2010/01/14 by J.‐F. Pascual‐Sánchez, J. -F. Pascual-Sánchez, A. San Miguel +5
Physics and Astronomy · #Cosmology and Gravitation Theories #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Instrumentation and Methods for Astrophysics (astro-ph.IM) #Pulsars and Gravitational Waves Research #Relativity and Gravitational Theory #astro-ph.IM #gr-qc
paper · pdf · doi:10.48550/arxiv.1001.2550
3 pages, 1 fig, Talk given by JFPS at the 12th Marcel Grossmann conference (Paris, July, 2009), submitted to the Proceedings
arxiv created 2010/01/14 · openalex publication_date 2010/01/14 · arxiv updated 2010/02/26 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The geometry of a light wavefront evolving from a flat wavefront under the action of weak gravity field in the 3-space associated to a post-Newtonian relativistic spacetime, is studied numerically by means of the ray tracing method.