4.5 Article

Third harmonic flow of charged particles in Au plus Au collisions at √sNN=200 GeV

期刊

PHYSICAL REVIEW C
卷 88, 期 1, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevC.88.014904

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资金

  1. RHIC Operations Group at BNL
  2. RCF at BNL
  3. NERSC Center at LBNL
  4. Open Science Grid consortium
  5. Offices of NP and HEP within the US DOE Office of Science
  6. US NSF
  7. Sloan Foundation
  8. CNRS/IN2P3
  9. FAPESP CNPq of Brazil
  10. Ministry of Education and Science of the Russian Federation
  11. NNSFC
  12. CAS
  13. MoST
  14. MoE of China,
  15. GA
  16. MSMT of the Czech Republic
  17. FOM
  18. NWO of the Netherlands
  19. DAE
  20. DST
  21. CSIR of India
  22. Polish Ministry of Science and Higher Education
  23. National Research Foundation [NRF-2012004024]
  24. Ministry of Science, Education and Sports of the Republic of Croatia
  25. RosAtom of Russia

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We report measurements of the third harmonic coefficient of the azimuthal anisotropy, upsilon(3), known as triangular flow. The analysis is for charged particles in Au + Au collisions at root s(NN) = 200 GeV, based on data from the STAR experiment at the BNL Relativistic Heavy Ion Collider. Two-particle correlations as a function of their pseudorapidity separation are fit with narrow and wide Gaussians. Measurements of triangular flow are extracted from the wide Gaussian, from two-particle cumulants with a pseudorapidity gap, and also from event plane analysis methods with a large pseudorapidity gap between the particles and the event plane. These results are reported as a function of transverse momentum and centrality. A large dependence on the pseudorapidity gap is found. Results are compared with other experiments and model calculations.

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