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Trying to understand the ridge effect in hydrodynamic model · Around

2009

Trying to understand the ridge effect in hydrodynamic model

Hama, Yogiro, Andrade, Rone Peterson G., Grassi, Frederique et al.

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In a recent paper, the hydrodynamic code NeXSPheRIO was used in conjunction with STAR analysis methods to study two-particle correlations as function of Delta_eta and Delta_phi.

Both the ridge-like near-side and the double-hump away-side structures were obtained.
However, the mechanism of ridge production was not clear.
In order to understand it, we study a simple model with only one high-energy density peripheral tube in a smooth cylindrical back-ground, with longitudinal boost invariance.

Built on

Aguiar CE, Kodama T, Osada T and Hama Y, (2001) J Phys G 27
2001
Earlier work this paper cites.
Drescher HJ, Liu FM, Ostapchenko S, Pierog T and Werner K (2002) Phys Rev C 65
2002
Earlier work this paper cites.
Aguiar CE, Hama Y, Kodama T, and Osada T, (2002) Nucl Phys A 698
2002
Earlier work this paper cites.

Similar

Putschke J [for the STAR Collaboration] (2007) Nucl Phys A 783
2007
Cited alongside, same era.
McCumber MP [for the PHENIX Collaboration] (2008) J Phys G 35
2008
Cited alongside, same era.
Li W [for the PHOBOS Collaboration] (2008) J Phys G 35
2008
Cited alongside, same era.
Takahashi J, Tavares BM, Qian WL, Andrade RPG, Grassi F, Hama Y, Kodama T, and Xu N, arXiv:0902.4870
Original
Cited in the paper.
Osada T, Aguiar CE, Hama Y and Kodama T, nucl-th/0102011
Cited in the paper.

Then

PHENIX Collaboration, Adare A., et al. (2008) Phys Rev C 78
2008
Later among the works it cites.
Hama Y, Andrade RPG, Grassi F, Qian WL, Osada T, Aguiar CE, and Kodama T (2008) Phys Atom Nuclei 71
2008
Later among the works it cites.
Feng A [for the STAR Collaboration] (2008) J Phys G 35
2008
Later among the works it cites.

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