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Main Authors: Zhu, Zhou-Run, Wang, Sheng, Liu, Yang-Kang, Hou, Defu
Format: Preprint
Published: 2025
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Online Access:https://arxiv.org/abs/2501.04318
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author Zhu, Zhou-Run
Wang, Sheng
Liu, Yang-Kang
Hou, Defu
author_facet Zhu, Zhou-Run
Wang, Sheng
Liu, Yang-Kang
Hou, Defu
contents 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 ultra-local description, the boosted fluid represents a globally rotating fluid. Using a holographic approach, we systematically analyze how boost parameter influences these quantities. Our results reveal that increasing boost parameter causes the imaginary potential to emerge at smaller interquark distances, suggesting that boost parameter accelerates quarkonium melting. Furthermore, we find that boost parameter enhances the thermal width, indicating greater instability of the bound state at higher boost parameter. Notably, we observe that the effect of boost parameter on quarkonium dissociation is more pronounced when the axis of the quark-antiquark pair is transverse to the direction of boost parameter.
format Preprint
id arxiv_https___arxiv_org_abs_2501_04318
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Imaginary potential and thermal width in the spinning black hole background from holography
Zhu, Zhou-Run
Wang, Sheng
Liu, Yang-Kang
Hou, Defu
High Energy Physics - Phenomenology
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 ultra-local description, the boosted fluid represents a globally rotating fluid. Using a holographic approach, we systematically analyze how boost parameter influences these quantities. Our results reveal that increasing boost parameter causes the imaginary potential to emerge at smaller interquark distances, suggesting that boost parameter accelerates quarkonium melting. Furthermore, we find that boost parameter enhances the thermal width, indicating greater instability of the bound state at higher boost parameter. Notably, we observe that the effect of boost parameter on quarkonium dissociation is more pronounced when the axis of the quark-antiquark pair is transverse to the direction of boost parameter.
title Imaginary potential and thermal width in the spinning black hole background from holography
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2501.04318