Evolution of the longitudinal and azimuthal structure of the near-side jet peak in Pb-Pb collisions at √sNN = 2.76 TeV
ALICE Collaboration. (2017). Evolution of the longitudinal and azimuthal structure of the near-side jet peak in Pb-Pb collisions at √sNN = 2.76 TeV. Physical Review C, 96(3), Article 034904. https://doi.org/10.1103/PhysRevC.96.034904
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2017Copyright
© 2017 CERN, for the ALICE Collaboration. Published by the American Physical Society under the terms of the
Creative Commons Attribution 3.0 License.
In two-particle angular correlation measurements, jets give rise to a near-side peak, formed by particles
associated to a higher-pT trigger particle. Measurements of these correlations as a function of pseudorapidity
(η) and azimuthal (ϕ) differences are used to extract the centrality and pT dependence of the shape of the
near-side peak in the pT range 1 < pT < 8 GeV/c in Pb-Pb and pp collisions at √sNN = 2.76 TeV. A combined
fit of the near-side peak and long-range correlations is applied to the data and the peak shape is quantified by
the variance of the distributions. While the width of the peak in the ϕ direction is almost independent of
centrality, a significant broadening in the η direction is found from peripheral to central collisions. This feature
is prominent for the low-pT region and vanishes above 4 GeV/c. The widths measured in peripheral collisions
are equal to those in pp collisions in the ϕ direction and above 3 GeV/c in the η direction. Furthermore, for
the 10% most central collisions and 1 < pT,assoc < 2 GeV/c, 1 < pT,trig < 3 GeV/c, a departure from a Gaussian
shape is found: a depletion develops around the center of the peak. The results are compared to A Multi-Phase
Transport (AMPT) model simulation as well as other theoretical calculations indicating that the broadening and
the development of the depletion are connected to the strength of radial and longitudinal flow.
...
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Except where otherwise noted, this item's license is described as © 2017 CERN, for the ALICE Collaboration. Published by the American Physical Society under the terms of the
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