The velocity field distribution for rigid motions in the Born?s sense applied to Post-Newtonian Relativistic Celestial Mechanics is examined together with its compatibility with the Newtonian distribution.
Se examinan la distribución del campo de velocidades para movimientos rígidos en el sentido de Born aplicado a la mecánica celeste Post-Newtoniana junto con su compatibilidad con la distribución Newtoniana.
@article{urn:eudml:doc:40963, title = {A theorem for rigid motions in Post-Newtonian celestial mechanics.}, journal = {RACSAM}, volume = {97}, year = {2003}, pages = {113-118}, mrnumber = {MR2037229}, zbl = {1229.70036}, language = {en}, url = {http://dml.mathdoc.fr/item/urn:eudml:doc:40963} }
Gambi, J.M.; Zamorano, P.; Romero, P.; García del Pino, M.L. A theorem for rigid motions in Post-Newtonian celestial mechanics.. RACSAM, Tome 97 (2003) pp. 113-118. http://gdmltest.u-ga.fr/item/urn:eudml:doc:40963/