output
20062026
most citedAsymptotically locally AdS and flat black holes in Horndeski theory

233 citations

Showing 2016 · gr-qcShow all

7 papers · 2 filters

gr-qc2016★ 87 cited

Thermodynamics of Regular Accelerating Black Holes

Marco Astorino

Using the covariant phase space formalism, we compute the conserved charges for a solution, describing an accelerating and electrically charged Reissner-Nordstrom black hole. The m…

gr-qc2016★ 33 cited

Do electromagnetic waves always propagate along null geodesics?

Felipe A. Asenjo, Sergio A. Hojman

We find exact solutions to Maxwell equations written in terms of four-vector potentials in non--rotating, as well as in Gödel and Kerr spacetimes. We show that Maxwell equations ca…

gr-qc2016★ 5 cited

Einstein-Katz action, variational principle, Noether charges and the thermodynamics of AdS-black holes

Andrés Anabalón, Nathalie Deruelle, Félix-Louis Julié

In this paper we describe 4-dimensional gravity coupled to scalar and Maxwell fields by the Einstein-Katz action, that is, the covariant version of the "Gamma-Gamma Gamma-Gamma…

gr-qc2016★ 7 cited

A Class of Integrable Metrics

Andres Anabalon, Carlos Batista

In four dimensions, the most general metric admitting two Killing vectors and a rank-two Killing tensor can be parameterized by ten arbitrary functions of a single variable. We sho…

gr-qc2016

Aspects of Stability of Hairy Black Holes

Andres Anabalon, Jiří Bičák

We analyze spherical and odd-parity linear perturbations of hairy black holes with a minimally coupled scalar field.

gr-qc2016★ 41 cited

Mass of Kerr-Newman Black Holes in an external magnetic field

M. Astorino, G. Compère, R. Oliveri +1

The explicit solution for a Kerr-Newman black hole immersed in an external magnetic field, sometimes called the Melvin-Kerr-Newman black hole, has been derived by Ernst and Wild in…

gr-qc2016★ 12 cited

On the Possibility of Non-Geodesic Motion of the Massless Spinning Top

Cristóbal Armaza, Sergio A. Hojman, Benjamin Koch +1

The motion of spinning massless particles in gravitationally curved backgrounds is revisited by considering new types of constraints. Those constraints guarantee zero mass ($P_μP^μ…