Random matrix theory for complexity growth and black hole interiors
نویسندگان
چکیده
We study a precise and computationally tractable notion of operator complexity in holographic quantum theories, including the ensemble dual Jackiw-Teitelboim gravity two-dimensional conformal field theories. This is refined, "microcanonical" version K-complexity that applies to theories with infinite or continuous spectra (including theories), we exhibits exponential growth for scrambling time, followed by linear until saturation at time entropy $\unicode{x2014}$a behavior characteristic chaos. show regime implies universal random matrix description dynamics after scrambling. Our main tool establishing this connection "complexity renormalization group" framework develop allows us effective different timescales "integrating out" large K-complexities. In setting, comment on empirical match between our maximal volume proposal, speculate theory spatial translation symmetry smooth black hole interiors.
منابع مشابه
Organizational Black Hole Theory
There are issues in organizations that require new theoretical formulation. Hence, metaphorical theorizing is used in the study of organizations to interpret them and understand their complexities. In this method, the organization is likened to an entity and one of the key features of that entity is generalized to the organization. It should be borne in mind that most organizational theories ar...
متن کاملQuantum effects in black hole interiors.
The Weyl curvature inside a black hole formed in a generic collapse grows, classically without bound, near to the inner horizon, due to partial absorption and blueshifting of the radiative tail of the collapse. Using a spherical model, we examine how this growth is modified by quantum effects of conformally coupled massless fields.
متن کاملNumerical investigation of black hole interiors
Gravitational perturbations which are present in any realistic stellar collapse to a black hole, die off in the exterior of the hole, but experience an infinite blueshift in the interior. This is believed to lead to a slowly contracting lightlike scalar curvature singularity, characterized by a divergence of the hole’s (quasi-local) mass function along the inner horizon. The region near the inn...
متن کاملSemiclassical effects in black hole interiors
First-order semiclassical perturbations to the Schwarzschild black hole geometry are studied within the black hole interior. The source of the perturbations is taken to be the vacuum stress-energy of quantized scalar, spinor, and vector fields, evaluated using analytic approximations developed by Page and others (for massless fields) and the DeWitt-Schwinger approximation (for massive fields). ...
متن کاملNumerical Black Hole Interiors and String Cosmology Initial Conditions
Recent work has proposed the principle of ‘asymptotic past triviality’ to characterize the initial state in the pre-big bang scenario of string cosmology, that it is a generic perturbative solution of the low-energy effective action. Among the more generic sets of solutions which is simple enough to investigate thoroughly, yet complex enough to exhibit interesting behavior, is the gravitydilato...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Journal of High Energy Physics
سال: 2022
ISSN: ['1127-2236', '1126-6708', '1029-8479']
DOI: https://doi.org/10.1007/jhep01(2022)016