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Phenomenology of D s 1 mesons radiative transitions. / Bondar, A. E.; Milstein, A. I.

In: Physical Review D, Vol. 111, No. 11, 114019, 20.06.2025.

Research output: Contribution to journal › Article › peer-review

Harvard

Bondar, AE & Milstein, AI 2025, 'Phenomenology of D s 1 mesons radiative transitions', Physical Review D, vol. 111, no. 11, 114019. https://doi.org/10.1103/64y1-qyvt

APA

Bondar, A. E., & Milstein, A. I. (2025). Phenomenology of D s 1 mesons radiative transitions. Physical Review D, 111(11), [114019]. https://doi.org/10.1103/64y1-qyvt

Vancouver

Bondar AE, Milstein AI. Phenomenology of D s 1 mesons radiative transitions. Physical Review D. 2025 Jun 20;111(11):114019. doi: 10.1103/64y1-qyvt

Author

Bondar, A. E. ; Milstein, A. I. / Phenomenology of D s 1 mesons radiative transitions. In: Physical Review D. 2025 ; Vol. 111, No. 11.

BibTeX

@article{d999a8e7a46441ef9695dc9592a13a65,
title = "Phenomenology of D s 1 mesons radiative transitions",
abstract = " We discuss radiative transitions D s 1 → D s γ and D s 1 → D s * γ of p -wave mesons. Since D s 1 mesons have no certain C -parity, and the masses of quarks in these mesons differ significantly, then due to the spin-orbit interaction, each of the p -wave mesons with the total angular momentum J = 1 is a superposition of states with the total spin of quarks S tot = 0 and S tot = 1 . We explain why the partial width of D s 1 ( 2460 ) → D s γ radiative transition is significantly larger than the corresponding value for D s 1 ( 2536 ) → D s γ . We also predict the corresponding partial widths of B s 1 and B c 1 . ",
author = "Bondar, {A. E.} and Milstein, {A. I.}",
note = "Bondar A. E., Milstein A. I.Phenomenology of D s 1 mesons radiative transitions / A. E. Bondar, A. I. Milstein // Physical Review D. - 2025. - Т. 111. № 11. - С. 114019. DOI 10.1103/64y1-qyvt ",
year = "2025",
month = jun,
day = "20",
doi = "10.1103/64y1-qyvt",
language = "English",
volume = "111",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "11",

}

RIS

TY - JOUR

T1 - Phenomenology of D s 1 mesons radiative transitions

AU - Bondar, A. E.

AU - Milstein, A. I.

N1 - Bondar A. E., Milstein A. I.Phenomenology of D s 1 mesons radiative transitions / A. E. Bondar, A. I. Milstein // Physical Review D. - 2025. - Т. 111. № 11. - С. 114019. DOI 10.1103/64y1-qyvt

PY - 2025/6/20

Y1 - 2025/6/20

N2 - We discuss radiative transitions D s 1 → D s γ and D s 1 → D s * γ of p -wave mesons. Since D s 1 mesons have no certain C -parity, and the masses of quarks in these mesons differ significantly, then due to the spin-orbit interaction, each of the p -wave mesons with the total angular momentum J = 1 is a superposition of states with the total spin of quarks S tot = 0 and S tot = 1 . We explain why the partial width of D s 1 ( 2460 ) → D s γ radiative transition is significantly larger than the corresponding value for D s 1 ( 2536 ) → D s γ . We also predict the corresponding partial widths of B s 1 and B c 1 .

AB - We discuss radiative transitions D s 1 → D s γ and D s 1 → D s * γ of p -wave mesons. Since D s 1 mesons have no certain C -parity, and the masses of quarks in these mesons differ significantly, then due to the spin-orbit interaction, each of the p -wave mesons with the total angular momentum J = 1 is a superposition of states with the total spin of quarks S tot = 0 and S tot = 1 . We explain why the partial width of D s 1 ( 2460 ) → D s γ radiative transition is significantly larger than the corresponding value for D s 1 ( 2536 ) → D s γ . We also predict the corresponding partial widths of B s 1 and B c 1 .

UR - https://www.mendeley.com/catalogue/4ee53db1-75f1-3879-bcb1-9717aabb4edf/

U2 - 10.1103/64y1-qyvt

DO - 10.1103/64y1-qyvt

M3 - Article

VL - 111

JO - Physical Review D

JF - Physical Review D

SN - 2470-0010

IS - 11

M1 - 114019

ER -

ID: 71565265