46 research outputs found
Energy Distribution of a G\"{o}del-Type Space-Time
We calculate the energy and momentum distributions associated with a
G\"{o}del-type space-time, using the well-known energy-momentum complexes of
Landau and Lifshitz and M{\o}ller. We show that the definitions of Landau and
Lifshitz and M{\o}ller do not furnish a consistent result.Comment: LaTex, no figure
M{\o}ller Energy-Momentum Complex of a Static Axially Symmetric Vacuum Space-Time
The energy and momentum densities associated with the Weyl metric are
calculated using M{\o}ller's energy-momentum complex. These results are
compared with the results obtained by using the energy-momentum complexes of
Einstein, Landau and Lifshitz, Papapetrou and Bergmann. We show that the
aforementioned different prescriptions and that of M{\o}ller do not give the
same energy density, while give the same momentum density.Comment: LATEX, 9 pages, no figures, an improved version, references added,
corrections [Admin note: substantial overlap with gr-qc/0403097,
gr-qc/0404108 , gr-qc/0303009 , hep-th/0311050
M{\o}ller's Energy in the Kantowski-Sachs Space-time
We present a counter example to paper \cite{P71} and show that the result
obtained is correct for a class of metric but not general. We calculate the
total energy of the Kantowski-Sachs space-time by using the energy-momentum
definitions of M{\o}ller in the theory of general relativity and the tetrad
theory of gravity.Comment: 7 pages and no figure
On the Singularities of Reissner-Nordstr\"{o}m Space-Time
It is shown that if two Reissner-Nordstr\"{o}m space-times, both with the
same mass m and charge e, glued together in the singularities, then the light
ray in black hole of the first space-time can go continuously through the
singularity into black hole of the second. The behavior of tidal forces near
the Reissner-Nordstr\"{o}m space-time singularity is examined by considering
what happens between two particles falling freely towards the singularity.Comment: Latex, 4 figures, 11 page
Axially Symmetric Cosmological Mesonic Stiff Fluid Models in Lyra's Geometry
In this paper, we obtained a new class of axially symmetric cosmological
mesonic stiff fluid models in the context of Lyra's geometry. Expressions for
the energy, pressure and the massless scalar field are derived by considering
the time dependent displacement field. We found that the mesonic scalar field
depends on only coordinate. Some physical properties of the obtained models
are discussed.Comment: 13 pages, no figures, typos correcte