Space-Time Analogy of Self-Similar Intense Vortices

AIAA Journal ◽  
2006 ◽  
Vol 44 (4) ◽  
pp. 912-917 ◽  
Author(s):  
Georgios H. Vatistas ◽  
Yasser Aboelkassem
Keyword(s):  
2020 ◽  
Vol 28 (4) ◽  
pp. 326-332
Author(s):  
I. V. Kaznacheev ◽  
V. M. Kuz’kin ◽  
M. V. Kutsov ◽  
G. A. Lyakhov ◽  
S. A. Pereselkov

2005 ◽  
Vol 71 (10) ◽  
Author(s):  
Brien C. Nolan ◽  
Thomas J. Waters
Keyword(s):  
The Self ◽  

2005 ◽  
Vol 30 (22) ◽  
pp. 2973 ◽  
Author(s):  
Jesús Lancis ◽  
Víctor Torres-Company ◽  
Enrique Silvestre ◽  
Pedro Andrés

2003 ◽  
Vol 12 (04) ◽  
pp. 639-648 ◽  
Author(s):  
S. G. GHOSH ◽  
A. BANERJEE

We investigate the occurrence and nature of a naked singularity in the gravitational collapse of an inhomogeneous dust cloud described by a self-similar higher dimensional Tolman–Bondi space–time. Bound, marginally bound and unbound space–times are analyzed. The degree of inhomogeneity of the collapsing matter necessary to form a naked singularity is given.


1994 ◽  
Vol 09 (29) ◽  
pp. 2745-2754 ◽  
Author(s):  
H. J. DE VEGA ◽  
A. V. MIKHAILOV ◽  
N. SÁNCHEZ

Exact and explicit string solutions in de Sitter space-time are found. (Here, the string equations reduce to a sinh-Gordon model). A new feature without flat space-time analogy appears: starting with a single worldsheet, several (here two) strings emerge. One string is stable and the other (unstable) grows as the universe grows. Their invariant size and energy either grow as the expansion factor or tend to constant. Moreover, strings can expand (contract) for large (small) universe radius at a different rate than the universe does.


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