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<p>Experiments on collisions of light nuclei at <InlineEquation ID="IEq1"> <EquationSource Format="TEX">\(\sqrt s = 5.36\)</EquationSource> <!--JETPLet2560882Zakharov-m1--> </InlineEquation> TeV have recently begun at the LHC. In this regard we make predictions for nuclear modification factor <InlineEquation ID="IEq2"> <EquationSource Format="TEX">\({{R}_{{AA}}}\)</EquationSource> <!--JETPLet2560882Zakharov-m2--> </InlineEquation> in 5.36 TeV C + C, O + O, and Ne + Ne collisions for scenarios with and without quark–gluon plasma formation in <InlineEquation ID="IEq3"> <EquationSource Format="TEX">\(pp\)</EquationSource> <!--JETPLet2560882Zakharov-m3--> </InlineEquation> collisions. We find a sizeable difference in <InlineEquation ID="IEq4"> <EquationSource Format="TEX">\({{R}_{{AA}}}\)</EquationSource> <!--JETPLet2560882Zakharov-m4--> </InlineEquation> for these two scenarios, which grows with decreasing atomic number. This says that data on <InlineEquation ID="IEq5"> <EquationSource Format="TEX">\({{R}_{{AA}}}\)</EquationSource> <!--JETPLet2560882Zakharov-m5--> </InlineEquation> for light nuclei could potentially give information on the presence of jet quenching in <InlineEquation ID="IEq6"> <EquationSource Format="TEX">\(pp\)</EquationSource> <!--JETPLet2560882Zakharov-m6--> </InlineEquation> collisions.</p>

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Predictions for RAA in 5.36 TeV C + C, O + O, and Ne + Ne Collisions at the LHC

  • 期刊论文

  • 发表日期：

    2025年10月13日

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  • B. G. Zakharov

摘要

Experiments on collisions of light nuclei at \(\sqrt s = 5.36\) TeV have recently begun at the LHC. In this regard we make predictions for nuclear modification factor \({{R}_{{AA}}}\) in 5.36 TeV C + C, O + O, and Ne + Ne collisions for scenarios with and without quark–gluon plasma formation in \(pp\) collisions. We find a sizeable difference in \({{R}_{{AA}}}\) for these two scenarios, which grows with decreasing atomic number. This says that data on \({{R}_{{AA}}}\) for light nuclei could potentially give information on the presence of jet quenching in \(pp\) collisions.