Titill: | Generalised global symmetries in holography: magnetohydrodynamic waves in a strongly interacting plasma |
Höfundur: |
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Útgáfa: | 2019-04-23 |
Tungumál: | Enska |
Umfang: | 141 |
Háskóli/Stofnun: | Háskóli Íslands University of Iceland |
Svið: | Verkfræði- og náttúruvísindasvið (HÍ) School of Engineering and Natural Sciences (UI) |
Deild: | Raunvísindastofnun (HÍ) Science Institute (UI) |
Birtist í: | Journal of High Energy Physics;2019(4) |
ISSN: | 1029-8479 |
DOI: | 10.1007/JHEP04(2019)141 |
Efnisorð: | Effective Field Theories; Gauge-gravity correspondence; Global Symmetries; Holography and quark-gluon plasmas; Sviðsfræði |
URI: | https://hdl.handle.net/20.500.11815/1779 |
Tilvitnun:Grozdanov, S., Poovuttikul, N. Generalised global symmetries in holography: magnetohydrodynamic waves in a strongly interacting plasma. Journal of High Energy Physics 2019, 141 (2019). https://doi.org/10.1007/JHEP04(2019)141
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Útdráttur:We begin the exploration of holographic duals to theories with generalised global (higher-form) symmetries. In particular, we focus on the case of magnetohydrodynamics (MHD) in strongly coupled plasmas by constructing and analysing a holographic dual to a recent, generalised global symmetry-based formulation of dissipative MHD. The simplest holographic dual to the effective theory of MHD that was proposed as a description of plasmas with any equation of state and transport coefficients contains dynamical graviton and two-form gauge field fluctuations in a magnetised black brane background. The dual field theory, which is closely related to the large-N c , N = 4 supersymmetric Yang-Mills theory at (infinitely) strong coupling, is, as we argue, in our setup coupled to a dynamical U(1) gauge field with a renormalisation condition-dependent electromagnetic coupling. After constructing the holographic dictionary for gauge-gravity duals of field theories with higher-form symmetries, we compute the dual equation of state and transport coefficients, and for the first time analyse phenomenology of MHD waves in a strongly interacting, dense plasma with a (holographic) microscopic description. From weak to extremely strong magnetic fields, several predictions for the behaviour of Alfvén and magnetosonic waves are discussed.
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Athugasemdir:Publisher's version (útgefin grein)
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Leyfi:This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.
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