Heavy four-quark mesons bcb‾c‾: Scalar particle

IF 4.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
S.S. Agaev , K. Azizi , H. Sundu
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引用次数: 0

Abstract

Parameters of the heavy four-quark scalar meson Tbcbc with content bcbc are calculated by means of the sum rule method. This structure is considered as a diquark-antidiquark state built of scalar diquark and antidiquark components. The mass and current coupling of Tbcbc are evaluated in the context of the two-point sum rule approach. The full width of this tetraquark is estimated by taking into account two types of its possible strong decay channels. First class includes dissociation of Tbcbc to mesons ηcηb, Bc+Bc, Bc+Bc and Bc+(13P0)Bc. Another type of processes are generated by annihilations bbqq of constituent b-quarks which produces the final-state charmed meson pairs D+D, D0D0, D+D, and D0D0. Partial width all of these decays are found using the three-point sum rule method which is required to calculate strong couplings at corresponding meson-meson-tetraquark vertices. Predictions obtained for the mass m=(12697±90)MeV and width Γ[Tbcbc]=(142.4±16.9)MeV of this state are compared with alternative results, and are useful for further experimental investigations of fully heavy resonances.
重四夸克介子 bcb‾c‾:标量粒子
利用和则法计算了含有bcb-‾c-‾的重四夸克标量介子Tbcb-‾c-‾的参数。这种结构被认为是由标量二夸克和反二夸克组成的二夸克-反二夸克态。在两点和则方法的背景下评估了Tbcb‾c‾的质量和电流耦合。通过考虑两类可能的强衰变通道,估算了这种四夸克的全宽。第一类包括Tbcb‾c‾解离成介子ηcηb、Bc+Bc-、Bc⁎+Bc⁎-和Bc+(13P0)Bc⁎-。另一类过程是由组成b-夸克的湮灭b‾b→q‾q产生的,它们产生了终态的粲介子对D+D-、D0D‾0、D⁎+D⁎-和D⁎0D‾⁎0。所有这些衰变的部分宽度都是用三点和规则方法找到的,而计算相应介子-介子-四夸克顶点的强耦合需要这种方法。对该状态的质量m=(12697±90)MeV和宽度Γ[Tbcb-‾c-‾]=(142.4±16.9)MeV进行了预测,并与其他结果进行了比较,这对全重共振的进一步实验研究很有帮助。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Physics Letters B
Physics Letters B 物理-物理:综合
CiteScore
9.10
自引率
6.80%
发文量
647
审稿时长
3 months
期刊介绍: Physics Letters B ensures the rapid publication of important new results in particle physics, nuclear physics and cosmology. Specialized editors are responsible for contributions in experimental nuclear physics, theoretical nuclear physics, experimental high-energy physics, theoretical high-energy physics, and astrophysics.
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