Heliospheric termination shock motion due to fluctuations in the solar wind upstream conditions: Spherically symmetric model

1996 ◽  
Vol 101 (A12) ◽  
pp. 27483-27497 ◽  
Author(s):  
R. Ratkiewicz ◽  
A. Barnes ◽  
G. A. Molvik ◽  
J. R. Spreiter ◽  
S. S. Stahara
Keyword(s):  
Solar Wind ◽  
Termination Shock ◽  
Symmetric Model ◽  
Spherically Symmetric ◽  
Shock Motion ◽  
Spherically Symmetric Model

MØLLER ENERGY–MOMENTUM COMPLEX FOR HIGHER-DIMENSIONAL SPHERICALLY SYMMETRIC SPACETIME IN GENERAL RELATIVITY

2012 ◽  
Vol 27 (40) ◽  
pp. 1250231 ◽  
Author(s):  
HÜSNÜ BAYSAL
Keyword(s):  
General Relativity ◽  
Momentum Density ◽  
Momentum Tensor ◽  
Symmetric Model ◽  
Spherically Symmetric ◽  
Higher Dimensional ◽  
Energy And Momentum ◽  
Momentum Complex ◽  
Spherically Symmetric Metric ◽  
Spherically Symmetric Model

We have calculated the total energy–momentum distribution associated with (n+2)-dimensional spherically symmetric model of the universe by using the Møller energy–momentum definition in general relativity (GR). We have found that components of Møller energy and momentum tensor for given spacetimes are different from zero. Also, we are able to get energy and momentum density of various well-known wormholes and black hole models by using the (n+2)-dimensional spherically symmetric metric. Also, our results have been discussed and compared with the results for four-dimensional spacetimes in literature.

scholarly journals Relativistic Zel’dovich approximation in a spherically symmetric model

1998 ◽  
Vol 57 (10) ◽  
pp. 6094-6103 ◽  
Author(s):  
Masaaki Morita ◽  
Kouji Nakamura ◽  
Masumi Kasai
Keyword(s):  
Symmetric Model ◽  
Spherically Symmetric ◽  
Spherically Symmetric Model
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