7,598 research outputs found
Complexity growth rates for AdS black holes in massive gravity and gravity
The "complexity = action" duality states that the quantum complexity is equal
to the action of the stationary AdS black holes within the Wheeler-DeWitt patch
at late time approximation. We compute the action growth rates of the neutral
and charged black holes in massive gravity and the neutral, charged and
Kerr-Newman black holes in gravity to test this conjecture. Besides, we
investigate the effects of the massive graviton terms, higher derivative terms
and the topology of the black hole horizon on the complexity growth rate.Comment: 11 pages, no figur
Domain wall brane in a reduced Born-Infeld- theory
The Born-Infeld theory is reduced from the Born-Infeld determinantal
gravity in Weitzenb\"ock spacetime. We investigate a braneworld scenario in
this theory and obtain an analytic domain wall solution by utilizing the
first-order formalism. The model is stable against the linear tensor
perturbation. It is shown that the massless graviton is localized on the brane,
but the continuous massive gravitons are non-localized and will generate a tiny
correction with the behavior of to the Newtonian potential.
The four-dimensional teleparallel gravity is recovered as an effective infrared
theory on the brane. As a physical application, we consider the
(quasi-)localization property of spin-1/2 Dirac fermion in this model.Comment: 9 pages, 2 figures, published versio
Integrated intracellular metabolic profiling and pathway analysis approaches reveal complex metabolic regulation by Clostridium acetobutylicum
Gravito-Electromagnetic coupled perturbations and quasinormal modes of a charged black hole with scalar hair
From the quantum point of view, singularity should not exist. Recently, Bah
and Heidmann constructed a five-dimensional singularity free topology
star/black hole [Phys. Rev. Lett. 126, 151101 (2021)]. By integrating the extra
dimension, a four-dimensional static spherical black hole with a magnetic
charge and scalar hair can be obtained. In this paper, we study the quasinormal
modes (QNMs) of the magnetic field and gravitational field on the background of
this four-dimensional charged black hole with scalar hair. The odd parity of
the gravitational perturbations couples with the even parity of the magnetic
field perturbations. Two coupled second-order derivative equations are
obtained. Using the matrix-valued direct integration method, we obtain the
fundamental QNM frequencies numerically. The effect of the magnetic charge on
the QNMs is studied. The differences of the frequencies of the fundamental QNMs
between the charged black hole with scalar hair and the Reissner-Norstr\"{o}m
black hole are very small for the angular number . However, some new
interesting results are found for higher angular number.Comment: 10 pages, 3 figures, 2 tables, some mistakes have been correcte
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