2017
DOI: 10.1103/physrevlett.118.212301
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Measurement of D0 Azimuthal Anisotropy at Midrapidity in Au+Au Collisions at

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Cited by 116 publications
(67 citation statements)
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“…Compared to CMS data, the calibrated model reproduces the transverse momentum and centrality dependence of Dmeson v 3 very well. In the last two columns of Figure 12, we again apply the model to the RHIC data and observe a good agreement with STAR measured v 2 of D 0 -mesons [64].…”
Section: Validation and Predictionssupporting
confidence: 59%
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“…Compared to CMS data, the calibrated model reproduces the transverse momentum and centrality dependence of Dmeson v 3 very well. In the last two columns of Figure 12, we again apply the model to the RHIC data and observe a good agreement with STAR measured v 2 of D 0 -mesons [64].…”
Section: Validation and Predictionssupporting
confidence: 59%
“…Calculation of heavy-flavor flows with a high likelihood parameter set. Results are compared to CMS D-meson measurements in Pb+Pb[59] and STAR D-meson measurements in Au+Au[64]. D-meson v3 and B-meson v2, v3 are predictions.…”
mentioning
confidence: 99%
“…In figure 8 we display the POWLANG predictions for the elliptic flow of charm quarks and hadrons in Au-Au collisions at √ s NN = 200 GeV in the 0-80% centrality class, comparing our results to STAR measurements of the D 0 meson v 2 [6]. In a previous publication [11] we already showed how the flow inherited from the light thermal partons at hadronization JHEP02 (2018) Figure 9.…”
Section: Model Results Versus Experimental Datamentioning
confidence: 77%
“…Experimental measurements of charm and beauty production in relativistic heavy-ion collisions are a major tool to get information on the properties of the (deconfined, if a sufficiently high energy-density is achieved) medium formed in these events, in particular on the heavy-flavour transport coefficients [1][2][3][4][5][6][7]. At high momentum the major effect of the interaction with the medium is a quenching of the heavy-quark momentum spectra due to parton energy-loss: this provides information on the medium opacity [2,4].…”
Section: Introductionmentioning
confidence: 99%
“…These operators were computed in [2,3]; we give the explicit expressions of ρ, H, and the C n in the following Eqs. (11) and (23) to (25) in Section III. The operators H and C n turn out to depend on only two transport coefficients, κ and γ, that encode the entire in medium dynamics.…”
Section: A Heavy Quarkonia Via Lindblad Equation: κ and γmentioning
confidence: 99%