{"title":"未来e+e -对撞机p波双粲重子的光产生","authors":"Xi-Jie Zhan, Xing-Gang Wu, Xu-Chang Zheng","doi":"10.1007/jhep11(2023)029","DOIUrl":null,"url":null,"abstract":"A bstract The photoproduction of P -wave doubly charmed baryon (Ξ cc ) is investigated in the context of future high-energy and high-luminosity e + e − colliders. The direct photoproduction via the sub-process $$ \\gamma +\\gamma \\to {\\Xi}_{cc}+\\overline{c}+\\overline{c} $$ <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\"> <mml:mi>γ</mml:mi> <mml:mo>+</mml:mo> <mml:mi>γ</mml:mi> <mml:mo>→</mml:mo> <mml:msub> <mml:mi>Ξ</mml:mi> <mml:mi>cc</mml:mi> </mml:msub> <mml:mo>+</mml:mo> <mml:mover> <mml:mi>c</mml:mi> <mml:mo>¯</mml:mo> </mml:mover> <mml:mo>+</mml:mo> <mml:mover> <mml:mi>c</mml:mi> <mml:mo>¯</mml:mo> </mml:mover> </mml:math> and the resolved channel $$ \\gamma +g\\to {\\Xi}_{cc}+\\overline{c}+\\overline{c} $$ <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\"> <mml:mi>γ</mml:mi> <mml:mo>+</mml:mo> <mml:mi>g</mml:mi> <mml:mo>→</mml:mo> <mml:msub> <mml:mi>Ξ</mml:mi> <mml:mi>cc</mml:mi> </mml:msub> <mml:mo>+</mml:mo> <mml:mover> <mml:mi>c</mml:mi> <mml:mo>¯</mml:mo> </mml:mover> <mml:mo>+</mml:mo> <mml:mover> <mml:mi>c</mml:mi> <mml:mo>¯</mml:mo> </mml:mover> </mml:math> are considered. Within the framework of non-relativistic QCD, the calculation encompasses four P -wave ( cc )-diquark configurations: $$ {(cc)}_{\\overline{\\textbf{3}}} $$ <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\"> <mml:msub> <mml:mfenced> <mml:mi>cc</mml:mi> </mml:mfenced> <mml:mover> <mml:mn>3</mml:mn> <mml:mo>¯</mml:mo> </mml:mover> </mml:msub> </mml:math> [ 1 P 1 ], ( cc ) 6 [ 3 P 0 ], ( cc ) 6 [ 3 P 1 ] and ( cc ) 6 [ 3 P 2 ]. The two S -wave states, $$ {(cc)}_{\\overline{\\textbf{3}}} $$ <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\"> <mml:msub> <mml:mfenced> <mml:mi>cc</mml:mi> </mml:mfenced> <mml:mover> <mml:mn>3</mml:mn> <mml:mo>¯</mml:mo> </mml:mover> </mml:msub> </mml:math> [ 3 S 1 ] and ( cc ) 6 [ 1 S 0 ], are also included for comparison. The cross sections, as well as the differential distributions involving transverse momentum, rapidity, and angular variables, have been computed. Numerical results reveal that the resolved photoproduction process plays a significant role and can provide dominant contributions. The photoproduction rate of the P -wave Ξ cc is approximately one order of magnitude lower than that of the S -wave.","PeriodicalId":48906,"journal":{"name":"Journal of High Energy Physics","volume":"28 1","pages":"0"},"PeriodicalIF":5.0000,"publicationDate":"2023-11-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Photoproduction of P-wave doubly charmed baryon at future e+e− collider\",\"authors\":\"Xi-Jie Zhan, Xing-Gang Wu, Xu-Chang Zheng\",\"doi\":\"10.1007/jhep11(2023)029\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"A bstract The photoproduction of P -wave doubly charmed baryon (Ξ cc ) is investigated in the context of future high-energy and high-luminosity e + e − colliders. The direct photoproduction via the sub-process $$ \\\\gamma +\\\\gamma \\\\to {\\\\Xi}_{cc}+\\\\overline{c}+\\\\overline{c} $$ <mml:math xmlns:mml=\\\"http://www.w3.org/1998/Math/MathML\\\"> <mml:mi>γ</mml:mi> <mml:mo>+</mml:mo> <mml:mi>γ</mml:mi> <mml:mo>→</mml:mo> <mml:msub> <mml:mi>Ξ</mml:mi> <mml:mi>cc</mml:mi> </mml:msub> <mml:mo>+</mml:mo> <mml:mover> <mml:mi>c</mml:mi> <mml:mo>¯</mml:mo> </mml:mover> <mml:mo>+</mml:mo> <mml:mover> <mml:mi>c</mml:mi> <mml:mo>¯</mml:mo> </mml:mover> </mml:math> and the resolved channel $$ \\\\gamma +g\\\\to {\\\\Xi}_{cc}+\\\\overline{c}+\\\\overline{c} $$ <mml:math xmlns:mml=\\\"http://www.w3.org/1998/Math/MathML\\\"> <mml:mi>γ</mml:mi> <mml:mo>+</mml:mo> <mml:mi>g</mml:mi> <mml:mo>→</mml:mo> <mml:msub> <mml:mi>Ξ</mml:mi> <mml:mi>cc</mml:mi> </mml:msub> <mml:mo>+</mml:mo> <mml:mover> <mml:mi>c</mml:mi> <mml:mo>¯</mml:mo> </mml:mover> <mml:mo>+</mml:mo> <mml:mover> <mml:mi>c</mml:mi> <mml:mo>¯</mml:mo> </mml:mover> </mml:math> are