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  4. Measurement of higher-order harmonic azimuthal anisotropy in PbPb collisions at √s[subscript NN] = 2.76 TeV

Measurement of higher-order harmonic azimuthal anisotropy in PbPb collisions at √s[subscript NN] = 2.76 TeV

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Author(s)
Apyan, Aram
•
Busza, Wit
•
Cali, Ivan Amos
•
Chan, M.
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Di Matteo, Leonardo
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Gomez-Ceballos, Guillelmo
•
Goncharov, Maxim
•
Gulhan, Doga Can
•
Klute, Markus
•
Lai, Yue Shi
more
Date Issued
April 2014
Journal
Physical Review C
Publisher
American Physical Society
Citation
Chatrchyan, S., V. Khachatryan, A. M. Sirunyan, A. Tumasyan, W. Adam, T. Bergauer, M. Dragicevic, et al. “Measurement of Higher-Order Harmonic Azimuthal Anisotropy in PbPb Collisions at √s[subscript NN] = 2.76 TeV.” Phys. Rev. C 89, no. 4 (April 2014). © 2014 CERN, for the CMS Collaboration
Version
Final published version
Abstract
Measurements are presented by the CMS Collaboration at the Large Hadron Collider (LHC) of the higher-order harmonic coefficients that describe the azimuthal anisotropy of charged particles emitted in √s[subscript NN] = 2.76 TeV PbPb collisions. Expressed in terms of the Fourier components of the azimuthal distribution, the n = 3–6 harmonic coefficients are presented for charged particles as a function of their transverse momentum (0.3 < p[subscript T] <8.0GeV/c), collision centrality (0%–70%), and pseudorapidity (|η| < 2.0). The data are analyzed using the event plane, multiparticle cumulant, and Lee-Yang zeros methods, which provide different sensitivities to initial-state fluctuations. Taken together with earlier LHC measurements of elliptic flow (n = 2), the results on higher-order harmonic coefficients develop a more complete picture of the collective motion in high-energy heavy-ion collisions and shed light on the properties of the produced medium.
MIT Department
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Laboratory for Nuclear Science
Massachusetts Institute of Technology. School of Science
Terms of Use
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
http://hdl.handle.net/1721.1/88935
DOI of Published Version
https://doi.org/10.1103/PhysRevC.89.044906
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