Revista mexicana de física
versão impressa ISSN 0035-001X
In this paper, we present the results of the numerical evolution of scalar field solitons in asymptotically flat space-times. First we introduce the model we are working with and then we briefly mention the complications that arise in this particular numerical simulation, presenting some details of code we used and some examples of the results.
Palavras-chave : Numerical relativity; classical black holes and solitons.