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\title{{\Large Lifetime measurements of light hypernuclei in Au+Au collisions from STAR experiment}}% Force line breaks with \\

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\author{\large Xiujun Li (for the STAR Collaboration)}
\affiliation{\normalsize University of Science and Technology of China}
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Hypernuclei are bound nuclear systems of correlated nucleons and hyperons. Therefore, the production of hypernuclei in heavy-ion collisions provides an experimental avenue for studying hyperon$-$nucleon (Y-N) interaction, which is an important ingredient, not only in the equation-of-state of astrophysical objects such as neutron stars, but also in the description of the hadronic phase of a heavy-ion collision. 
The strength of the Y-N interaction can be investigated by measuring the properties of hypernuclei.
For example, light $\Lambda$-hypernuclei containing one hyperon are conventionally understood as a weakly bound system of a $\Lambda$ and a nucleus, suggesting their lifetimes are close to the free-$\Lambda$ lifetime.% and the level of closeness has implications on the strength of the Y-N interaction. %Thus, precise lifetime measurements of hypernuclei help us to understand the Y-N interaction.

In heavy-ion collisions, light hypernuclei are expected to be abundantly produced at low collision energies due to the high baryon density. 
In this presentation, we will report precise lifetime measurements of $^3_{\Lambda}$H, $^4_{\Lambda}$H, and $^4_{\Lambda}$He in Au+Au collisions at $\sqrt{s_{NN}}$ = 3 GeV and 7.2 GeV, recorded by the  STAR experiment at RHIC in the fixed-target mode in 2018. The results will be compared with model calculations and physics implications will be discussed.
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