Inhomogeneous universe models with varying cosmological term

DOI10.1023/A:1018826426240zbMath0915.53048arXivgr-qc/9803079MaRDI QIDQ1289190

Luis P. Chimento, Diego Pavón

Publication date: 6 July 1999

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/9803079

zbMATH Keywords

varying cosmological termdecay of vacuum energyinhomogeneous spherically symmetric universe modelsmaterial fluid

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Applications of differential geometry to physics (53Z05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (4)

Dark energy problem, physics of early universe and some new approaches in gravity ⋮ Inhomogeneous cylindrically-symmetric models with varying cosmological term ⋮ Laboratory bounds for the cosmological term gradient ⋮ QUANTUM THEORY AT PLANCK SCALE, LIMITING VALUES, DEFORMED GRAVITY AND DARK ENERGY PROBLEM

Cites Work

• Unnamed Item
• Bianchi type I cosmological models with variable \(G\) and \(\Lambda\)
• Expanding models with a varying cosmological term and bulk stress
• Ideal gas sources for the Lemaître-Tolman-Bondi metrics
• Form invariance of differential equations in general relativity
• The cosmological constant problem

This page was built for publication: Inhomogeneous universe models with varying cosmological term