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  • Open Access

Imaginary potential and thermal width in the spinning black hole background from holography

Zhou-Run Zhu1,*, Sheng Wang2,†, Yang-Kang Liu2,‡, and Defu Hou2,§

  • *Contact author: zhuzhourun@zknu.edu.cn
  • †Contact author: shengwang@mails.ccnu.edu.cn
  • ‡Contact author: ykl@mails.ccnu.edu.cn
  • §Contact author: houdf@mail.ccnu.edu.cn

Phys. Rev. D 112, 026012 – Published 7 July, 2025

DOI: https://doi.org/10.1103/rwrh-z742

Abstract

In this study, we investigate the imaginary potential of heavy quarkonium in the spinning black hole background. Then, we estimate the thermal width, which is determined by the imaginary part of the finite-temperature potential. In the ultralocal description, the boosted fluid represents a globally rotating fluid. Using a holographic approach, we systematically analyze how the boost parameter influences these quantities. Our results reveal that increasing the boost parameter causes the imaginary potential to emerge at smaller interquark distances, suggesting that the boost parameter accelerates quarkonium melting. Furthermore, we find that the boost parameter enhances the thermal width, indicating greater instability of the bound state at higher boost parameter values. Notably, we observe that the effect of the boost parameter on quarkonium dissociation is more pronounced when the axis of the quark-antiquark pair is transverse to the direction of the boost parameter.

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