The unexpected uses of a bowling pin: exploiting $^{20}$Ne isotopes for precision characterizations of collectivity in small systems
Giuliano Giacalone, Benjamin Bally, Govert Nijs, Shihang Shen, Thomas, Duguet, Jean-Paul Ebran, Serdar Elhatisari, Mikael Frosini, Timo A. L\"ahde,, Dean Lee, Bing-Nan Lu, Yuan-Zhuo Ma, Ulf-G. Mei{\ss}ner, Jacquelyn, Noronha-Hostler, Christopher Plumberg, Tom\'as R. Rodr\'iguez

TL;DR
This paper explores how collisions of $^{20}$Ne ions, with their bowling-pin shape, can provide new insights into the collective behavior of quark-gluon plasma in small systems, using advanced ab initio models and hydrodynamic simulations.
Contribution
It demonstrates the potential of using $^{20}$Ne collisions alongside $^{16}$O to perform precision tests of the hydrodynamic QGP paradigm in small systems.
Findings
Enhanced elliptic flow in $^{20}$Ne$^{20}$Ne collisions compared to $^{16}$O$^{16}$O.
Theoretical uncertainties cancel out when comparing relative observables between systems.
Method enables precision characterization of collective dynamics in small collision systems.
Abstract
Whether or not femto-scale droplets of quark-gluon plasma (QGP) are formed in so-called small systems at high-energy colliders is a pressing question in the phenomenology of the strong interaction. For proton-proton or proton-nucleus collisions the answer is inconclusive due to the large theoretical uncertainties plaguing the description of these processes. While upcoming data on collisions of O nuclei may mitigate these uncertainties in the near future, here we demonstrate the unique possibilities offered by complementing OO data with collisions of Ne ions. We couple both NLEFT and PGCM ab initio descriptions of the structure of Ne and O to hydrodynamic simulations of OO and NeNe collisions at high energy. We isolate the imprints of the bowling-pin shape of Ne on the collective flow of hadrons, which can be…
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Taxonomy
TopicsHigh-Energy Particle Collisions Research · Stochastic processes and statistical mechanics · Quantum Chromodynamics and Particle Interactions
