2011
DOI: 10.1103/physrevlett.107.052303
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Chiral Magnetic Wave at Finite Baryon Density and the Electric Quadrupole Moment of the Quark-Gluon Plasma

Abstract: The chiral magnetic wave is a gapless collective excitation of quark-gluon plasma in the presence of an external magnetic field that stems from the interplay of chiral magnetic and chiral separation effects; it is composed of the waves of the electric and chiral charge densities coupled by the axial anomaly. We consider a chiral magnetic wave at finite baryon density and find that it induces the electric quadrupole moment of the quark-gluon plasma produced in heavy ion collisions: the "poles" of the produced f… Show more

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Cited by 285 publications
(355 citation statements)
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References 54 publications
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“…The results are shown in Fig. 2, together with the simulation calculations with UrQMD event generator [23] and with the theoretical calculations with the CMW effect with different duration times for the magnetic field [14]. For most data points, the slopes are positive and reach a maximum in mid-celtral/mid-peripheral collisions.…”
Section: Introductionmentioning
confidence: 83%
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“…The results are shown in Fig. 2, together with the simulation calculations with UrQMD event generator [23] and with the theoretical calculations with the CMW effect with different duration times for the magnetic field [14]. For most data points, the slopes are positive and reach a maximum in mid-celtral/mid-peripheral collisions.…”
Section: Introductionmentioning
confidence: 83%
“…The CMW manifests itself in a finite electric quadrupole moment of the collision system, where the "poles" ("equator") of the produced fireball acquire additional positive (negative) charge [14]. This effect, if realized, will be reflected in the measurement of chargedependent elliptic flow.…”
Section: Introductionmentioning
confidence: 99%
See 1 more Smart Citation
“…for some p T selection and, more importantly, some η acceptance. Indeed, this observable has been proposed theoretically [4] and measured experimentally in Au-Au collisions at √ s NN = 200 GeV by the STAR collaboration [5]. However, one of the issues with this observable is that the slope of v n vs A is not independent of experimental effects (for example tracking efficiency) and therefore requires a correction factor.…”
Section: Methodology and Observablesmentioning
confidence: 99%
“…The lower row of the figure shows the same schematic for the opposite case with µ V < 0, which leads to exactly the same effect with all signs flipped. A detailed explanation and derivation of how the presence of CMW affects the final state observables in this way is given in [4] …”
Section: Introductionmentioning
confidence: 99%