@misc{10481/58773,
year = {2018},
url = {http://hdl.handle.net/10481/58773},
abstract = {We present a systematic study on the influence of spatial correlations between the proton constituents, in our case
gluonic hot spots, their size and their number on the symmetric cumulant SC(2, 3), at the eccentricity level, within a
Monte Carlo Glauber framework [1]. When modeling the proton as composed by 3 gluonic hot spots, the most common
assumption in the literature, we find that the inclusion of spatial correlations is indispensable to reproduce the negative
sign of SC(2, 3) in the highest centrality bins as dictated by data. Further, the subtle interplay between the different
scales of the problem is discussed. To conclude, the possibility of feeding a 2+1D viscous hydrodynamic simulation
with our entropy profiles is exposed.},
organization = {This work was partially supported by a Helmholtz Young Investigator Group VH-NG-822 from the
Helmholtz Association and GSI, a FP7-PEOPLE-2013-CIG Grant of the European Commission, reference
QCDense/ 631558, by Ramón y Cajal and MINECO projects reference RYC-2011-09010 and FPA2013-
47836 and by the DFG through the grant CRC-TR 211. HN is supported by the Academy of Finland,
project 297058.},
publisher = {Elsevier BV},
keywords = {Initial state},
keywords = {Small systems},
keywords = {Hot spots},
keywords = {Correlations},
keywords = {Elliptic flow},
title = {Correlated gluonic hot spots meet symmetric cumulants data at LHC energies},
doi = {10.1016/j.nuclphysa.2018.08.013},
author = {López Albacete, Javier and Niemi, Harri and Petersen, Hannah and Soto-Ontoso, Alba},
}