1. Exploring light nuclei production at RHIC and LHC energies with A Multi-Phase Transport model and a coalescence afterburner.
- Author
-
Bailung, Yoshini, Shah, Neha, and Roy, Ankhi
- Subjects
- *
CENTER of mass , *DARK matter , *ANTIMATTER , *PARTICLES (Nuclear physics) , *DEUTERONS - Abstract
In heavy-ion collisions, understanding how light nuclei species are produced can provide insight into the nature of hadronic interactions in extreme conditions. It can also shed light on understanding the matter-antimatter asymmetry and dark matter searches in astrophysical processes. To investigate the production mechanism of light nuclei such as deuteron, triton, and helium-3, we use a naive coalescence afterburner coupled to the well-known "A Multi-Phase Transport model" (AMPT). We focus on studying the production of light nuclei in central Au+Au collisions at different center of mass energies ( s NN = 19.6, 39, and 200 GeV) and in Pb+Pb collisions at s NN = 2.76 TeV, at mid-rapidity. We generate events with the string melting version of AMPT, and feed the information of the nucleons with spatial and momentum conditions into the coalescence afterburner. Our study reports differential and integrated yields in transverse momentum (p T) of the light nuclei in different center of mass energies. We also estimate the coalescence parameters (B A) as a function of p T and collision energy for (anti-)deuterons, tritons and helium-3s for Au+Au and Pb+Pb collisions, which are compared to other light nuclei production studies. All results are compared with measurements from the STAR and ALICE experiments. • The simple coalescence afterburner is effective in comprehensively describing light nuclei production. • The "Coalescence" mode outperforms the kinetic implementation of (anti-)deuteron production in AMPT. • The model closely performs with the PHQMD approach of deuteron production via potential interactions. • The model provides a better description of light nuclei yields at higher collision energies. [ABSTRACT FROM AUTHOR]
- Published
- 2023
- Full Text
- View/download PDF