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Abstract
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The behavior of the mass spectrum of Ω-hyperons composed of three strange quarks is a significant topic in astrophysics, cosmology, and particle physics. The interactions associated with this hadronic structure in dense matter become particularly important due to the high pressure and the formation of bound hyperon pairs. In the presence of other hadronic matter, omega hyperons, along with extremely high density and temperature in dense matter, can contribute to the formation of new systems of hypernuclei and strange nuclei, which influence the dynamic properties of condensed matter. Therefore, in this study, a theoretical analysis based on quantum chromodynamics and the nature of the strong interaction is presented, focusing on relativistic mass corrections at high temperatures for the omega hyperon mass spectrum. The theoretical results obtained show good agreement with experimental data and are applicable in studies related to hyperon interactions with hypernuclei and condensed quark matter.
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