最近Ξ-nuclear绑定状态信号的兼容性

IF 4.5 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
E. Friedman, A. Gal
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Gal","doi":"10.1016/j.physletb.2025.139728","DOIUrl":null,"url":null,"abstract":"<div><div>J-PARC E05 reported recently a hint of a <span><math><msup><mrow><mi>Ξ</mi></mrow><mrow><mo>−</mo></mrow></msup><msup><mrow><mo>−</mo></mrow><mrow><mn>11</mn></mrow></msup><mi>B</mi></math></span> nuclear state in the <span><math><mmultiscripts><mrow><mi>C</mi></mrow><mprescripts></mprescripts><none></none><mrow><mn>12</mn></mrow></mmultiscripts><msubsup><mrow><mo>(</mo><msup><mrow><mi>K</mi></mrow><mrow><mo>−</mo></mrow></msup><mo>,</mo><msup><mrow><mi>K</mi></mrow><mrow><mo>+</mo></mrow></msup><mo>)</mo></mrow><mrow><mi>Ξ</mi></mrow><mrow><mn>12</mn></mrow></msubsup><mrow><mi>Be</mi></mrow></math></span> spectrum, bound by <span><math><msub><mrow><mi>B</mi></mrow><mrow><msup><mrow><mi>Ξ</mi></mrow><mrow><mo>−</mo></mrow></msup></mrow></msub><mo>=</mo><mn>8.9</mn><mo>±</mo><msubsup><mrow><mn>1.4</mn></mrow><mrow><mo>−</mo><mn>3.1</mn></mrow><mrow><mo>+</mo><mn>3.8</mn></mrow></msubsup></math></span> MeV. Using a density-dependent Ξ-nuclear optical potential <span><math><msubsup><mrow><mi>V</mi></mrow><mrow><mi>opt</mi></mrow><mrow><mi>Ξ</mi></mrow></msubsup><mo>(</mo><mi>ρ</mi><mo>)</mo></math></span> we explore to what extent a <span><math><msubsup><mrow><mi>Ξ</mi></mrow><mrow><mn>1</mn><mi>s</mi></mrow><mrow><mo>−</mo></mrow></msubsup></math></span> assignment of this nuclear state is compatible with <span><math><msubsup><mrow><mi>Ξ</mi></mrow><mrow><mn>1</mn><mi>s</mi></mrow><mrow><mo>−</mo></mrow></msubsup></math></span> and <span><math><msubsup><mrow><mi>Ξ</mi></mrow><mrow><mn>1</mn><mi>p</mi></mrow><mrow><mo>−</mo></mrow></msubsup></math></span> nuclear-state interpretations of <span><math><msup><mrow><mi>Ξ</mi></mrow><mrow><mo>−</mo></mrow></msup></math></span> capture events in light emulsion-nuclei experiments. 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This finding supports reassigning <span><math><msup><mrow><mi>Ξ</mi></mrow><mrow><mo>−</mo></mrow></msup></math></span> capture events in <sup>14</sup>N, originally assigned as <span><math><msubsup><mrow><mi>Ξ</mi></mrow><mrow><mn>1</mn><mi>s</mi></mrow><mrow><mo>−</mo></mrow></msubsup><msup><mrow><mo>−</mo></mrow><mrow><mn>14</mn></mrow></msup><mi>N</mi></math></span> nuclear states, to <span><math><msubsup><mrow><mi>Ξ</mi></mrow><mrow><mn>1</mn><mi>p</mi></mrow><mrow><mn>0</mn></mrow></msubsup><msup><mrow><mo>−</mo></mrow><mrow><mn>14</mn></mrow></msup><mi>C</mi></math></span> nuclear states. 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引用次数: 0

摘要

J-PARC E05最近报道了在BΞ−=8.9±1.4−3.1+3.8 MeV的C12(K−,K+)Ξ12Be谱中发现Ξ−−11B核态的提示。利用密度相关的Ξ-nuclear光势VoptΞ(ρ),我们探索了在何种程度上该核态的Ξ1s -赋值与轻乳剂核实验中Ξ-捕获事件的Ξ1s -和Ξ1p -核态解释兼容。我们发现,目前唯一可接受的Ξ1s -分配,除非VoptΞ(ρ)的异常强的排斥ρ2分量,是Ξ - - 11B信号的分配。这一发现支持将原来分配为Ξ1s−−14N核态的14N中的Ξ−捕获事件重新分配为Ξ1p0−14C核态。当核物质密度ρ0=0.17 fm−3时,VoptΞ(ρ)的深度为−VoptΞ(ρ0)≈21 MeV。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Compatibility of recent Ξ-nuclear bound state signals
J-PARC E05 reported recently a hint of a Ξ11B nuclear state in the C12(K,K+)Ξ12Be spectrum, bound by BΞ=8.9±1.43.1+3.8 MeV. Using a density-dependent Ξ-nuclear optical potential VoptΞ(ρ) we explore to what extent a Ξ1s assignment of this nuclear state is compatible with Ξ1s and Ξ1p nuclear-state interpretations of Ξ capture events in light emulsion-nuclei experiments. We find that the only acceptable Ξ1s assignment at present, barring an abnormally strong repulsive ρ2 component of VoptΞ(ρ), is that for the Ξ11B signal. This finding supports reassigning Ξ capture events in 14N, originally assigned as Ξ1s14N nuclear states, to Ξ1p014C nuclear states. The depth of VoptΞ(ρ) at nuclear-matter density ρ0=0.17 fm−3 is then VoptΞ(ρ0)21 MeV.
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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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