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Jet substructure in p+p and p+Au collisions at $\sqrt{s_\mathrm{NN}}$ = 200 GeV at STAR
<!--HTML-->In order to attribute the partonic energy loss within jets (jet quenching) observed in A+A collisions to the traversal of partons through the hot QCD medium, it is necessary to examine cold nuclear matter (CNM) effects on the corresponding jets. Such examination has historically bee...
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Lenguaje: | eng |
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2020
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Acceso en línea: | http://cds.cern.ch/record/2722153 |