Thick domain wall spacetimes with and without reflection symmetry Melfo, Alejandra; Pantoja, Nelson; Skirzewski, Aureliano Abstract We show that the spacetimes of domain wall solutions to the coupled Einstein-scalar field equations with a given scalar field potential fall into two classes, depending on whether or not reflection symmetry on the wall is imposed. Solutions with reflection symmetry are dynamic, while the asymmetric ones are static. Asymmetric walls are asymptotically flat on one side and reduce to the Taub spacetime on the other. Examples of asymmetric thick walls in D-dimensional spacetimes are given, and results on the thin-wall limit of the dynamic, symmetric walls are extended to the asymme...
We consider static cylindrically symmetric spacetimes with a cosmological constant Lambda and obtai...
In theoretical physics, it is often conjectured that a correspondence exists between the gravitatio...
We solve numerically equations of motion for real self-interacting scalar fields in the background o...
An exact solution of the Einstein equations for a static, planar domain wall with finite thickness i...
We investigate a self-gravitating thick domain wall for a $\lambda \Phi^4$ potential. The system of ...
[[abstract]]We solve the vacuum Einstein’s field equations with the cosmological constant in space-t...
The case of a domain wall of finite thickness is examined by use of two different expressions for th...
We propose a general method for solving exactly the static field equations of Einstein and Einstein-...
Generalizing the Lie derivative of smooth tensor fields to distribution-valued tensors, we examine t...
We analyze the possibility of constructing supersymmetric curved domain wall solutions in five-dimen...
New BPS domain wall solutions. (Pantoja, Nelson y Ramírez, Alba) Abstract Smooth solutions of gr...
We consider BPS domain walls in four-dimensional N = 1 supersymmetric models with continuous global ...
We find Einstein–Yang–Mills (EYM) black hole solutions endowed with massless scalar hair in the pres...
We construct a plane symmetric, standing gravitational wave for a domain wall plus a massless scalar...
We describe the exact solution of Einstein's equation corresponding to a static homogenous distribut...
We consider static cylindrically symmetric spacetimes with a cosmological constant Lambda and obtai...
In theoretical physics, it is often conjectured that a correspondence exists between the gravitatio...
We solve numerically equations of motion for real self-interacting scalar fields in the background o...
An exact solution of the Einstein equations for a static, planar domain wall with finite thickness i...
We investigate a self-gravitating thick domain wall for a $\lambda \Phi^4$ potential. The system of ...
[[abstract]]We solve the vacuum Einstein’s field equations with the cosmological constant in space-t...
The case of a domain wall of finite thickness is examined by use of two different expressions for th...
We propose a general method for solving exactly the static field equations of Einstein and Einstein-...
Generalizing the Lie derivative of smooth tensor fields to distribution-valued tensors, we examine t...
We analyze the possibility of constructing supersymmetric curved domain wall solutions in five-dimen...
New BPS domain wall solutions. (Pantoja, Nelson y Ramírez, Alba) Abstract Smooth solutions of gr...
We consider BPS domain walls in four-dimensional N = 1 supersymmetric models with continuous global ...
We find Einstein–Yang–Mills (EYM) black hole solutions endowed with massless scalar hair in the pres...
We construct a plane symmetric, standing gravitational wave for a domain wall plus a massless scalar...
We describe the exact solution of Einstein's equation corresponding to a static homogenous distribut...
We consider static cylindrically symmetric spacetimes with a cosmological constant Lambda and obtai...
In theoretical physics, it is often conjectured that a correspondence exists between the gravitatio...
We solve numerically equations of motion for real self-interacting scalar fields in the background o...