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These results are calculations done with a parameterized energy loss model BBMG on top of an event-by-event relativistic viscous hydrodynamic model mckln+v-USPhydro.

The models is v-USPhydro+BBMG Phys.Rev.Lett. 116 (2016) no.25, 252301 and the predictions for 5.02 TeV for RAA and flow are from arXiv:1609.05171

BBMG was formulated in B. Betz, M. Gyulassy and G. Torrieri, Phys. Rev. C 84, 024913 (2011) doi:10.1103/PhysRevC.84.024913 [arXiv:1102.5416[nucl-th]]. B. Betz and M. Gyulassy, Phys. Rev. C 86, 024903 (2012) doi:10.1103/PhysRevC.86.024903 [arXiv:1201.0281 [nucl-th]]. B. Betz and M. Gyulassy, JHEP 1408, 090 (2014) Erratum: [JHEP 1410, 043 (2014)] doi:10.1007/JHEP10(2014)043, 10.1007/JHEP08(2014)090 [arXiv:1404.6378 [hep-ph]].

mckln H.-J. Drescher and Y. Nara, Phys. Rev. C 75, 034905 (2007) doi:10.1103/PhysRevC.75.034905 [nucl-th/0611017].

v-USPhydro J. Noronha-Hostler et al, Phys. Rev. C88, 044916 (2013); Phys. Rev. C90, 034907 (2014)

We make predictions for the RAA, multiparticle cumulants, and symmetric cummulants.