On prethermal time crystals from semi-holography

We demonstrate the existence of a pair of almost dissipationless oscillating modes at low temperatures in both the shear and sound channels of a hybrid quantum system, comprised of a weakly self-interacting perturbative sector coupled to strongly self-interacting holographic degrees of freedom descr...

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Autores principales: Mitra, Toshali (Autor) , Mondkar, Sukrut (Autor) , Mukhopadhyay, Ayan (Autor) , Soloviev, Alexander (Autor)
Formato: Article (Journal)
Lenguaje:inglés
Publicado: June 16, 2026
In: Journal of high energy physics
Year: 2026, Volumen: 2026, Número: 6, Pages: 1-37
ISSN:1029-8479
DOI:10.1007/JHEP06(2026)172
Acceso en línea:Verlag, kostenfrei, Volltext: https://doi.org/10.1007/JHEP06(2026)172
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Notas de Autor:Toshali Mitra, Sukrut Mondkar, Ayan Mukhopadhyay and Alexander Soloviev
Descripción
Sumario:We demonstrate the existence of a pair of almost dissipationless oscillating modes at low temperatures in both the shear and sound channels of a hybrid quantum system, comprised of a weakly self-interacting perturbative sector coupled to strongly self-interacting holographic degrees of freedom described by a black hole geometry. We argue that these modes realize prethermal time-crystal behavior in semi-holographic systems without fine-tuning and can be observed by measuring operators that probe either the hard (perturbative) or the soft (holographic) sector. We also find novel short wavelength instabilities that lead to the formation of inhomogeneities even at higher temperatures. These results provide evidence that black holes with planar horizons and dynamical boundary conditions can develop both inhomogeneous and metastable time-crystal phases over a wide range of temperatures set by an intermediate scale given by the intersector coupling. Furthermore, they suggest that such phases can be realized without external driving in non-Abelian plasmas of asymptotically free gauge theories in the large-N limit.
Notas:Veröffentlicht: 16. Juni 2026
Gesehen am 25.09.2026
Descripción Física:Online Resource
ISSN:1029-8479
DOI:10.1007/JHEP06(2026)172