衰变 D0→π+π-π+π- 和 π+π-π0π0 的振幅分析

Xinyu Shan
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摘要

利用 BESIII 探测器在质心能量 √s=3.773 GeV 时获得的相当于 2.93 fb-1 综合光度的 e+e- 歼灭数据,对衰变 D0→π+π-π+π- 和 D0→π+π-π0π0(non-η) 进行了联合振幅分析。得到了各个分量的拟合分数,并在两个信道中发现了衰变 D0→a1(1260)π、D0→π(1300)π、D0→ρ(770)ρ(770)和 D0→2(ππ)S 的主要分量之间的巨大干扰。根据得到的振幅模型,D0→π+π-π+π- 和 D0→π+π-π0π0(非η)的 CP 偶合分数分别为 (75.2 ± 1.1stat. ± 1.5syst.)%和 (68.9 ± 1.5stat. ± 2.4syst.)%。D0→π+π-π+π-和 D0→π+π-π0π0(非η)的分支率分别为 (0.688 ± 0.010stat. ± 0.010syst.)%和 (0.951 ± 0.025stat. ± 0.021syst.)%。在通过B-→DK-衰变确定CKM角γ(Φ3)时,振幅分析为测量D0→4π强相参数的分选策略提供了一个重要模型。本文内容可根据知识共享署名 3.0 许可条款使用。对本作品的任何进一步传播都必须注明作者、作品名称、期刊引文和 DOI。文章由 SCOAP3 资助,由中国物理学会、中国科学院高能物理研究所、中国科学院近代物理研究所和 IOP Publishing Ltd. 授权出版。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Amplitude Analysis of the Decays D0→π+π-π+π- and π+π-π0π0
Using e+e- annihilation data corresponding to an integrated luminosity of 2.93 fb-1 taken at the center-of-mass energy √s=3.773 GeV with the BESIII detector, a joint amplitude analysis is performed on the decays D0→π+π-π+π- and D0→π+π-π0π0(non-η). The fit fractions of individual components are obtained, and large interferences among the dominant components of the decays D0→a1(1260)π, D0→π(1300)π, D0→ρ(770)ρ(770) and D0→2(ππ)S are found in both channels. With the obtained amplitude model, the CP-even fractions of D0→π+π-π+π- and D0→π+π-π0π0(non-η) are determined to be (75.2 ± 1.1stat. ± 1.5syst.)% and (68.9 ± 1.5stat. ± 2.4syst.)%, respectively. The branching fractions of D0→π+π-π+π- and D0→π+π-π0π0(non-η) are measured to be (0.688 ± 0.010stat. ± 0.010syst.)% and (0.951 ± 0.025stat. ± 0.021syst.)%, respectively. The amplitude analysis provides an important model for binning strategy in the measurements of the strong phase parameters of D0→4π when used to determine the CKM angle γ(Φ3) via the B-→DK- decay. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Article funded by SCOAP3 and published under licence by Chinese Physical Society and the Institute of High Energy Physics of the Chinese Academy of Science and the Institute of Modern Physics of the Chinese Academy of Sciences and IOP Publishing Ltd.
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