scholarly journals Nonminimal black holes with regular electric field

2015 ◽  
Vol 24 (09) ◽  
pp. 1542009 ◽  
Author(s):  
Alexander B. Balakin ◽  
Alexei E. Zayats

We discuss the problem of identification of coupling constants, which describe interactions between photons and spacetime curvature, using exact regular solutions to the extended equations of the nonminimal Einstein–Maxwell theory. We argue the idea that three nonminimal coupling constants in this theory can be reduced to the single guiding parameter, which plays the role of nonminimal radius. We base our consideration on two examples of exact solutions obtained earlier in our works: the first of them describes a nonminimal spherically symmetric object (star or black hole) with regular radial electric field; the second example represents a nonminimal Dirac-type object (monopole or black hole) with regular metric. We demonstrate that one of the inflexion points of the regular metric function identifies a specific nonminimal radius, thus marking the domain of dominance of nonminimal interactions.

2020 ◽  
Vol 2020 (9) ◽  
Author(s):  
Zachary Elgood ◽  
Patrick Meessen ◽  
Tomás Ortín

Abstract We re-derive the first law of black hole mechanics in the context of the Einstein-Maxwell theory in a gauge-invariant way introducing “momentum maps” associated to field strengths and the vectors that generate their symmetries. These objects play the role of generalized thermodynamical potentials in the first law and satisfy generalized zeroth laws, as first observed in the context of principal gauge bundles by Prabhu, but they can be generalized to more complex situations. We test our ideas on the d-dimensional Reissner-Nordström-Tangherlini black hole.


2002 ◽  
Vol 67 (5) ◽  
pp. 301-308 ◽  
Author(s):  
V. S. TSYPIN ◽  
R. M. O. GALVÃO ◽  
I. C. NASCIMENTO ◽  
M. TENDLER ◽  
J. H. F. SEVERO ◽  
...  

Absorption by trapped particles is supposed to seriously hinder current drive by Alfvén waves. However, it is shown in this paper that the same effect is rather beneficial for the emergence of the radial electric field induced by these waves, which is important for creating and maintaining transport barriers in tokamaks.


1998 ◽  
Vol 5 (6) ◽  
pp. 2390-2398 ◽  
Author(s):  
M. G. Shats ◽  
C. A. Michael ◽  
D. L. Rudakov ◽  
B. D. Blackwell

1994 ◽  
Vol 1 (5) ◽  
pp. 1536-1544 ◽  
Author(s):  
K. H. Burrell ◽  
E. J. Doyle ◽  
P. Gohil ◽  
R. J. Groebner ◽  
J. Kim ◽  
...  

Author(s):  
M. B. Tataryn ◽  
M. M. Stetsko

A three-dimensional slowly rotating black hole solution in the presence of negative cosmological constant in the Einstein-power-Maxwell theory is studied. It is shown that in the small rotation limit, the electric field, diagonal metric function and thermodynamic properties are the same as for static case, whereas the small rotation gives in addition a nondiagonal metric function and magnetic field which are also small. For these functions cased by rotation of black hole, exact integral solution and analytic asymptotic solution were obtained.


1997 ◽  
Vol 39 (12B) ◽  
pp. B273-B286 ◽  
Author(s):  
R Brakel ◽  
M Anton ◽  
J Baldzuhn ◽  
R Burhenn ◽  
V Erckmann ◽  
...  

2020 ◽  
Vol 2020 (10) ◽  
Author(s):  
Pablo A. Cano ◽  
Ángel Murcia

Abstract We identify a set of higher-derivative extensions of Einstein-Maxwell theory that allow for spherically symmetric charged solutions characterized by a single metric function f (r) = −gtt = 1/grr. These theories are a non-minimally coupled version of the recently constructed Generalized Quasitopological gravities and they satisfy a number of properties that we establish. We study magnetically-charged black hole solutions in these new theories and we find that for some of them the equations of motion can be fully integrated, enabling us to obtain analytic solutions. In those cases we show that, quite generally, the singularity at the core of the black hole is removed by the higher-derivative corrections and that the solution describes a globally regular geometry. In other cases, the equations are reduced to a second order equation for f (r). Nevertheless, for all the theories it is possible to study the thermodynamic properties of charged black holes analytically. We show that the first law of thermodynamics holds exactly and that the Euclidean and Noether-charge methods provide equivalent results. We then study extremal black holes, focusing on the corrections to the extremal charge-to-mass ratio at a non-perturbative level. We observe that in some theories there are no extremal black holes below certain mass. We also show the existence of theories for which extremal black holes do not represent the minimal mass state for a given charge. The implications of these findings for the evaporation process of black holes are discussed.


2000 ◽  
Vol 7 (2) ◽  
pp. 615-625 ◽  
Author(s):  
D. R. Ernst ◽  
R. E. Bell ◽  
M. G. Bell ◽  
R. V. Budny ◽  
B. Coppi ◽  
...  

2007 ◽  
Vol 47 (8) ◽  
pp. 762-772 ◽  
Author(s):  
A.V Chankin ◽  
D.P Coster ◽  
N Asakura ◽  
G Corrigan ◽  
S.K Erents ◽  
...  

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