12061131003, 12192260, 12192261, 12192262, 12192263, 12192264, 12192265, 12221005, 12225509, 12235017, 12342502, 12361141819; Outstanding Young Talent Support Program of Henan Province; Science and Technology R&D Program Joint Fund Project of Henan Province (Grant No.225200810030); Science and Technology Innovation Leading Talent Support Program of Henan Province; the Excellent Youth Foundation of Henan Scientific Commitee under Contract No. 242300421044; Supported by the China Postdoctoral Science Foundation under Grant Number 2025M783403; the Chinese Academy of Sciences (CAS) Large-Scale Scientific Facility Program; the Strategic Priority Research Program of Chinese Academy of Sciences under Contract No. XDA0480600; CAS under Contract No. YSBR-101; 100 Talents Program of CAS; The Institute of Nuclear and Particle Physics (INPAC) and Shanghai Key Laboratory for Particle Physics and Cosmology; ERC under Contract No. 758462; German Research Foundation DFG under Contract No. FOR5327; Istituto Nazionale di Fisica Nucleare, Italy; Knut and Alice Wallenberg Foundation under Contracts Nos. 2021.0174, 2021.0299, 2023.0315; Ministry of Development of Turkey under Contract No. DPT2006K-120470; National Research Foundation of Korea under Contract No. NRF-2022R1A2C1092335; National Science and Technology fund of Mongolia; Polish National Science Centre under Contract No. 2024/53/B/ST2/00975; STFC (United Kingdom); Swedish Research Council under Contract No. 2019.04595; U.S. Department of Energy under Contract No. DE-FG02-05ER41374.",
year = "2026",
month = jul,
day = "28",
doi = "10.1007/JHEP07(2026)266",
language = "English",
volume = "2026",
journal = "Journal of High Energy Physics",
issn = "1029-8479",
publisher = "Springer US",
number = "7",

}

RIS

TY - JOUR

T1 - Search for the radiative decay Ds+→γK∗892+

AU - BESIII Collaboration

AU - Ачасов, Михаил Николаевич

AU - Мучной, Николай Юрьевич

AU - Николаев, Иван Борисович

N1 - The BESIII Collaboration thanks the staff of BEPCII (https://cstr.cn/31109.02.BEPC) and the IHEP computing center for their strong support. This work is supported in part by National Key R&D Program of China under Contracts Nos. 2023YFA1606000, 2023YFA1606704; National Natural Science Foundation of China (NSFC) under Contracts Nos. 12405094, 12275067, 11635010, 11935015, 11935016, 11935018, 12025502, 12035009, 12035013, 12061131003, 12192260, 12192261, 12192262, 12192263, 12192264, 12192265, 12221005, 12225509, 12235017, 12342502, 12361141819; Outstanding Young Talent Support Program of Henan Province; Science and Technology R&D Program Joint Fund Project of Henan Province (Grant No.225200810030); Science and Technology Innovation Leading Talent Support Program of Henan Province; the Excellent Youth Foundation of Henan Scientific Commitee under Contract No. 242300421044; Supported by the China Postdoctoral Science Foundation under Grant Number 2025M783403; the Chinese Academy of Sciences (CAS) Large-Scale Scientific Facility Program; the Strategic Priority Research Program of Chinese Academy of Sciences under Contract No. XDA0480600; CAS under Contract No. YSBR-101; 100 Talents Program of CAS; The Institute of Nuclear and Particle Physics (INPAC) and Shanghai Key Laboratory for Particle Physics and Cosmology; ERC under Contract No. 758462; German Research Foundation DFG under Contract No. FOR5327; Istituto Nazionale di Fisica Nucleare, Italy; Knut and Alice Wallenberg Foundation under Contracts Nos. 2021.0174, 2021.0299, 2023.0315; Ministry of Development of Turkey under Contract No. DPT2006K-120470; National Research Foundation of Korea under Contract No. NRF-2022R1A2C1092335; National Science and Technology fund of Mongolia; Polish National Science Centre under Contract No. 2024/53/B/ST2/00975; STFC (United Kingdom); Swedish Research Council under Contract No. 2019.04595; U.S. Department of Energy under Contract No. DE-FG02-05ER41374.

PY - 2026/7/28

Y1 - 2026/7/28

N2 - Using 7.33 fb−1 of e+e− collision data samples collected with the BESIII detectorat center-of-mass energies between 4.128 and 4.226 GeV, we perform a search for the radiative decay D+s → γK∗(892)+ via K∗(892)+ → K+π0 and K∗(892)+ → K0Sπ + for the first time. No significant signals are observed. The upper limit on the branching fraction of D+s → γK∗(892)+ is set to be 2.3 × 10−4 at the 90% confidence level.

AB - Using 7.33 fb−1 of e+e− collision data samples collected with the BESIII detectorat center-of-mass energies between 4.128 and 4.226 GeV, we perform a search for the radiative decay D+s → γK∗(892)+ via K∗(892)+ → K+π0 and K∗(892)+ → K0Sπ + for the first time. No significant signals are observed. The upper limit on the branching fraction of D+s → γK∗(892)+ is set to be 2.3 × 10−4 at the 90% confidence level.

KW - Branching fraction

KW - Charm Physics

KW - e +-e − Experiments

UR - https://www.scopus.com/pages/publications/105047915312

U2 - 10.1007/JHEP07(2026)266

DO - 10.1007/JHEP07(2026)266

M3 - Article

VL - 2026

JO - Journal of High Energy Physics

JF - Journal of High Energy Physics

SN - 1029-8479

IS - 7

M1 - 266

ER -

ID: 83281485