A Comment on the plane symmetric solution of Einstein equations

1970 ◽  
Vol 20 (9) ◽  
pp. 1053-1054
Author(s):  
J. Horský ◽  
M. Lenc





2009 ◽  
Vol 671 (4-5) ◽  
pp. 428-434 ◽  
Author(s):  
Hongsheng Zhang ◽  
Hyerim Noh


1985 ◽  
Vol 17 (10) ◽  
pp. 1001-1013 ◽  
Author(s):  
Li jian-zeng ◽  
Liang can-bin


1985 ◽  
Vol 2 (1) ◽  
pp. 23-26 ◽  
Author(s):  
Li Jian-zeng ◽  
Liang Can-bin


2016 ◽  
Vol 94 (2) ◽  
pp. 177-179
Author(s):  
L.A. López ◽  
Omar Pedraza ◽  
V.E. Ceron

We present a three-parameter time-dependent solution of the vacuum Einstein equations in five dimensions. The solution is obtained by applying the Wick rotation to the Myers–Perry solution that represents a rotating black hole in five dimensions. The new interpretation of the Myers–Perry solution can be considered among the generalized Einstein–Rosen type that can be interpreted as plane-symmetric waves, cylindrical waves or cosmological space–time in five dimensions. In some limits the solution has boost-rotational symmetry and it is asymptotically flat. In the case that the solution represents a cylindrical space–time, the E-energy is analyzed.



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