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Rotating quark-gluon plasma in relativistic heavy ion collisions (1602.06580v2)

Published 21 Feb 2016 in hep-ph and nucl-th

Abstract: We study the rotational collective motion of the quark-gluon plasma in relativistic heavy ion collisions using the widely-adopted AMPT (A Multi-Phase Transport) model. The global angular momentum, the average vorticity carried by the quark-gluon plasma, and the locally defined vorticity fields are computed for Au+Au collisions, with detailed information of their time evolution, spatial distribution, as well as the dependence on beam energy and collision centrality.

Citations (168)

Summary

Rotating Quark-Gluon Plasma in Relativistic Heavy Ion Collisions

The paper conducted on the rotational collective motion of quark-gluon plasma (QGP) in relativistic heavy ion collisions offers valuable insight into the rotational dynamics of such collisions. Utilizing the AMPT (A Multi-Phase Transport) model, the authors undertake a thorough analysis of the angular momentum and vorticity characteristics of the QGP produced in non-central heavy-ion collisions. The focus is on collisions involving gold nuclei (Au+Au) across varying parameters such as beam energy and collision centrality.

Overview of Key Concepts

In non-central heavy ion collisions, a significant amount of angular momentum is present, which is primarily carried by the "spectators", the non-interacting nucleons. However, a notable portion is retained within the QGP, manifesting as rotational motion. This retained angular momentum is pivotal for understanding the global rotation of the QGP, and its quantification is essential due to its potential to induce observable effects, such as hadron spin polarization and various chiral phenomena including the Chiral Vortical Effect (CVE).

Angular Momentum Analysis

The research identifies the primary axis of rotation for the QGP as being perpendicular to the reaction plane (y-axis), which is consistent across different beam energies and collision centralities. The analysis shows that the QGP retains approximately 10-20% of the total angular momentum of the colliding system, attributed primarily to the nontrivial spatial distribution and dynamics of the QGP. An intriguing result is the non-monotonic dependence of the angular momentum on the impact parameter, where a peak is observed due to the interplay between the size of the overlap region and the geometry of the collision zone.

Vorticity Distribution and Implications

The local vorticity distribution shows complex patterns that are significantly influenced by the underlying radial flow within the QGP. Computations using the non-relativistic definition of vorticity, along with sensitivity analysis over different volumes and weighting functions, help to isolate the component of vorticity genuinely associated with global rotation. The paper reveals a systematic dependence of the average vorticity on the impact parameter and beam energy, highlighting an increase in vorticity with more peripheral collisions and a decrease with higher beam energies, pointing to a possible constraint on the initial conditions of such collisions.

Future Directions and Implications

The results from this research underscore the necessity for a comprehensive understanding of vorticity and its implications for experimental observables. The quantification of rotational effects is crucial for interpreting signals related to chiral magnetic and vortical phenomena in experimental settings. These findings point towards future experiments and simulations designed to measure direct consequences of these rotational dynamics, such as spin polarization observables and baryon separation in different collision configurations.

This paper exemplifies a rigorous quantitative approach to understanding the rotational aspects of QGP dynamics, offering a foundational framework for further exploration and a benchmark for interpreting experimental data in high-energy nuclear physics. Future investigations could explore the impact of different initial conditions, medium responses, and the role of magnetic fields in such rotational phenomena, advancing our understanding of the QGP's complex nature.

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