Probing (Hyper)Nuclei Wave Functions and Production Mechanisms in sNN=200 GeV Isobar Collisions at RHIC
The STAR Collaboration
Abstract
The study of nuclei and hypernuclei production is a powerful tool to investigate the formation mechanism of loosely bound states in high-energy heavy-ion collisions. A key prediction from coalescence models is a strong suppression of the hypertriton (3ΛH) compared to 3He production in small collision systems due to the larger radius of 3ΛH. In this letter, the STAR collaboration reports measurements on (hyper)nuclei (3ΛH, 3ΛH, 3He, 3He, t) production at mid-rapidity in Ru+Ru and Zr+Zr collisions at sNN=200 GeV as a function of collision centrality. We find that the ratios NtNp/Nd2 and S3 =(N3ΛH/N3He)/(NΛ/Np) deviate significantly from thermal model expectations. Coalescence calculations incorporating realistic non-Gaussian wave functions for the d and 3ΛH provide an improved description of the data, while Gaussian descriptions of the 3ΛH wave function fail to simultaneously reproduce the measured S3 and the binding energy of 3ΛH. These results suggest that the 3ΛH wave function contains larger short-distance d--Λ probability than implied by a Gaussian ansatz, demonstrating the potential of heavy-ion production measurements as a probe of hypernuclear wave functions and the underlying hyperon--nucleon interaction.
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