2015/06/08 by L. Herrera, Herrera, L.
Physics and Astronomy · #Cosmology and Gravitation Theories #Cosmology and Nongalactic Astrophysics (astro-ph.CO) #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Pulsars and Gravitational Waves Research #Relativity and Gravitational Theory #astro-ph.CO #gr-qc
paper · pdf · doi:10.48550/arxiv.1506.02422
Talk given at the International Conference on Relativistic Astrophysics (through Skype), Lahore, February 2015. To appear in the proceedings, to be published by Punjab University Press. 9 pages, Revtex-4
arxiv created 2015/06/08 · openalex publication_date 2015/06/08 · arxiv updated 2015/06/10 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We review a recently proposed framework for studying axially symmetric dissipative fluids \citeRef1. Some general results are discussed at the most general level. We then proceed to analyze some particular cases. First, the shear-free case is considered \cite3. We shall next discuss the perfect fluid case under the geodesic condition, without impossing ab initio the shear--free condition \cite2. Finally a dissipative, geodesic fluid \cite4, is analyzed in some detail. We conclude by bringing out the attention to some open issues.