scholarly journals Geodesics near a curvature singularity of stationary and axially symmetric space-times

Author(s):  
Juan Carlos Del Águila Rodríguez ◽  
Tonatiuh Matos
2010 ◽  
Vol 81 (8) ◽  
Author(s):  
Miguel Zilhão ◽  
Helvi Witek ◽  
Ulrich Sperhake ◽  
Vitor Cardoso ◽  
Leonardo Gualtieri ◽  
...  

2017 ◽  
Vol 14 (04) ◽  
pp. 1750053 ◽  
Author(s):  
Saeed Nayeh ◽  
Mehrdad Ghominejad

In this paper, we obtain the field equations of Weyl static axially symmetric space-time in the framework of [Formula: see text] gravity, where [Formula: see text] is torsion scalar. We will see that, for [Formula: see text] related to teleparallel equivalent general relativity, these equations reduce to Einstein field equations. We show that if the components of energy–momentum tensor are symmetric, the scalar torsion must be either constant or only a function of radial component [Formula: see text]. The solutions of some functions [Formula: see text] in which [Formula: see text] is a function of [Formula: see text] are obtained.


2016 ◽  
Vol 94 (11) ◽  
pp. 1148-1152
Author(s):  
Ragab M. Gad ◽  
A.E. Al Mazrooei

This paper investigates axially symmetric space–times that admit a homothetic vector field based on Lyra’s geometry. The cases when the displacement vector is a function of t and when it is constant are studied. In the context of this geometry, we find and classify the solutions of the Einstein’s field equations for the space–time under consideration, which display a homothetic symmetry.


1988 ◽  
Vol 66 (4) ◽  
pp. 338-340
Author(s):  
M. D. Roberts

An attempt is made to introduce dipole structure into gravitational theory. We do this by trying to produce torsion tensors with the same form as the electric-field tensor for an electric dipole. First, we construct Ricci tensors for space-times with vanishing Christoffel connections. Then we discuss the conditions to put on the tensors. Each condition gives differential equations; however, none of the solutions provides an entirely satisfactory dipole structure. Finally, we briefly discuss how to "force" axially symmetric space-times having dipole structure.


Microwaves ◽  
1963 ◽  
pp. 610-615
Author(s):  
D. A. Dunn ◽  
R. P. Borghi ◽  
R. C. Morwood

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