A note on the flow equations under space-time transformation

Author(s):  
Z.-N. Wu
2011 ◽  
Vol 08 (05) ◽  
pp. 1031-1077
Author(s):  
RAJU ROYCHOWDHURY

Following the same treatment of Bellucci et al. we obtain, the hitherto unknown general solutions of the radial attractor flow equations for extremal black holes, both for non-BPS with non-vanishing and vanishing central charge Z for the so-called st2 model, the minimal rank-two [Formula: see text] symmetric supergravity in d = 4 space-time dimensions. We also make useful comparisons with results that already exist in literature, and introduce the fake supergravity (first-order) formalism to be used in our analysis. An analysis of the BPS bound all along the non-BPS attractor flows and of the marginal stability of corresponding D-brane charge configurations has also been presented.


JETP Letters ◽  
2009 ◽  
Vol 89 (11) ◽  
pp. 535-539 ◽  
Author(s):  
I. V. Blonskii ◽  
V. N. Kadan ◽  
O. I. Shpotyuk ◽  
I. N. Dmitruk ◽  
I. A. Pavlov

2020 ◽  
Vol 59 (28) ◽  
pp. 8595
Author(s):  
Shuo Zhang ◽  
Lipeng Sun ◽  
Yongran Chen ◽  
Yong Bi

2015 ◽  
Author(s):  
Viktor P. Galileiskii ◽  
Alexey I. Elizarov ◽  
Dmitrii V. Kokarev ◽  
Aleksandr M. Morozov

Wave Motion ◽  
2014 ◽  
Vol 51 (5) ◽  
pp. 785-797 ◽  
Author(s):  
C. García-Meca ◽  
S. Carloni ◽  
C. Barceló ◽  
G. Jannes ◽  
J. Sánchez-Dehesa ◽  
...  

2002 ◽  
Vol 17 (17) ◽  
pp. 2369-2376 ◽  
Author(s):  
A. IORIO ◽  
T. SÝKORA

We study the space–time symmetries and transformation properties of the non-commutative U(1) gauge theory, by using Noether charges. We carry out our analysis by keeping an open view on the possible ways θμν could transform. Since the theory is not invariant under the conformal transformations, with the only exception of space–time translations, we conclude that the most natural and dynamically consistent requirement is that θμν does not transform under any space–time transformation. A similar analysis should apply to other gauge groups.


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