2016
DOI: 10.1140/epjc/s10052-016-4130-9
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Origins of the di-jet asymmetry in heavy-ion collisions

Abstract: The di-jet asymmetry-the measure of the momentum imbalance in a di-jet system-is a key jet quenching observable. Using the event generator Jewel we show that the di-jet asymmetry is dominated by fluctuations both in proton-proton and in heavy-ion collisions. We discuss how in proton-proton collisions the asymmetry is generated through recoil and out-of-cone radiation. In heavy-ion collisions two additional sources can contribute to the asymmetry, namely energy loss fluctuations and differences in path length. … Show more

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Cited by 101 publications
(102 citation statements)
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“…This is a consequence of the fact that wider jets typically contain more, and less hard, partonic fragments and lose more energy than narrower jets with the same energy. The same phenomenon has been observed in calculations of jet quenching that are entirely done at strong coupling [145,147] and in Monte Carlo calculations of radiative energy loss that are entirely done at weak coupling [105]. We find that this observation leads to two unexpected consequences.…”
Section: Jhep03(2017)135supporting
confidence: 80%
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“…This is a consequence of the fact that wider jets typically contain more, and less hard, partonic fragments and lose more energy than narrower jets with the same energy. The same phenomenon has been observed in calculations of jet quenching that are entirely done at strong coupling [145,147] and in Monte Carlo calculations of radiative energy loss that are entirely done at weak coupling [105]. We find that this observation leads to two unexpected consequences.…”
Section: Jhep03(2017)135supporting
confidence: 80%
“…Because of the steeply falling spectrum, there are not many jets that originate with higher energies, lose energy, and end up in the given energy bin. The result is a narrowing of jets that remain in a given energy bin, something that has been seen previously in both perturbative [105] and holographic [145,147] analyses. And, we see from the K = 0 results in figure 4 that narrower dijets are less acoplanar.…”
Section: Jhep03(2017)135supporting
confidence: 61%
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“…In a back-to-back dijet pair propagating through the QGP, the sub-leading jet has typically lost more energy than its leading partner [56]. This quenching asymmetry can be combined with ΔS 12 to experimentally further constrain the nature of jet quenching.…”
Section: Subjets In Dijet Pairsmentioning
confidence: 99%