Charmonia and Bottomonia in asymmetric magnetized hot nuclear matter

preprint2019arXivOpen access

Abstract

We investigate the mass-shift of PP-wave charmonium (χc0{χ_c}_0, χc1{χ_c}_1) and SS and PP-wave bottomonium (ηbη_b, ΥΥ, χb0{χ_b}_0 and χb1{χ_b}_1) states in magnetized hot asymmetric nuclear matter using the unification of QCD sum rules (QCDSR) and chiral SU(3)SU(3) model. Within QCDSR, we use two approaches, i.e.i.e., moment sum rule and Borel sum rule. The magnetic field induced scalar gluon condensate ⟨αsπGμνaGaμν⟩\left\langle \frac{α_{s}}π G^a_{μν} {G^a}^{μν} \right\rangle and the twist-2 gluon operator ⟨αsπGμσaGaνσ⟩\left\langle \frac{α_{s}}π G^a_{μσ} {{G^a}_ν}^σ \right\rangle calculated in chiral SU(3SU(3) model are utilised in QCD sum rules to calculate the in-medium mass-shift of above mesons. The attractive mass-shift of these mesons is observed which is more sensitive to magnetic field in high density regime for charmonium, but less for bottomonium. These results may be helpful to understand the decay of higher quarkonium states to the lower quarkonium states in asymmetric heavy ion collision experiments.

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