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

Mathematics Subject Classification ID

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

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