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Role of $Σ^*(1385)$ on $Λ$ hyperon polarization in relativistic heavy ion collisions

Haesom Sung, Che Ming Ko, Su Houng Lee

TL;DR

This work addresses the origin and time evolution of Λ polarization in relativistic heavy-ion collisions by explicitly treating the Σ^*(1385) resonance as a dynamical degree of freedom through Λ+π↔Σ^*↔Σ+π, and by incorporating feed-down from Σ^0, Σ^*, and Ξ decays. The authors derive spin-dependent, coupled kinetic equations for the numbers and polarizations of Λ, Σ, and Σ^* (and similarly for Ξ/Ξ^*) and compute thermally averaged cross sections and decay rates to drive the evolution during the hadronic stage of Au-Au collisions at √s_{NN}=7.7 GeV. They find that Λ polarization exhibits only a small time dependence, increasing slightly in the early hadronic phase, but being reduced when feed-down is included; Σ^* polarization continuously decreases, and Σ polarization remains nearly constant. Overall, the time variation of P_Λ is small, supporting the common assumption of early Λ spin freeze-out at chemical freeze-out, with feed-down contributing a modest additional reduction, and the framework provides a basis for extending the analysis to other hyperons such as Ξ and Ω.

Abstract

The effect of $Σ^*(1385)$ baryon resonance on the time evolution of the $Λ$ hyperon polarization in hadronic matter is studied using a kinetic approach. This approach explicitly includes the production of the $Σ^*$ resonance from the $Λ-π$ and $Σ(1192)-π$ scatterings as well as its decay into $Λ+π$ or $Σ+π$. The resulting coupled kinetic equations governing the time evolution of $Λ$, $Σ$ and $Σ^*$ numbers and polarizations are solved for Au-Au collisions at $\sqrt{s_{NN}}=7.7$ GeV and 20-50\% centrality, using initial values determined by thermal yields and the thermal vorticity at chemical freeze-out temperature. As the hadronic matter expands and cools, the $Λ$ polarization is found to increase slightly during early times and then decreases very slowly afterwards, while the $Σ$ polarization remains nearly constant and the $Σ^*$ polarization continuously decreases. Including feed-down contributions to the $Λ$ polarization from the decays of partially polarized $Σ^0$, $Σ^*$, and $Ξ(1322)$ hyperons, where the $Ξ$ polarization is obtained by solving coupled kinetic equations for the $Ξ$ and $Ξ^*(1532)$ system, the resulting $Λ$ polarization becomes smaller and decreases over time. In both cases, however, the time variation of the $Λ$ polarization is sufficiently small to support the assumption of an early freeze-out of $Λ$ spin degree of freedom in relativistic heavy ion collisions.

Role of $Σ^*(1385)$ on $Λ$ hyperon polarization in relativistic heavy ion collisions

TL;DR

This work addresses the origin and time evolution of Λ polarization in relativistic heavy-ion collisions by explicitly treating the Σ^*(1385) resonance as a dynamical degree of freedom through Λ+π↔Σ^*↔Σ+π, and by incorporating feed-down from Σ^0, Σ^*, and Ξ decays. The authors derive spin-dependent, coupled kinetic equations for the numbers and polarizations of Λ, Σ, and Σ^* (and similarly for Ξ/Ξ^*) and compute thermally averaged cross sections and decay rates to drive the evolution during the hadronic stage of Au-Au collisions at √s_{NN}=7.7 GeV. They find that Λ polarization exhibits only a small time dependence, increasing slightly in the early hadronic phase, but being reduced when feed-down is included; Σ^* polarization continuously decreases, and Σ polarization remains nearly constant. Overall, the time variation of P_Λ is small, supporting the common assumption of early Λ spin freeze-out at chemical freeze-out, with feed-down contributing a modest additional reduction, and the framework provides a basis for extending the analysis to other hyperons such as Ξ and Ω.

Abstract

The effect of baryon resonance on the time evolution of the hyperon polarization in hadronic matter is studied using a kinetic approach. This approach explicitly includes the production of the resonance from the and scatterings as well as its decay into or . The resulting coupled kinetic equations governing the time evolution of , and numbers and polarizations are solved for Au-Au collisions at GeV and 20-50\% centrality, using initial values determined by thermal yields and the thermal vorticity at chemical freeze-out temperature. As the hadronic matter expands and cools, the polarization is found to increase slightly during early times and then decreases very slowly afterwards, while the polarization remains nearly constant and the polarization continuously decreases. Including feed-down contributions to the polarization from the decays of partially polarized , , and hyperons, where the polarization is obtained by solving coupled kinetic equations for the and system, the resulting polarization becomes smaller and decreases over time. In both cases, however, the time variation of the polarization is sufficiently small to support the assumption of an early freeze-out of spin degree of freedom in relativistic heavy ion collisions.

Paper Structure

This paper contains 7 sections, 15 equations, 6 figures.

Figures (6)

  • Figure 1: Temperature dependence of the thermal averages of the spin-averaged $\Lambda+\pi\rightarrow \Sigma^*$ (solid line) and $\Sigma+\pi\rightarrow \Sigma^*$ (dashed line) cross sections shown in the inset.
  • Figure 2: Time evolution of $\Lambda$ (solid line), $\Sigma$ (dashed line), and $\Sigma^*$ (dotted line) numbers in Au-Au collisions at $\sqrt{s_{NN}}=7.7$ GeV and 20-50% collision centrality.
  • Figure 3: Time evolution of $\Lambda$ (solid line), $\Sigma$ (dashed line), and $\Sigma^*(1385)$ (dotted line) polarizations in Au-Au collisions at $\sqrt{s_{NN}}=7.7$ GeV and 20-50% collision centrality, for initial $\Lambda$ and $\Sigma$ polarizations of 0.025 and initial $\Sigma^*$ polarization of 0.042. Also shown (dot-dashed line) is the $\Lambda$ polarization $P_\Lambda^{\rm FD}$ that includes the feed-down contributions described in the text.
  • Figure 4: Temperature dependence of the thermal average of the spin-averaged $\Xi+\pi\rightarrow \Xi^*$ cross section shown in inset.
  • Figure 5: Time evolution of the $\Xi$ number (solid line) and $\Xi^*$ number (dotted line) in Au-Au collisions at $\sqrt{s_{NN}}=7.7$ GeV and 20-50% collision centrality.
  • ...and 1 more figures