Does parton saturation at high density explain hadron multiplicities at RHIC?

Baier R, Mueller AH, Schiff D, Son DT (2002)
PHYSICS LETTERS B 539(1-2): 46-52.

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Zeitschriftenaufsatz | Veröffentlicht | Englisch
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Abstract / Bemerkung
We discuss the recent claim that hadron multiplicities measured at RHIC energies are directly described in terms of gluon degrees of freedom fixed from the initial conditions of central heavy ion collisions. The argument is based on the parton saturation scenario expected to be valid at high parton densities and on the assumption of conserved gluon number. Alternatively we conjecture that "bottom-up" equilibration before hadronization. modifies this picture, due to nonconservation of the number of gluons. (C) 2002 Elsevier Science B.V. All rights reserved.
Erscheinungsjahr
Zeitschriftentitel
PHYSICS LETTERS B
Band
539
Zeitschriftennummer
1-2
Seite
46-52
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Baier R, Mueller AH, Schiff D, Son DT. Does parton saturation at high density explain hadron multiplicities at RHIC? PHYSICS LETTERS B. 2002;539(1-2):46-52.
Baier, R., Mueller, A. H., Schiff, D., & Son, D. T. (2002). Does parton saturation at high density explain hadron multiplicities at RHIC? PHYSICS LETTERS B, 539(1-2), 46-52. doi:10.1016/S0370-2693(02)02037-3
Baier, R., Mueller, A. H., Schiff, D., and Son, D. T. (2002). Does parton saturation at high density explain hadron multiplicities at RHIC? PHYSICS LETTERS B 539, 46-52.
Baier, R., et al., 2002. Does parton saturation at high density explain hadron multiplicities at RHIC? PHYSICS LETTERS B, 539(1-2), p 46-52.
R. Baier, et al., “Does parton saturation at high density explain hadron multiplicities at RHIC?”, PHYSICS LETTERS B, vol. 539, 2002, pp. 46-52.
Baier, R., Mueller, A.H., Schiff, D., Son, D.T.: Does parton saturation at high density explain hadron multiplicities at RHIC? PHYSICS LETTERS B. 539, 46-52 (2002).
Baier, Rudolf, Mueller, AH, Schiff, D, and Son, DT. “Does parton saturation at high density explain hadron multiplicities at RHIC?”. PHYSICS LETTERS B 539.1-2 (2002): 46-52.

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