3ΛH and 4ΛH Lifetime, Yield and Directed Flow Measurements in Au+Au Collisions at √sNN=3 GeV with the STAR Detector
Y.H. Leung*
on behalf of the STAR collaboration*: corresponding author
Pre-published on:
August 23, 2022
Published on:
September 01, 2022
Abstract
The study of hyperon-nucleon (Y-N) interaction is of great interest in recent years because of its relation to high-density matter systems such as neutron stars. The presence of hyperons inside neutron stars would soften the equation of state. Hypernuclei, bound states of nucleons and hyperons, serve as a probe to study the Y-N interaction. The data from fixed target Au+Au collisions at √sNN=3 GeV, taken in 2018 by the STAR detector, is ideal for studying the properties of light hypernuclei, such as 3ΛH and 4ΛH, due to the large statistics and high production yield. In this talk, the lifetime of 3ΛH and 4ΛH, the rapidity and centrality dependence of their yields in Au+Au collisions at √sNN=3 GeV will be presented. The measured yield will be compared to measurements at other energies and theoretical models, and the physics implications will be discussed. We also report the first observation of the 3ΛH and 4ΛH directed flow in 5−40% centrality. The directed flow of 3ΛH and 4ΛH are compared with those of the copiously produced particles such as p, Λ, d, t, 3He and 4He. These results will shed light on light hypernuclei production in heavy-ion collisions in high baryon density region.
DOI: https://doi.org/10.22323/1.400.0040
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