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The non-zero value of Planck constant $hbar$ underlies the emergence of several inequalities that must be satisfied in the quantum realm, the most prominent one being the Heisenberg Uncertainty Principle. Among these inequalities, the Bekenstein bound provides a universal limit on the entropy that can be contained in a localized quantum system of given size and total energy. In this letter, we explore how the Bekenstein bound is affected when the Heisenberg uncertainty relation is deformed so as to accommodate gravitational effects at the Planck scale (Generalized Uncertainty Principle). By resorting to very general arguments, we derive in this way a generalized Bekenstein bound. Physical implications of this result are discussed for both cases of positive and negative values of the deformation parameter.
We explore the structure of holographic entropy relations (associated with information quantities given by a linear combination of entanglement entropies of spatial sub-partitions of a CFT state with geometric bulk dual). Such entropy relations can b
We analyze general uncertainty relations and we show that there can exist such pairs of non--commuting observables $A$ and $B$ and such vectors that the lower bound for the product of standard deviations $Delta A$ and $Delta B$ calculated for these v
In recent work we showed that, for a class of conformal field theories (CFT) with Gauss-Bonnet gravity dual, the shear viscosity to entropy density ratio, $eta/s$, could violate the conjectured Kovtun-Starinets-Son viscosity bound, $eta/sgeq1/4pi$. I
Studies in string theory and quantum gravity suggest the existence of a finite lower limit $Delta x_0$ to the possible resolution of distances, at the latest on the scale of the Planck length of $10^{-35}m$. Within the framework of the euclidean path
We extend the perturbative classical double copy to the analysis of bound systems. We first obtain the leading order perturbative gluon radiation field sourced by a system of interacting color charges in arbitrary time dependent orbits, and test its