# Basic Generic Properties of Regular Rotating Black Holes and Solitons.

1. Introduction

Presented in the current literature, regular rotating solutions [1-10] are obtained from regular spherical solutions with using the Newman-Janis complex translation . In , it was shown that the Newman-Janis translation works for algebraically special metrics which belong to the Kerr-Schild class  and can be presented as [g.sub.[mu]v] = [[eta].sub.[mu]v] + 2f(r)[k.sub.[mu][k.sub.v], where [[eta].sub.[mu]v] is the Minkowski metric and [k.[mu]] are principal null congruences. More general approach, with using basic properties of metrics from the Kerr-Schild class, was applied for obtaining the axially symmetric solutions in the noncommutative geometry .

Spherical metrics of the Kerr-Schild class have the form 

[mathematical expression not reproducible], (1)

where

[mathematical expression not reproducible], (2)

and are generated by stress-energy tensors satisfying [15-18]

[T.sup.t.sub.t] = [T.sup.r.sub.r]. (3)

The energy density is [rho] = [T.sup.t.sub.t], the radial pressure [p.sub.r] = - [T.sup.r.sub.r], and the transversal pressure [p.sub.[perpendicular to] = - [T.sup.[theta].sub.[theta]] = -[T.sup.[phi].sub.[phi]]. Equation (3) represents the radial part of the r-dependent equation of state, [p.sub.r] = -[rho]. The contracted Bianchi identities ([T.sup.v.[mu];v] = 0) yield the second part of the r-dependent equation of state, [p.sub.[perpendicular to]] = -[rho] - (r/2) [rho]' [15, 19].

All regular spherical solutions of this class, satisfying the weak energy condition (nonnegative density as measured by any local observer on a time-like curve), have obligatory de Sitter center, [[T.sup.v.sub.[mu]] [right arrow] [[rho].sub.0] [[[delta].sup.v.sub.[mu]]; g(r) [right arrow] 1 - [r.sup.2]/[r.sup.2.sub.0] as r [right arrow] 0 with [r.sup.2.sub.0] = 3/(8[pi]G[[rho].sub.0]) [18, 20].

Gurses and Gursey have found that the algebraically special metrics of the Kerr-Schild class can be presented in the Lorentz covariant coordinate system, developed the general approach based on the complex Trautman-Newman techniques (which include the Newman-Janis translation), and derived the axially symmetric metric in the general, model-independent form. In the Boyer-Lindquist coordinates the metric reads 

[mathematical expression not reproducible], (4)

[DELTA] = [r.sup.2] - 2f(r) + [a.sup.2]; [summation] = [r.sup.2] + [a.sup.2] [cos.sup.2] [theta]. (5)

It involves a master function

f(r) = r M (r) (6)

which comes from a spherically symmetric solution (2). For f(r) = Mr - [q.sup.2]/2, it describes the Kerr-Newman geometry , where M is the mass parameter and q is the electric charge. The case q = 0 corresponds to the Kerr geometry . Each of these two geometries can have at most two horizons, the solutions without horizons describe naked singularities.

The parameter r in (4) is defined as an affine parameter along a principal null congruence. The surfaces of constant r are the confocal ellipsoids of revolution 

[r.sup.4] -([x.sup.2] + [y.sup.2] + [z.sup.2] - 2a)[r.sup.2] - [a.sup.2] [z.sup.2] = 0 (7)

which degenerate, for r = 0, to the equatorial disk

[x.sup.2] + [y.sup.2] [less than or equal to] [a.sup.2], z = 0, (8)

centered on the symmetry axis and bounded by the ring [x.sup.2] + [y.sup.2] = [a.sup.2], z = 0 (in the Kerr and Kerr-Newman geometries, it comprises their ring singularities).

Regular axially symmetric solutions satisfy condition (3) in the corotating reference frame [24,25] and describe regular rotating objects, asymptotically Kerr or Kerr-Newman for a distant observer with the mass parameter M = M(r [right arrow] [infinity]). Solutions of this class describe regular rotating black holes and spinning solitons with de Sitter vacuum interiors [25-28]. Rotation transforms de Sitter center of regular spherical solutions into de Sitter vacuum disk (8). All regular solutions presented in the literature belong to this class. Most of them are devoted to study of particular solutions specified by a choice of the mass function M(r) in (2).

