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Title: Anisotropic Flow in the Forward Directions

Conference ·
OSTI ID:822861

The STAR Forward TPCs (FTPCs) extend the STAR acceptance for charged particles into the region 2.5 < |eta| < 4.0. We see the first signal of directed flow (v{sub 1}) at RHIC energies. While v{sub 1} is consistent with zero in the central rapidity region it rises up to 2 percent at pseudorapidities of +-4. With this signal we can verify that elliptic flow (v{sub 2}) is in-plane. The measurement of v{sub 2} in the FTPCs confirms the falloff by a factor of about 2 compared to mid-rapidity previously seen by PHOBOS [1]. In addition we look for higher harmonics (v{sub n}, n>2) where in the case of v{sub 4} a signal is seen in the STAR TPC. With the available statistics for the FTPCs we give an upper limit for these harmonics, since the results agree with zero within the errors. However, the falloff of v{sub 4} from mid-rapidity to forward-rapidities appears to be faster than for v{sub 2}.[1] B.B. Back. Phys. Rev. Lett. 89, 222301 (2002)

Research Organization:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Organization:
USDOE Director. Office of Science. Nuclear Physics (US)
DOE Contract Number:
AC03-76SF00098
OSTI ID:
822861
Report Number(s):
LBNL-54700; R&D Project: NRNC; TRN: US0401437
Resource Relation:
Conference: Quark Matter 2004, Oakland, CA (US), 01/11/2004--01/17/2004; Other Information: PBD: 9 Mar 2004
Country of Publication:
United States
Language:
English