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  Beam Energy Dependence of Jet-Quenching Effects in Au+Au Collisions at sqrt{s_NN} = 7.7, 11.5, 14.5, 19.6, 27, 39, and 62.4 GeV

STAR Collaboration, Adamczyk, L., Schmitz, N., Seyboth, P., & et al. (2018). Beam Energy Dependence of Jet-Quenching Effects in Au+Au Collisions at sqrt{s_NN} = 7.7, 11.5, 14.5, 19.6, 27, 39, and 62.4 GeV. Physical Review Letters, (121), 032301. Retrieved from https://publications.mppmu.mpg.de/?action=search&mpi=MPP-2018-317.

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STAR Collaboration1, Autor
Adamczyk, L.1, Autor
Schmitz, N.1, Autor
Seyboth, P.1, Autor
et al.1, Autor
Affiliations:
1Max Planck Institute for Physics, Max Planck Society and Cooperation Partners, ou_2253650              

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Schlagwörter: STAR
 Zusammenfassung: We report measurements of the nuclear modification factor, $R_{ \mathrm{CP}}$, for charged hadrons as well as identified $π^{+(-)}$, $K^{+(-)}$, and $p(\overline{p})$ for Au+Au collision energies of $\sqrt{s_{_{ \mathrm{NN}}}}$ = 7.7, 11.5, 14.5, 19.6, 27, 39, and 62.4 GeV. We observe a clear high-$p_{\mathrm{T}}$ net suppression in central collisions at 62.4 GeV for charged hadrons which evolves smoothly to a large net enhancement at lower energies. This trend is driven by the evolution of the pion spectra, but is also very similar for the kaon spectra. While the magnitude of the proton $R_{ \mathrm{CP}}$ at high $p_{\mathrm{T}}$ does depend on collision energy, neither the proton nor the anti-proton $R_{ \mathrm{CP}}$ at high $p_{\mathrm{T}}$ exhibit net suppression at any energy. A study of how the binary collision scaled high-$p_{\mathrm{T}}$ yield evolves with centrality reveals a non-monotonic shape that is consistent with the idea that jet-quenching is increasing faster than the combined phenomena that lead to enhancement.

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 Datum: 2018
 Publikationsstatus: Erschienen
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Titel: Physical Review Letters
  Alternativer Titel : Phys.Rev.Lett.
Genre der Quelle: Zeitschrift
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Seiten: - Band / Heft: (121) Artikelnummer: - Start- / Endseite: 032301 Identifikator: -