{"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}
引用次数: 0
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 $$ \gamma +\gamma \to {\Xi}_{cc}+\overline{c}+\overline{c} $$ 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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