4.5 Article

Identified particle production, azimuthal anisotropy, and interferometry measurements in Au plus Au collisions at √sNN=9.2 GeV

期刊

PHYSICAL REVIEW C
卷 81, 期 2, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevC.81.024911

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资金

  1. Offices of NP
  2. US DOE Office of Science
  3. US NSF
  4. Sloan Foundation
  5. DFG cluster of excellence 'Origin and Structure of the Universe'
  6. RA
  7. RPL
  8. EMN of France
  9. STFC
  10. EPSRC of the United Kingdom
  11. FAPESP of Brazil
  12. Russian Ministry of Sci. and Tech.
  13. NNSFC
  14. CAS
  15. MoST
  16. MoE of China
  17. IRP
  18. GA of the Czech Republic
  19. FOM of the Netherlands
  20. DAE
  21. DST
  22. CSIR of the Government of India
  23. Polish State Committee for Scientific Research
  24. Korea Sci. & Eng. Foundation
  25. Korea Research Foundation
  26. [CNRS/IN2P3]
  27. Science and Technology Facilities Council [PP/F001061/1] Funding Source: researchfish
  28. STFC [PP/F001061/1] Funding Source: UKRI
  29. Division Of Physics
  30. Direct For Mathematical & Physical Scien [0758018] Funding Source: National Science Foundation

向作者/读者索取更多资源

We present the first measurements of identified hadron production, azimuthal anisotropy, and pion interferometry from Au + Au collisions below the nominal injection energy at the BNL Relativistic Heavy-Ion Collider (RHIC) facility. The data were collected using the large acceptance solenoidal tracker at RHIC (STAR) detector at root s(NN) = 9.2 GeV from a test run of the collider in the year 2008. Midrapidity results on multiplicity density dN/dy in rapidity y, average transverse momentum < p(T)>, particle ratios, elliptic flow, and Hanbury-Brown-Twiss (HBT) radii are consistent with the corresponding results at similar root s(NN) from fixed-target experiments. Directed flow measurements are presented for both midrapidity and forward-rapidity regions. Furthermore the collision centrality dependence of identified particle dN/dy, < p(T)>, and particle ratios are discussed. These results also demonstrate that the capabilities of the STAR detector, although optimized for root s(NN) = 200 GeV, are suitable for the proposed QCD critical-point search and exploration of the QCD phase diagram at RHIC.

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