3–9 Sept 2023
Hilton of the Americas, 1600 Lamar, Houston, Texas, 77010, USA
US/Central timezone

Measurements of Hypernuclei Production and Their Properties in Heavy-Ion Collisions at STAR

5 Sept 2023, 17:30
2h 10m
Grand Ballroom, 4th floor ( Hilton of the Americas)

Grand Ballroom, 4th floor

Hilton of the Americas

Poster Light and strange flavor Poster Session

Speaker

Xiujun Li (USTC)

Description

Hypernuclei, bound states of nuclei with one or more hyperons, serve as a natural laboratory to investigate the hyperon-nucleon ($Y$-$N$) interaction, an important ingredient for the equation-of-state (EoS) of nuclear matter. Precise measurements of hypernuclei properties and their production yields in heavy-ion collisions are crucial for the understanding of their production mechanisms and the strength of the $Y$-$N$ interaction. The strangeness population factor, $S_{\rm A}=(^{A}_{\Lambda}\mathrm{H}/^{A}\mathrm{He})/(\Lambda/p)$ (A=3,4), is of particular interest as it directly relates to the ratio of light nuclei and hypernuclei coalescence parameters $B_{A}$. Moreover, it is suggested that $S_{A}$ might be sensitive to the onset of deconfinement. The STAR Beam Energy Scan II program and isobar collisions offer a great opportunity to investigate energy and system size dependence of hypernuclei production.

In this talk, we present new measurements on transverse momentum ($p_T$), rapidity\,($y$), and centrality dependence of $\rm ^{3}_{\Lambda}H$, $\rm ^{4}_{\Lambda}H$, and $\rm ^{4}_{\Lambda}He$ production yields in Au+Au collisions from $\sqrt{s_{\rm NN}}=$ 3 to 27 GeV, as well as in Ru+Ru and Zr+Zr collisions at $\sqrt{s_{\rm NN}}=200$ GeV. Strangeness population factors $S_{3,4}$ as functions of collision energy, centrality, $p_T$, and $y$ are also reported. In addition, we present new measurements on $\rm {}^{4}_{\Lambda}He$ and $\rm {}^{5}_{\Lambda}He$ lifetimes. These results are compared with phenomenological model calculations, and the physics implications on the hypernuclei production mechanism and properties of $Y$-$N$ interaction will be discussed.

Category Experiment
Collaboration (if applicable) STAR Collaboration

Primary author

Presentation materials