Relativistic hydrodynamics under rotation: Prospects and limitations from a holographic perspective

被引:2
作者
Amano, Markus A. G. [1 ,2 ]
Cartwright, Casey [3 ]
Kaminski, Matthias [4 ]
Wu, Jackson [4 ]
机构
[1] Henan Univ, Inst Conorary Math, Sch Math & Stat, Kaifeng 475004, Henan, Peoples R China
[2] Yamagata Univ, Dept Phys, Kojirakawa Machi 1-4-12, Yamagata 9908560, Japan
[3] Univ Utrecht, Inst Theoret Phys, Princetonpl 5, NL-3584 CC Utrecht, Netherlands
[4] Univ Alabama, Dept Phys & Astron, 514 Univ Blvd, Tuscaloosa, AL 35487 USA
基金
美国国家科学基金会;
关键词
AdS/CFT; Holography; Hydrodynamics; Strongly-coupled field theory; BLACK-HOLES; NUCLEAR COLLISIONS; SHEAR VISCOSITY; THERMODYNAMICS; POLARIZATION; GRAVITY; EXAMPLE; FLOW;
D O I
10.1016/j.ppnp.2024.104135
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
The AdS/CFT correspondence, or holography, has provided numerous important insights into the behavior of strongly-coupled many-body systems. Crucially, it has provided a testing ground for the construction of new effective field theories, especially those in the low frequency, long wavelength limit known as hydrodynamics. We review the study of strongly-coupled rotating fluids using holography, and we examine the hydrodynamics emerging from the study of rotating Myers-Perry black holes. We discuss three regimes in which holographic rotating fluids display either (1) hydrodynamic behavior of a boosted fluid, (2) hydrodynamic behavior distinct from a boosted fluid, or (3) no obvious hydrodynamic behavior. We describe techniques to obtain hydrodynamic and non-hydrodynamic modes, and we compute the radius of convergence for the hydrodynamic regimes. The limitations of hydrodynamics under rotation are discussed alongside our findings.
引用
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页数:56
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