Characterizing implications of two-dimensional space–time orientations for principal component analysis of geographic time series

2015 ◽  
Vol 36 (1) ◽  
pp. 290-299 ◽  
Author(s):  
Neeti Neeti ◽  
J. Ronald Eastman
2009 ◽  
Vol 18 (04) ◽  
pp. 599-611 ◽  
Author(s):  
ALFRED MOLINA ◽  
NARESH DADHICH

By considering the product of the usual four-dimensional space–time with two dimensional space of constant curvature, an interesting black hole solution has recently been found for Einstein–Gauss–Bonnet gravity. It turns out that this as well as all others could easily be made to radiate Vaidya null dust. However, there exists no Kerr analog in this setting. To get the physical feel of the four-dimensional black hole space–times, we study asymptotic behavior of stresses at the two ends, r → 0 and r → ∞.


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