An approximate global stationary axisymmetric solution of the Einstein equations

Simple item page
dc.creatorMartin-Martin, J.
dc.creatorMolina, A.
dc.creatorRuiz, E.
dc.date2004-07-05
dc.date2004-08-30
dc.date.accessioned2026-07-07T03:28:49Z
dc.date.available2026-07-07T03:28:49Z
dc.descriptionIn this work we present an approximate solution of the Einstein equations describing a global model for the gravitational field generated by a bounded, self-gravitating stationary and axisymmetric body rotating rigidly with constant angular velocity.
dc.description12 pages, LaTeX, conference done at Spanish Relativity Meeting (Alicante, Spain, 2003). A few minor errata have been corrected. A formula for pressure is also added
dc.identifierhttps://arxiv.org/abs/gr-qc/0407016
dc.identifierhttp://arxiv.org/abs/gr-qc/0407016
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34981
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAn approximate global stationary axisymmetric solution of the Einstein equations
dc.typetext

Files

Collections

arXiv