2018
Complexity Growth Rate in Lovelock Gravity
Abstract: Using the "Complexity = Action" framework we compute the late time growth of complexity for charged black holes in Lovelock gravity. Our calculation is facilitated by the fact that the null boundaries of the Wheeler-DeWitt patch do not contribute at late times and essential contributions coming from the joints are now understood [1]. The late time growth rate reduces to a difference of internal energies associated with the inner and outer horizons, and in the limit where the mass is much larger than the charge…
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Cited by 93 publications
(89 citation statements)
References 116 publications
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“…This is valid to generally static black holes in higher derivative gravities. The result covers previous results published in literatures [9,32,33,34,35,36].…”
Section: Discussionsupporting
confidence: 90%
“…This is valid to generally static black holes in higher derivative gravities. The result covers previous results published in literatures [9,32,33,34,35,36].…”
Section: Discussionsupporting
confidence: 90%
“…This reproduces the result first obtained in [34] for charged Lovelock black holes. Moreover, it was established [34] that the above result can be expressed as…”
Section: Late Times and Early Timessupporting
confidence: 91%
“…It is worth noting that in the limit r 0 → r − , which is equal to r c → ∞, the above result at late times exactly matches with the known result [64]. Furthermore, because of the same reasons for Einstein-Hilbert theory we do not consider the contribution of counterterm action (41) on r = r 0 surface.…”
Section: Complexity In Gauss-bonnet-maxwell Theory At Finite Cut Offsupporting
confidence: 78%
