Description
A new approach to solve Einstein equations in higher dimensions will be discussed. It consists in decomposing the equations into several sectors with known integrable structure. I will construct large classes of non-supersymmetric smooth solutions that are asymptotic to four-dimensional Minkowski spacetime with additional compact circles. They are induced by bubbles of spacetime supported by electromagnetic flux and look like Reissner-Nordström black holes but are smooth and horizonless. I will pay particular attention to the neutral solutions and compare their geometries to Schwarzschild black holes. I will also briefly discuss the stability of the solutions.
Auteur principal
Dr
Pierre Heidmann
(Johns Hopkins University)
Co-auteurs
Prof.
Ibrahima Bah
(Johns Hopkins University)
M.
Peter Weck
(Johns Hopkins University)
