2020/10/20 by Yi-An Li, Song Zhang, Y. G. +1
Chemistry · Physics and Astronomy · #Atomic physics #Center (category theory) #Chemistry #Cluster (spacecraft) #Computer science #Crystallography #Energy (signal processing) #High-Energy Particle Collisions Research #Nuclear physics #Nuclear physics research studies #Particle physics #Physics #Quantum Chromodynamics and Particle Interactions #Quantum mechanics #hep-ph #nucl-ex #nucl-th
paper · pdf · doi:10.1103/physrevc.102.054907
published as Phys. Rev. C 102, 054907 (2020) · 9 pages, 4 figures; accepted version of Physical Review C
arxiv created 2020/10/20 · openalex created_date 2020/10/29 · openalex publication_date 2020/11/11 · arxiv updated 2020/11/18 · openalex updated_date 2026/08/05
\ensuremathα-clustered structures in light nuclei could be studied through ``snapshots'' taken by relativistic heavy-ion collisions. A multiphase transport model is employed to simulate the initial structure of collision nuclei and the proceeding collisions at center of mass energy √sNN=6.37 TeV. This initial structure can finally be reflected in the subsequent observations, such as elliptic flow (v2), triangular flow (v3), and quadrangular flow (v4). Three sets of the collision systems are chosen to illustrate that the system scan is a good way to identify the exotic \ensuremathα-clustered nuclear structure: case I, 16O nucleus (with or without \ensuremathα-cluster) + ordinary nuclei (always in Woods-Saxon distribution) in most central collisions; case II, 16O nucleus (with or without \ensuremathα-cluster) + 197Au nucleus collisions for centrality dependence; and case III, symmetric collision systems [namely, 10B + 10B, 12C + 12C, 16O + 16O (with or without \ensuremathα-cluster), 20Ne + 20Ne, and 40Ca + 40Ca] in most central collisions. Our calculations propose that relativistic heavy-ion collision experiments at √sNN=6.37 TeV are promised to distinguish the tetrahedral structure of 16O from the Woods-Saxon one and shed light on the system scan projects in experiments.