It appears you don't have support to open PDFs in this web browser. To view this file, Open with your PDF reader
Abstract
We present a new excision technique used in constrained formulations of Einstein equations to deal with black hole in numerical simulations. We show the applicability of this scheme in several scenarios. In particular, we present the dynamical evolution of the collapse of a neutron star to a black hole, using the CoCoNuT code and this excision technique.
You have requested "on-the-fly" machine translation of selected content from our databases. This functionality is provided solely for your convenience and is in no way intended to replace human translation. Show full disclaimer
Neither ProQuest nor its licensors make any representations or warranties with respect to the translations. The translations are automatically generated "AS IS" and "AS AVAILABLE" and are not retained in our systems. PROQUEST AND ITS LICENSORS SPECIFICALLY DISCLAIM ANY AND ALL EXPRESS OR IMPLIED WARRANTIES, INCLUDING WITHOUT LIMITATION, ANY WARRANTIES FOR AVAILABILITY, ACCURACY, TIMELINESS, COMPLETENESS, NON-INFRINGMENT, MERCHANTABILITY OR FITNESS FOR A PARTICULAR PURPOSE. Your use of the translations is subject to all use restrictions contained in your Electronic Products License Agreement and by using the translation functionality you agree to forgo any and all claims against ProQuest or its licensors for your use of the translation functionality and any output derived there from. Hide full disclaimer
Details
1 Department of Applied Mathematics, University of Valencia, C/ Dr. Moliner 50, E-46100 Burjassot, Spain; Laboratoire Univers et Théories (LUTH), Observatoire de Paris/CNRS/Université Paris Diderot, 5 place Jules Janssen, F-92190 Meudon, France
2 Laboratoire Univers et Théories (LUTH), Observatoire de Paris/CNRS/Université Paris Diderot, 5 place Jules Janssen, F-92190 Meudon, France
3 Université de Bretagne Occidentale, 6 ave. Le Gorgeu, CS 93837, 29238 Brest Cedex 3, France