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Search for the leptonic decay D+→e+νe. / The BESIII Collaboration ; Ачасов, Михаил Николаевич; Мучной, Николай Юрьевич и др.

в: Chinese Physics C, Том 49, № 6, 063001, 2025.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

The BESIII Collaboration, Ачасов, МН, Мучной, НЮ & Николаев, ИБ 2025, 'Search for the leptonic decay D+→e+νe', Chinese Physics C, Том. 49, № 6, 063001. https://doi.org/10.1088/1674-1137/adc11d

APA

The BESIII Collaboration, Ачасов, М. Н., Мучной, Н. Ю., & Николаев, И. Б. (2025). Search for the leptonic decay D+→e+νe. Chinese Physics C, 49(6), [063001]. https://doi.org/10.1088/1674-1137/adc11d

Vancouver

The BESIII Collaboration, Ачасов МН, Мучной НЮ, Николаев ИБ. Search for the leptonic decay D+→e+νe. Chinese Physics C. 2025;49(6):063001. doi: 10.1088/1674-1137/adc11d

Author

The BESIII Collaboration ; Ачасов, Михаил Николаевич ; Мучной, Николай Юрьевич и др. / Search for the leptonic decay D+→e+νe. в: Chinese Physics C. 2025 ; Том 49, № 6.

BibTeX

@article{2f6d96a3012147dcaa3133160370302d,
title = "Search for the leptonic decay D+→e+νe",
abstract = "We search for the leptonic decay D+→e+νe using an e+e- collision data sample with an integrated luminosity of 20.3 fb collected with the BESIII detector at a center-of-mass energy of 3.773 GeV. Significant signal is not observed, and an upper limit on the branching fraction of D+→e+νe is set as 9.7 × 10-7, at a confidence level of 90%. Our upper limit is an order of magnitude smaller than the previous limit for this decay mode.",
author = "{BESIII Collaboration} and Ачасов, {Михаил Николаевич} and Мучной, {Николай Юрьевич} and Николаев, {Иван Борисович}",
note = "Supported in part by the National Key R&D Program of China (2023YFA1606000, 2020YFA0406400, 2020YFA0406300), the National Natural Science Foundation of China(NSFC) (11635010, 11735014, 11935015, 11935016, 11875054, 11935018, 12025502, 12035009, 12035013, 12061131003, 12192260, 12192261, 12192262, 12192263, 12192264, 12192265, 12221005, 12225509, 12235017, 12361141819), the Chinese Academy of Sciences (CAS) Large-Scale Scientific Facility Program, the CAS Center for Excellence in Particle Physics (CCEPP), the Joint Large-Scale Scientific Facility Funds of the NSFC and CAS (U2032104, U1832207), the 100 Talents Program of CAS, the Excellent Youth Foundation of Henan Scientific Commitee (242300421044), the Institute of Nuclear and Particle Physics (INPAC) and Shanghai Key Laboratory for Particle Physics and Cosmology, the German Research Foundation DFG (FOR5327), the Istituto Nazionale di Fisica Nucleare, Italy, the Knut and Alice Wallenberg Foundation (2021.0174, 2021.0299), the Ministry of Development of Turkey (DPT2006K-120470), the National Research Foundation of Korea (NRF-2022R1A2C1092335), the National Science and Technology Fund of Mongolia, the National Science Research and Innovation Fund (NSRF) via the Program Management Unit for Human Resources & Institutional Development, Research, and Innovation of Thailand (B16F640076, B50G670107), the Polish National Science Center (2019/35/O/ST2/02907), the Swedish Research Council (2019.04595), the Swedish Foundation for International Cooperation in Research and Higher Education (CH2018-7756), and the US Department of Energy (DE-FG02-05ER41374).",
year = "2025",
doi = "10.1088/1674-1137/adc11d",
language = "English",
volume = "49",
journal = "Chinese Physics C",
issn = "1674-1137",
publisher = "IOP Publishing Ltd.",
number = "6",

}

RIS

TY - JOUR

T1 - Search for the leptonic decay D+→e+νe

AU - BESIII Collaboration

AU - Ачасов, Михаил Николаевич

AU - Мучной, Николай Юрьевич

AU - Николаев, Иван Борисович

N1 - Supported in part by the National Key R&D Program of China (2023YFA1606000, 2020YFA0406400, 2020YFA0406300), the National Natural Science Foundation of China(NSFC) (11635010, 11735014, 11935015, 11935016, 11875054, 11935018, 12025502, 12035009, 12035013, 12061131003, 12192260, 12192261, 12192262, 12192263, 12192264, 12192265, 12221005, 12225509, 12235017, 12361141819), the Chinese Academy of Sciences (CAS) Large-Scale Scientific Facility Program, the CAS Center for Excellence in Particle Physics (CCEPP), the Joint Large-Scale Scientific Facility Funds of the NSFC and CAS (U2032104, U1832207), the 100 Talents Program of CAS, the Excellent Youth Foundation of Henan Scientific Commitee (242300421044), the Institute of Nuclear and Particle Physics (INPAC) and Shanghai Key Laboratory for Particle Physics and Cosmology, the German Research Foundation DFG (FOR5327), the Istituto Nazionale di Fisica Nucleare, Italy, the Knut and Alice Wallenberg Foundation (2021.0174, 2021.0299), the Ministry of Development of Turkey (DPT2006K-120470), the National Research Foundation of Korea (NRF-2022R1A2C1092335), the National Science and Technology Fund of Mongolia, the National Science Research and Innovation Fund (NSRF) via the Program Management Unit for Human Resources & Institutional Development, Research, and Innovation of Thailand (B16F640076, B50G670107), the Polish National Science Center (2019/35/O/ST2/02907), the Swedish Research Council (2019.04595), the Swedish Foundation for International Cooperation in Research and Higher Education (CH2018-7756), and the US Department of Energy (DE-FG02-05ER41374).

PY - 2025

Y1 - 2025

N2 - We search for the leptonic decay D+→e+νe using an e+e- collision data sample with an integrated luminosity of 20.3 fb collected with the BESIII detector at a center-of-mass energy of 3.773 GeV. Significant signal is not observed, and an upper limit on the branching fraction of D+→e+νe is set as 9.7 × 10-7, at a confidence level of 90%. Our upper limit is an order of magnitude smaller than the previous limit for this decay mode.

AB - We search for the leptonic decay D+→e+νe using an e+e- collision data sample with an integrated luminosity of 20.3 fb collected with the BESIII detector at a center-of-mass energy of 3.773 GeV. Significant signal is not observed, and an upper limit on the branching fraction of D+→e+νe is set as 9.7 × 10-7, at a confidence level of 90%. Our upper limit is an order of magnitude smaller than the previous limit for this decay mode.

UR - https://www.webofscience.com/wos/woscc/full-record/WOS:001489785500001

U2 - 10.1088/1674-1137/adc11d

DO - 10.1088/1674-1137/adc11d

M3 - Article

VL - 49

JO - Chinese Physics C

JF - Chinese Physics C

SN - 1674-1137

IS - 6

M1 - 063001

ER -

ID: 80860033