Energy, momentum and angular momentum conservations in de Sitter gravity
arXiv:1508.01981 · doi:10.1088/0264-9381/33/15/155009
Abstract
In de Sitter (dS) gravity, where gravity is a gauge field introduced to realize the local dS invariance of the matter field, two kinds of conservation laws are derived. The first kind is a differential equation for a dS-covariant current, which unites the canonical energy-momentum (EM) and angular momentum (AM) tensors. The second kind presents a dS-invariant current which is conserved in the sense that its torsion-free divergence vanishes. The dS-invariant current unites the total (matter plus gravity) EM and AM currents. It is well known that the AM current contains an inherent part, called the spin current. Here it is shown that the EM tensor also contains an inherent part, which might be observed by its contribution to the deviation of the dust particle's world line from a geodesic. All the results are compared to the ordinary Lorentz gravity.
13 pages, title changed
References in corpus (8)
- Invariant conserved currents in gravity theories with local Lorentz and diffeomorphism symmetry
- Snyder's Model -- de Sitter Special Relativity Duality and de Sitter Gravity
- On Principle of Inertia in Closed Universe
- Invariant conserved currents for gravity
- Invariant conserved currents in generalized gravity
- A Kaluza--Klein-like model of the gauge theory of gravity and its cosmological meaning
- Cosmological meaning of the gravitational gauge group
- Energy, momentum and angular momentum conservations in de Sitter special relativity