Speaker
Mr
Nikolaos Chatzarakis
(Aristotle University of Thessaloniki)
Description
Following the generalised form of non-stationary axisymmetric space-time (Chandrasekhar 1983), we assume a bifocale elliptic symmetry and attempt to show that this particular metric can be a solution to Einstein's field equations. We discuss the form of the metric and the curvature implied, as well as its possible physical meaning and applications.
Primary author
Mr
Nikolaos Chatzarakis
(Aristotle University of Thessaloniki)
