Global dynamics for a relativistic charged matter in the presence of a massive scalar field and the presence of a cosmological constant on Bianchi spacetimes
DOI10.1063/1.4748310zbMath1278.83047OpenAlexW2045760054WikidataQ126005099 ScholiaQ126005099MaRDI QIDQ2872292
Norbert Noutchegueme, Alexis Nangue
Publication date: 14 January 2014
Published in: Journal of Mathematical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1063/1.4748310
Asymptotic behavior of solutions to PDEs (35B40) Geometrodynamics and the holographic principle (83E05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) PDEs in connection with relativity and gravitational theory (35Q75) Einstein-Maxwell equations (83C22)
Cites Work
- The Einstein-Vlasov system with a scalar field
- Asymptotic behavior of homogeneous cosmological models in the presence of a positive cosmological constant
- Cosmic no-hair theorem in homogeneous spacetimes. I. Bianchi models
- Accelerated cosmological expansion due to a scalar field whose potential has a positive lower bound
- Introduction to 3+1 Numerical Relativity
- The Large Scale Structure of Space-Time
- General Relativity
This page was built for publication: Global dynamics for a relativistic charged matter in the presence of a massive scalar field and the presence of a cosmological constant on Bianchi spacetimes
