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            <title xml:lang="en">Inhibition of splitting of the chiral and deconfinement transition due to rotation in QCD: the phase diagram of linear sigma model coupled to Polyakov loop</title>
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            <funder>This work is supported by the European Union - NextGenerationEU through grant No.760079/23.05.2023, funded by the Romanian ministry of research, innovation and digitalization through Romania’s National Recovery and Resilience Plan, call no. PNRR-III-C9-2022-I8.</funder>
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            <idno type="stamp" n="UNIV-TOURS">Université François Rabelais</idno>
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            <idno type="stamp" n="UNIV-ORLEANS">Université d'Orléans</idno>
            <idno type="stamp" n="INSMI">CNRS-INSMI - INstitut des Sciences Mathématiques et de leurs Interactions</idno>
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                <title xml:lang="en">Inhibition of splitting of the chiral and deconfinement transition due to rotation in QCD: the phase diagram of linear sigma model coupled to Polyakov loop</title>
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                    <forename type="first">Victor E</forename>
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                <term xml:lang="en">sigma model, linear</term>
                <term xml:lang="en">critical phenomena, deconfinement</term>
                <term xml:lang="en">transition, chiral</term>
                <term xml:lang="en">splitting</term>
                <term xml:lang="en">velocity</term>
                <term xml:lang="en">rotation</term>
                <term xml:lang="en">Polyakov loop</term>
                <term xml:lang="en">temperature</term>
                <term xml:lang="en">causality</term>
                <term xml:lang="en">quantum chromodynamics</term>
                <term xml:lang="en">quark</term>
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              <p>We discuss the effect of rigid rotation on critical temperatures of deconfinement and chiral transitions in the linear sigma model coupled to quarks and the Polyakov loop. We point out the essential role of the causality condition, which requires that any point of the system should rotate slower than the velocity of light. We show that imposing this physical requirement leads to inhibition of the splitting between the chiral and confining transitions, which becomes negligibly small ($\Delta T \sim 1$~MeV or less) for experimentally relevant, slow angular velocities $\Omega \sim 10$~MeV of a $(5-10)$~fm-sized systems. Moreover, the boundedness of the system has a much bigger effect on temperature splitting than the rotation itself: the splitting reaches 10~MeV in a small, one-fermi-sized non-rotating system. The temperature splitting may, however, become enhanced in an academic limit of ultra-relativistic regimes when the boundary of the system rotates at near-to-light velocities.</p>
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