In this paper, we present a systematic review of the basic generic properties of regular rotating black holes and spinning solitons replacing naked singularities and defined in the spirit of Coleman lumps  as nonsingular nondissipative objects without horizons keeping themselves together by their own self-interaction. For convenience and transparency in analysis of various aspects of generic behavior, we use the geometrized units c = G = 1. Conversion factors and instructions for transition to different nongeometrized units can be found in .

The paper is organized as follows. In Section 2, we present horizons, ergospheres, and ergoregions. Section 3 is devoted to basic physical properties of regular interiors. Section 4 outlines behavior of electromagnetic fields in the case of electrically charged regular black holes and electromagnetic solitons. In Section 5, we summarize and discuss the results.

2. Horizons, Ergospheres, and Ergoregions

The basic features of regular rotating objects are closely related to generic properties of related regular spherical solutions (1)-(2).

Horizons are defined by [DELTA](r) = 0. The function [DELTA](r) can be written as

[DELTA] (r) = [r.sup.2] + [a.sup.2] - 2f (r) = [a.sup.2] + [r.sup.2] g (r). (9)

It follows that [DELTA] = [a.sup.2] at zero points of the metric function g(r), g(r) = 0, and evolves from [DELTA] = [a.sup.2] as r = 0 to [DELTA] [right arrow] [infinity] as r [right arrow] [infinity].

A spherical metric function g(r) in (2) in the asymptotically flat case can have at most two zero points and one minimum between them . Typical behavior of a spherical metric function g(r) is shown in Figure 1.

Derivatives of [DELTA] are [DELTA]' = 2rg(r) + [r.sup.2] g'(r); [DELTA]" = 2g(r) + 4rg'(r) + r g" (r). At r = 0 derivatives take the values [DELTA]' = 0; [DELTA]" = 2 and the function [DELTA] has the minimum, [DELTA] = [a.sup.2]. Next it grows and can have maximum at a certain value [r.sub.m] < [r.sub.1], where [r.sub.1] is the 1st zero of the function g(r). At the maximum [DELTA]'([r.sub.m]) = 0 and hence g'([r.sub.m]) = - 2g([r.sub.m])/[r.sub.m], second derivative [DELTA]"([r.sub.m]) = -6g([r.sub.m]) + [r.sup.2.sub.m] g"([r.sub.m]) < 0. After passing the maximum, decreasing [DELTA] achieves [DELTA] = [a.sup.2] at the 1st zero of g(r); then it will achieve this value at the 2nd zero point [r.sub.2] of g(r). The function g(r) < 0 between its zeros and has the minimum. In this region, g'(r) is first negative and then passes zero and becomes positive; hence, g" [greater than or equal to] 0 everywhere between zeros of g(r), while g [less than or equal to] 0; as a result, [DELTA]" [greater than or equal to] 0 everywhere in this region, so that the function [DELTA](r) can have only minimum and only one. At r > [r.sub.2] we have g(r) > 0 and g' > 0 so that [DELTA] cannot vanish. Since the function g(r) has at most two zero points, axially symmetric space-time can have at most two horizons, the event horizon [r.sub.+] and the internal Cauchy horizon [r.sub.-] < [r.sub.+] [27, 28].

Ergosphere is a surface of a static limit [g.sub.tt] = 0 given by

[g.sub.tt] (r, [theta]) = [r.sup.2] + [a.sup.2] [cos.sup.2] [theta] - 2f (r) = 0. (10)

Ergoregions are defined by [g.sub.tt] < 0 which makes possible extraction of rotational energy (see, e.g.,  and references therein).

Each point of the ergosphere belongs to some of confocal ellipsoids (7) covering the whole space as the coordinate surfaces r = const. The Cartesian coordinates satisfy z = r cos [theta]; [x.sup.2] + [y.sup.2] = ([a.sup.2] + [r.sup.2])[sin.sup.2] [theta]. It follows from (10) that [z.sup.2] = (2[r.sup.2]f(r) - [r.sup.4])/[a.sup.2] on the ergosphere.

