Constraint Relaxation

dc.creatorMarronetti, Pedro
dc.date2006-12-28
dc.date.accessioned2026-07-07T07:40:25Z
dc.date.available2026-07-07T07:40:25Z
dc.descriptionFull relativistic simulations in three dimensions are known to develop runaway modes that grow exponentially and are accompanied by violations of the Hamiltonian and momentum constraints. We present here a method that controls the violation of these constraints and is tested with simulations of binary neutron stars in circular orbits. We show that this technique improves the overall quality of the simulations.
dc.description3 pages. To appear in the Proceedings of the Eleventh Marcel Grossmann Meeting, Berlin, Germany, 23-29 Jule 2006, World Scientific, Singapore (2007)
dc.identifierhttps://arxiv.org/abs/gr-qc/0612181
dc.identifierhttp://arxiv.org/abs/gr-qc/0612181
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/121768
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleConstraint Relaxation
dc.typetext

Files

Collections