considered. Within the framework of non-relativistic QCD, the calculation encompasses four P -wave ( cc )-diquark configurations: $$ {(cc)}_{\\\\overline{\\\\textbf{3}}} $$ <mml:math xmlns:mml=\\\"http://www.w3.org/1998/Math/MathML\\\"> <mml:msub> <mml:mfenced> <mml:mi>cc</mml:mi> </mml:mfenced> <mml:mover> <mml:mn>3</mml:mn> <mml:mo>¯</mml:mo> </mml:mover> </mml:msub> </mml:math> [ 1 P 1 ], ( cc ) 6 [ 3 P 0 ], ( cc ) 6 [ 3 P 1 ] and ( cc ) 6 [ 3 P 2 ]. The two S -wave states, $$ {(cc)}_{\\\\overline{\\\\textbf{3}}} $$ <mml:math xmlns:mml=\\\"http://www.w3.org/1998/Math/MathML\\\"> <mml:msub> <mml:mfenced> <mml:mi>cc</mml:mi> </mml:mfenced> <mml:mover> <mml:mn>3</mml:mn> <mml:mo>¯</mml:mo> </mml:mover> </mml:msub> </mml:math> [ 3 S 1 ] and ( cc ) 6 [ 1 S 0 ], are also included for comparison. The cross sections, as well as the differential distributions involving transverse momentum, rapidity, and angular variables, have been computed. Numerical results reveal that the resolved photoproduction process plays a significant role and can provide dominant contributions. The photoproduction rate of the P -wave Ξ cc is approximately one order of magnitude lower than that of the S -wave.\",\"PeriodicalId\":48906,\"journal\":{\"name\":\"Journal of High Energy Physics\",\"volume\":\"28 1\",\"pages\":\"0\"},\"PeriodicalIF\":5.0000,\"publicationDate\":\"2023-11-06\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of High Energy Physics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1007/jhep11(2023)029\",\"RegionNum\":1,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q1\",\"JCRName\":\"PHYSICS, PARTICLES & FIELDS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of High Energy Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1007/jhep11(2023)029","RegionNum":1,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"PHYSICS, PARTICLES & FIELDS","Score":null,"Total":0}
引用次数: 0
摘要
在未来高能高亮度e + e−对撞机的背景下,研究了P波双粲重子(Ξ cc)的光产生。考虑了通过子过程$$ \gamma +\gamma \to {\Xi}_{cc}+\overline{c}+\overline{c} $$ γ + γ→Ξ cc + c¯+ c¯和解析通道$$ \gamma +g\to {\Xi}_{cc}+\overline{c}+\overline{c} $$ γ + g→Ξ cc + c¯+ c¯的直接光生产。在非相对论性QCD的框架内,计算包括四种P波(cc)-双夸克构型:$$ {(cc)}_{\overline{\textbf{3}}} $$ cc 3¯[1 p1], (cc) 6 [3 p1], (cc) 6 [3 p2]和(cc) 6 [3 p2]。两种S波状态,$$ {(cc)}_{\overline{\textbf{3}}} $$ cc 3¯[3 S 1]和(cc) 6 [1 S 0],也包括在其中进行比较。横截面,以及微分分布涉及横向动量,速度,和角变量,已经计算。数值结果表明,分辨光产生过程起着重要的作用,可以提供主导的贡献。P波Ξ cc的光产生率比S波的光产生率大约低一个数量级。
Photoproduction of P-wave doubly charmed baryon at future e+e− collider
A bstract The photoproduction of P -wave doubly charmed baryon (Ξ cc ) is investigated in the context of future high-energy and high-luminosity e + e − colliders. The direct photoproduction via the sub-process $$ \gamma +\gamma \to {\Xi}_{cc}+\overline{c}+\overline{c} $$ γ+γ→Ξcc+c¯+c¯ and the resolved channel $$ \gamma +g\to {\Xi}_{cc}+\overline{c}+\overline{c} $$ γ+g→Ξcc+c¯+c¯ are considered. Within the framework of non-relativistic QCD, the calculation encompasses four P -wave ( cc )-diquark configurations: $$ {(cc)}_{\overline{\textbf{3}}} $$ cc3¯ [ 1 P 1 ], ( cc ) 6 [ 3 P 0 ], ( cc ) 6 [ 3 P 1 ] and ( cc ) 6 [ 3 P 2 ]. The two S -wave states, $$ {(cc)}_{\overline{\textbf{3}}} $$ cc3¯ [ 3 S 1 ] and ( cc ) 6 [ 1 S 0 ], are also included for comparison. The cross sections, as well as the differential distributions involving transverse momentum, rapidity, and angular variables, have been computed. Numerical results reveal that the resolved photoproduction process plays a significant role and can provide dominant contributions. The photoproduction rate of the P -wave Ξ cc is approximately one order of magnitude lower than that of the S -wave.
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