There are four cases for the existence of ergospheres and ergoregions shown in Figure 2. The width of the ergosphere at a certain z is [x.sup.2] + [y.sup.2] = ([a.sup.2] + [r.sup.2])(1 - [z.sup.2]/[r.sup.2]). In the equatorial plane [x.sup.2] + [y.sup.2] = [a.sup.2] + [r.sup.2] and [z.sup.2] = 0 [right arrow] 2f(r) - [r.sup.2] = 0. For any regular density profile, the function f(r) (curves (3), (4) in Figure 2) is everywhere nonnegative and monotonically grows from f(r) = 4[pi][[rho].sub.0][r.sup.4]/3 at r [right arrow] 0 . Ergosphere exists when the curve u = 2f(r) intersects or touches the parabola u = [r.sup.2] (curves (2) in Figure 2). It is evident that in this case the curve u = 2f(r) intersects also the (situated above) parabola u = [r.sup.2] + [a.sup.2] [cos.sup.2] [theta] for a given [theta] (curves (1)).

In the black hole case, ergospheres and ergoregions exist for any density profile (the curve (3a) for the case of two horizons and the curve (3b) for the double-horizon case). In the case of a soliton the existence of ergospheres depends on the density profile. Solitons can have two ergospheres and ergoregion between them (the curve (4a)), one ergosphere and ergoregion involving the whole interior (the curve (4b)), or no ergospheres [27, 28].

3. Internal Structure of Regular Rotating Objects

3.1. Density and Pressures. The anisotropic stress-energy tensor responsible for (4) can be written in the form 

[mathematical expression not reproducible] (11)

[mathematical expression not reproducible]. (12)

The sign plus refers to the regions outside the event horizon and inside the Cauchy horizon where the vector [u.sup.[mu]] is time-like, and the sign minus refers to the regions between the horizons where the vector F is time-like. The vectors [m.sup.[mu]] and [n.sup.[mu]] are space-like in all regions.

The eigenvalues of the stress-energy tensor (11), calculated in the corotating references frame where each of ellipsoidal layers of constant r rotates with the angular velocity [omega](r) = [u.sup.[phi]]/[u.sup.t] = a/([r.sup.2] + [a.sup.2]) , are defined by

[mathematical expression not reproducible] (13)

in the regions outside the event horizon and inside the Cauchy horizon where density is defined as the eigenvalue corresponding to the time-like eigenvector [u.sup.[mu]].

The eigenvalues of the stress-energy tensor are related to the master function f(r) as 

[mathematical expression not reproducible], (14)

where [kappa] = 8[pi]G. It follows that

[mathematical expression not reproducible], (15)

where [??](r) is the related spherical density. In the corotating frame, we thus have

[mathematical expression not reproducible]. (16)

3.2. De Sitter Disk. Near the disk (8) the function f(r) in (4) approaches de Sitter asymptotic 2f(r) [right arrow] [r.sup.4]/[r.sup.2.sub.0]; [r.sup.2.sub.0] = 3/(8[pi]G[[??].sub.0]). Taking into account [summation] = ([r.sup.4] + [a.sup.2] [z.sup.2])[r.sup.-2], we get in the equatorial plane [r.sup.2]/[summation] [right arrow] 1 as z [right arrow] 0, and (16) reduces to 

([p.sub.[perpendicular to]] + [rho]) = -r[??]'(r)/2. (17)

For the regular spherical solutions satisfying the weak energy condition [??]' [less than or equal to] 0, and regularity requires r[??]'(r) [right arrow] 0 as r [right arrow] 0 . Then [p.sub.[perpendicular to]] = -[rho], and the equation of state on the disk

P = -[rho] (18)

represents the rotating de Sitter vacuum in the corotating frame . According to (15), the density in the equatorial plane is [rho](r, [theta]) = [??](r). When r [right arrow] 0, [??](r) [right arrow] [[??].sub.0], so that on the equatorial disk [rho](r, [theta]) = [[??].sub.0](r).

3.3. Two Types of Interiors. In , it was suggested that rotation should inevitably lead to violation of the weak energy condition in interior regions of regular rotating structures. Violation of the weak energy condition was found for regular rotating solutions obtained with the Newman-Janis algorithm from particular spherical metrics [3, 4] and for a solution found by postulating a metric [g.sub.[mu]v] and calculating [T.sub.[mu]v] from the Einstein equations .

