A dynamical Einstein-Born-Infeld-dilaton model and holographic quarkonium melting in a magnetic field

被引:0
|
作者
Jena, Siddhi Swarupa [1 ]
Barman, Jyotirmoy [1 ,2 ]
Toniato, Bruno [3 ,4 ]
Dudal, David [3 ]
Mahapatra, Subhash [1 ]
机构
[1] Natl Inst Technol Rourkela, Dept Phys & Astron, Rourkela 769008, India
[2] Int Ctr Theoret Sci, Bengaluru 560089, India
[3] KU Leuven Campus Kortrijk Kulak, Dept Phys, Etienne Sabbelaan 53 Bus 7657, B-8500 Kortrijk, Belgium
[4] Univ Fed ABC UFABC, Ctr Ciencias Nat & Humanas, BR-09210170 Santo Andre, SP, Brazil
来源
JOURNAL OF HIGH ENERGY PHYSICS | 2024年 / 12期
基金
巴西圣保罗研究基金会;
关键词
Gauge-Gravity Correspondence; Holography and Condensed Matter Physics (AdS/CMT); Quarkonium; SPECTRAL FUNCTIONS; SYMMETRY-BREAKING; PHASE-TRANSITION; HEAVY; PLASMA; GAUGE; EVENT;
D O I
10.1007/JHEP12(2024)096
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We generalize the potential reconstruction method to set up a dynamical Einstein-Born-Infeld-dilaton model, which we then use to study holographic quarkonium melting in an external magnetic field. The non-linear nature of the model allows to couple the magnetic field to the quarkonium inner structure without having to introduce back-reacting charged flavour degrees of freedom. The magnetic field dependent melting temperature is computed from the spectral functions and suggests a switch from inverse magnetic to magnetic catalysis when the magnetic field increases. We also discuss the differences due to the anisotropy brought in by the external field.
引用
收藏
页数:34
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