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Title: Jet quenching and azimuthal anisotropy of large p{sub T} spectra in noncentral high-energy heavy-ion collisions

Journal Article · · Physical Review C

Parton energy loss inside a dense medium leads to the suppression of large p{sub T} hadrons and can also cause azimuthal anisotropy of hadron spectra at large transverse momentum in noncentral high-energy heavy-ion collisions. Such azimuthal anisotropy is studied qualitatively in a parton model for heavy-ion collisions at RHIC energies. The coefficient v{sub 2}(p{sub T}) of the elliptic anisotropy at large p{sub T} is found to be very sensitive to parton energy loss. It decreases slowly with p{sub T} contrary to its low p{sub T} behavior where v{sub 2} increases very rapidly with p{sub T}. The turning point signals the onset of contributions of hard processes and the magnitude of parton energy loss. The centrality dependence of v{sub 2}(p{sub T}) is shown to be sensitive to both size and density dependence of the parton energy loss and the latter can also be studied via variation of the colliding energy. The anisotropy coefficient v{sub 2}/{epsilon} normalized by the spatial ellipticity {epsilon} is found to decrease significantly toward semiperipheral collisions, differing from the hydrodynamic results for low p{sub T} hadrons. Constrained by the existing WA98 experimental data at the SPS energy on parton energy loss, both hadron spectra suppression and azimuthal anisotropy at high p{sub T} are predicted to vanish for b>7--8 fm in Au+Au collisions at s=130-200 GeV when the hadron rapidity density per unit area of the initial overlapped region is less than what is achieved in the central Pb+Pb collisions at the SPS energy.

Sponsoring Organization:
(US)
OSTI ID:
40206193
Journal Information:
Physical Review C, Vol. 63, Issue 5; Other Information: DOI: 10.1103/PhysRevC.63.054902; Othernumber: PRVCAN000063000005054902000001; 013105PRC; PBD: May 2001; ISSN 0556-2813
Publisher:
The American Physical Society
Country of Publication:
United States
Language:
English

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