| Home > Publications database > Determination of the $\phi$ -meson production process and its absorption cross section via directed flow |
| Journal Article | GSI-2026-00014 |
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2025
North-Holland Publ.
Amsterdam
Please use a persistent id in citations: doi:10.1016/j.physletb.2025.139870 doi:10.15120/GSI-2026-00014
Abstract: It is shown that the directed flow of ϕ-mesons in Au+Au collisions at sNN=3 GeV, is sensitive to the production and the absorption cross section of the ϕ in a nuclear medium. This provides a new observable to constrain the in-medium properties of the ϕ which is independent of its absolute production rate. STAR data disfavor any significant ϕ-N absorption in dense nuclear matter and are consistent with a very small cross section of the ϕ comparable to the vacuum cross section. The similarity of the ϕ-meson and proton directed flow also indicates that the ϕ is produced in conjunction with a baryon.
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