Understanding the energy dependence of $B_2$ in heavy ion collisions: Interplay of volume and space-momentum correlations

TL;DR

This study investigates how the deuteron coalescence parameter $B_2$ varies with collision energy in heavy ion collisions, revealing a transition from volume-dominated suppression at low energies to flow-driven saturation at high energies.

Contribution

It combines UrQMD transport simulations with phase space coalescence modeling to explain the energy dependence of $B_2$, highlighting the role of radial flow and space-momentum correlations.

Findings

$B_2$ decreases with energy below 20 GeV due to volume effects.

$B_2$ saturates at high energies because of strong radial flow.

Radial flow induces space-momentum correlations that offset volume suppression.

Abstract

The deuteron coalescence parameter $B_2$ in proton+proton and nucleus+nucleus collisions in the energy range of $\sqrt{s_{NN}}=$ 900 - 7000 GeV for proton+proton and $\sqrt{s_{NN}}=$ 2 - 2760 GeV for nucleus+nucleus collisions is analyzed with the Ultrarelativistic Quantum Molecular Dynamics (UrQMD) transport model, supplemented by an event-by-event phase space coalescence model for deuteron and anti-deuteron production. The results are compared to data by the E866, E877, PHENIX, STAR and ALICE experiments. The $B_2$ values are calculated from the final spectra of protons and deuterons. At lower energies, $\sqrt{s_{NN}}\leq 20$ GeV, $B_2$ drops drastically with increasing energy. The calculations confirm that this is due to the increasing freeze-out volume reflected in $B_2\sim 1/V$. At higher energies, $\sqrt{s_{NN}}\geq 20$ GeV, $B_2$ saturates at a constant level. This qualitative change and the vanishing of the volume suppression is shown to be due to the development of strong radial flow with increasing energy. The flow leads to strong space-momentum correlations which counteract the volume effect.