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WANG Wenjun. Radiative Decays of the Bottom Strange Mesons in a Relativistic Quark Model[J]. Nuclear Physics Review, 2016, 33(1): 30-35. doi: 10.11804/NuclPhysRev.33.01.030
Citation: WANG Wenjun. Radiative Decays of the Bottom Strange Mesons in a Relativistic Quark Model[J]. Nuclear Physics Review, 2016, 33(1): 30-35. doi: 10.11804/NuclPhysRev.33.01.030

Radiative Decays of the Bottom Strange Mesons in a Relativistic Quark Model

doi: 10.11804/NuclPhysRev.33.01.030
  • Received Date: 2015-12-22
  • Accepted Date: 2016-03-20
  • Publish Date: 2016-03-20
  • We systematically study the radiative transitions of bottom-strange mesons in the framework of the relativistic constituent quark model. The partial widths of the E1 and M1 decays are predicted. The results predict that most of E1 decay widths are several keV and most of M1 decay widths are less than 1 keV,which give a roadmap of searching for the higher bottom-strange mesons via radiative decays. The experimental searches by the forthcoming Belle II can in turn provide further tests to our result in the present work.

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    沈阳化工大学材料科学与工程学院 沈阳 110142

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Radiative Decays of the Bottom Strange Mesons in a Relativistic Quark Model

doi: 10.11804/NuclPhysRev.33.01.030

Abstract: We systematically study the radiative transitions of bottom-strange mesons in the framework of the relativistic constituent quark model. The partial widths of the E1 and M1 decays are predicted. The results predict that most of E1 decay widths are several keV and most of M1 decay widths are less than 1 keV,which give a roadmap of searching for the higher bottom-strange mesons via radiative decays. The experimental searches by the forthcoming Belle II can in turn provide further tests to our result in the present work.

WANG Wenjun. Radiative Decays of the Bottom Strange Mesons in a Relativistic Quark Model[J]. Nuclear Physics Review, 2016, 33(1): 30-35. doi: 10.11804/NuclPhysRev.33.01.030
Citation: WANG Wenjun. Radiative Decays of the Bottom Strange Mesons in a Relativistic Quark Model[J]. Nuclear Physics Review, 2016, 33(1): 30-35. doi: 10.11804/NuclPhysRev.33.01.030

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