scholarly journals Fully anisotropic string cosmologies, Maxwell fields, and primordial shear

1999 ◽  
Vol 59 (12) ◽  
Author(s):  
Massimo Giovannini
Keyword(s):  
2016 ◽  
Vol 25 (09) ◽  
pp. 1641011 ◽  
Author(s):  
Mengjie Wang

Perturbative methods are useful to study the interaction between black holes and test fields. The equation for a perturbation itself, however, is not complete to study such a composed system if we do not assign physically relevant boundary conditions. Recently we have proposed a new type of boundary conditions for Maxwell fields in Kerr-anti-de Sitter (Kerr-AdS) spacetimes, from the viewpoint that the AdS boundary may be regarded as a perfectly reflecting mirror, in the sense that energy flux vanishes asymptotically. In this paper, we prove explicitly that a vanishing energy flux leads to a vanishing angular momentum flux. Thus, these boundary conditions may be dubbed as vanishing flux boundary conditions.


Author(s):  
Deep Bhattacharjee

Chronology unprotected mechanisms are considered with a very low gravitational polarization to make the wormhole traversal with positive energy density everywhere. No need of exotic matter has been considered with the assumption of the Einstein-Dirac-Maxwell Fields, encountering above the non-zero stress-energy-momentum tensor through spacelike hypersurfaces by a hyperbolic coordinate shift.


1986 ◽  
Vol 18 (6) ◽  
pp. 633-640 ◽  
Author(s):  
S. Chakravarty ◽  
J. Ivancovich ◽  
E. T. Newman
Keyword(s):  

1985 ◽  
Vol 17 (7) ◽  
pp. 659-668 ◽  
Author(s):  
M. A. H. MacCallum
Keyword(s):  

1998 ◽  
Vol 39 (11) ◽  
pp. 5934-5945
Author(s):  
Matthias Wollensak

Author(s):  
H. P. Künzle

AbstractIt is shown that Huygens's principle holds for the solutions of Maxwell's equations for p-forms of all degrees in a gravitational plane wave space, while the solutions of the wave equation for 1, 2, and 3-forms, however, may have tails.


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