The observable universe could be a 1+ 3-surface (the “brane”) embedded in a 1+ 3+ d-
dimensional spacetime (the “bulk”), with Standard Model particles and fields trapped on the …

We start by reviewing the existing literature on the creation of black holes during high-
energy particle collisions, both in the absence and in the presence of extra, compact …

In the context of the Randall-Sundrum braneworld, the minimal geometric deformation
approach<? format?> is used to generate an analytic interior solution to four-dimensional …

The condition R= 0, where R is the four-dimensional scalar curvature, is used for obtaining a
large class (with an arbitrary function of r) of static, spherically symmetric Lorentzian …

We describe new numerical methods to solve the static axisymmetric vacuum Einstein
equations in more than four dimensions. As an illustration, we study the compactified non …

At the beginning of the 20th century, only two physical fields were known, the
electromagnetic and gravitational ones. Einstein's theory of special relativity (SR), created in …

The minimal geometric deformation approach is employed to show the existence of brane-
world stellar distributions with a vacuum Schwarzschild exterior, thus without energy leaking …

We give a comparative description of different types of regular static, spherically symmetric
black holes (BHs) and discuss in more detail their particular type, which we suggest to call …

The brane cosmology scenario is based on the idea that the Universe is a 3-brane
embedded in a five-dimensional bulk. In this work, a general class of braneworld wormholes …

In the context of the Randall–Sundrum braneworld, the minimal geometric deformation
approach is used to generate a new physically acceptable interior solution to Einstein's field …