Sensitivity study of <inline-formula><tex-math id="M1">\begin{document}$\bar{K}_1(1270)$\end{document}</tex-math></inline-formula> decay dynamics using four <inline-formula><tex-math id="M2">\begin{document}$D\to \bar{K}_1(1270)(\to \bar K\pi\pi)e^+\nu$\end{document}</tex-math></inline-formula> decay channels

[1]
H.-Y. Cheng and X.-W. Kang, Eur. Phys. J. C 77: 587 (2017), [Erratum: Eur.Phys.J.C 77, 863 (2017)], arXiv: 1707.02851 [hep-ph].
[2]
G.-Y. Wang, L. Roca, E. Wang, W.-H. Liang, and E. Oset, Eur. Phys. J. C 80, 388 (2020), arXiv: 2002.07610[hep-ph]
[3]
S. Momeni, Eur. Phys. J. C 80, 553 (2020), arXiv: 2004.02522[hep-ph]
[4]
S. Momeni and R. Khosravi, J. Phys. G 46, 105006 (2019), arXiv: 1903.00860[hep-ph]
[5]
N. Isgur, D. Scora, B. Grinstein, and M. B. Wise, Phys. Rev. D 39, 799 (1989)
[6]
D. Scora and N. Isgur, Phys. Rev. D 52, 2783 (1995), arXiv: hep-ph/9503486
[7]
H. Hatanaka and K.-C. Yang, Phys. Rev. D 78, 074007 (2008), arXiv: 0808.3731[hep-ph]
[8]
S. Navas et al. (Particle Data Group), Phys. Rev. D 110, 030001 (2024)
[9]
W. Wang, F.-S. Yu, and Z.-X. Zhao, Phys. Rev. Lett. 125, 051802 (2020), arXiv: 1909.13083[hep-ph]
[10]
L. Bian, L. Sun, and W. Wang, Phys. Rev. D 104, 053003 (2021), arXiv: 2105.06207[hep-ph]
[11]
C. Daum et al. (ACCMOR), Nucl. Phys. B 187, 1 (1981)
[12]
M. Ablikim et al. (BESIII), Phys. Rev. D 104, 032011 (2021), arXiv: 2103.02482[hep-ex]
[13]
M. Ablikim et al. (BESIII), JHEP 10, 199 (2024), arXiv: 2408.04422[hep-ex]
[14]
H. Guler et al. (Belle), Phys. Rev. D 83, 032005 (2011), arXiv: 1009.5256[hep-ex]
[15]
M. Artuso et al. (CLEO), Phys. Rev. D 85, 122002 (2012), arXiv: 1201.5716[hep-ex]
[16]
M. Ablikim et al. (BESIII), Phys. Rev. D 95, 072010 (2017), arXiv: 1701.08591[hep-ex]
[17]
R. Aaij et al. (LHCb), Eur. Phys. J. C 78, 443 (2018), arXiv: 1712.08609[hep-ex]
[18]
P. d’Argent, N. Skidmore, J. Benton, J. Dalseno, E. Gersabeck, S. Harnew, P. Naik, C. Prouve, and J. Rademacker, JHEP 05, 143 (2017), arXiv: 1703.08505[hep-ex]
[19]
P.-F. Guo, D. Wang, and F.-S. Yu, Nucl. Phys. Rev. 36, 125 (2019), arXiv: 1801.09582[hep-ph]
[20]
M. Ablikim et al. (BESIII), Phys. Rev. Lett. 123, 231801 (2019), arXiv: 1907.11370[hep-ex]
[21]
M. Ablikim et al. (BESIII), Phys. Rev. Lett. 127, 131801 (2021), arXiv: 2102.10850[hep-ex]
[22]
M. Ablikim et al. (BESIII), JHEP 09, 089 (2024), arXiv: 2403.19091[hep-ex]
[23]
M. Ablikim et al. (BESIII), Phys. Rev. Lett. 135, 091801 (2025)
[24]
M. Ablikim et al. ((BESIII),, BESIII), Chin. Phys. C 48, 123001 (2024), arXiv: 2406.05827[hep-ex]
[25]
\begin{document}$ {\cal{B}}\left(K_1^{-}(1270) \rightarrow K^{-} \pi^{+} \pi^{-}\right)=\frac{1}{3} {\cal{B}}_{K_1 \rightarrow K \rho}+\frac{4}{9} {\cal{B}}_{K_1 \rightarrow K^* \pi}+$\end{document} \begin{document}$ {\cal{B}}_{K_1 \rightarrow K \omega} \times {\cal{B}}_{\omega \rightarrow \pi+\pi^{-}}+{\cal{B}}_{K_1 \rightarrow K f_0}, {\cal{B}}\left(\bar{K}_1^0(1270) \rightarrow\right.$\end{document} \begin{document}$ \left.K^{-} \pi^{+} \pi^0\right)=\frac{2}{3} {\cal{B}}_{K_1 \rightarrow K \rho}+\frac{4}{9} {\cal{B}}_{K_1 \rightarrow K^* \pi}.$\end{document}
[26]
R. M. Baltrusaitis et al. (MARK-III), Phys. Rev. Lett. 56, 2140 (1986)
[27]
J. Adler et al. (MARK-III), : 153 (1987).
[28]
M. Ablikim et al. (BESIII), Phys. Rev. D 110, L111102 (2024), arXiv: 2404.09219[hep-ex]
[29]
M. Achasov et al., Front. Phys. (Beijing) 19, 14701 (2024), arXiv: 2303.15790[hep-ex]
[30]
Y.-L. Fan, X.-D. Shi, X.-R. Zhou, and L. Sun, Eur. Phys. J. C 81, 1068 (2021), arXiv: 2107.06118[hep-ex]