Conserved Quantities in Gravity via Noether Symmetry
arXiv:1207.1008 · doi:10.1088/0256-307X/29/8/080402
Abstract
This paper is devoted to investigate gravity using Noether symmetry approach. For this purpose, we consider Friedmann Robertson-Walker (FRW) universe and spherically symmetric spacetimes. The Noether symmetry generators are evaluated for some specific choice of models in the presence of gauge term. Further, we calculate the corresponding conserved quantities in each case. Moreover, the importance and stability criteria of these models are discussed.
14 pages, accepted for publication in Chin. Phys. Lett
References in corpus (9)
- Disappearing cosmological constant in f(R) gravity
- Spherically symmetric solutions of modified field equations in f(R) theories of gravity
- Spherically symmetric solutions in f(R)-gravity via Noether Symmetry Approach
- Static spherically symmetric perfect fluid solutions in theories of gravity
- Cylindrical solutions in metric f(R) gravity
- The existence of relativistic stars in f(R) gravity
- Non-Vacuum Bianchi Types I and V in f(R) Gravity
- AdS and stabilized extra dimensions in multidimensional gravitational models with nonlinear scalar curvature terms 1/R and R^4
- Re-Scaling of Energy in the Stringy Charged Black Hole Solutions using Approximate Symmetries