In our papers [27, 28] we have studied the weak energy condition for rotating regular structures on general setting and found the existence of two kinds of regular interiors, one preserving and the other violating the weak energy condition.

The weak energy condition is valid if and only if [rho] [greater than or equal to] 0 and [p.sub.[perpendicular to]] + [rho] [greater than or equal to] 0 . The first condition is satisfied according to (15). The general equation (16) for [p.sub.[perpendicular to]] + [rho] can be written as

[mathematical expression not reproducible]. (19)

It implies a possibility for generic violation of the weak energy condition beyond the de Sitter vacuum surface S(r,z) = 0,on which [p.sub.[perpendicular to]] + [rho] = 0 and the right-hand side in (19) can change its sign. It can be expressed through the pressure of a related spherical solution, [mathematical expression not reproducible], which gives

[mathematical expression not reproducible]. (20)

As we see, the existence of vacuum surfaces and hence the violation of the weak energy condition beyond them is possible if and only if a related spherical solution satisfies the dominant energy condition  ([??] [greater than or equal to] [[??].sub.k] in (20)). In the case when a related spherical solution violates the dominant energy condition, the weak energy condition is preserved for a rotating solution.

Regular Interiors Satisfying the Weak Energy Condition. In this case [??] < [[??].sub.[perpendicular to]], hence P(r) [less than or equal to] 0, and the function S(r, z) in (20) vanishes only at approaching the disk r = 0. In this case the interior region looks as shown in Figure 3  where we also plotted two horizons defined by the roots of the equation [r.sup.2] + [a.sup.2] - 2f(r) = 0, the event and the internal horizons r = [r.sub.+], r = [r.sub.-], respectively, and the ergosphere satisfying [r.sup.2] + [a.sup.2] [cos.sup.2] [theta] - 2f(r) = 0.

Regular Interiors Violating the Weak Energy Condition. In the case when P(r) [greater than or equal to] 0, there can in principle exist S- surface at which [p.sub.[perpendicular to]] + [rho] = 0 and beyond which the weak energy condition is violated. On the S-surface [z.sup.2] = [r.sup.4]/P(r) and hence [r.sup.2] = [absolute value of z] [square root of P(r)]. The squared width of the S-surface, [mathematical expression not reproducible]. The squared width of the ellipsoid r = [[absolute value of z].sub.max] = [r.sub.e] is [W.sup.2.sub.e] = ([a.sup.2] + [r.sup.2.sub.e])(1 - [z.sup.2]/[r.sup.2.sub.e]). The difference [mathematical expression not reproducible]. Assume that [W.sub.S] > [W.sub.e] for some value of z; it means that there exists a ring specified by [absolute value of z] < [[absolute value of z].sub.max] which belongs to the ellipsoid r = [r.sub.e], where these two surfaces intersect and where thus [absolute value of z] [square root of (P([r.sub.e]))]/[r.sup.2.sub.e] = 1. As a result, [absolute value of z] = [r.sup.2.sub.e]/[square root of (P([r.sub.e]))] = [[absolute value of z].sub.max], so that these two surfaces can only touch each other on the poles and hence never cross. It follows that the S-surface is always entirely confined within the ellipsoid defined by [[absolute value of z].sub.max] = [r.sub.e] = [r.sup.2.sub.e]/[square root of (P([r.sub.e]))] and contains the disk r = 0 as a bridge.

For regular spherical solutions r[??]' [right arrow] 0, [[??].sub.[perpendicular to]] [right arrow] -[??] as r [right arrow] 0, and in the most general case P(r) [right arrow] [A.sup.2] [r.sup.-(n+1)] with the integer n [greater than or equal to] 0 as r [right arrow] 0. As a result the derivative of [W.sub.S] (z) near z [right arrow] 0 behaves as [z.sup.-(n+3)/(n+5)] and goes to [+ or - ][infinity] as z [right arrow] 0, so that the function [W.sub.S](z) has the cusp at approaching the disk and at least two symmetric (with respect to the equatorial plane) maxima between z = [+ or -] [absolute value of [z.sub.max]] and z = 0. Typical form of the de Sitter S-surface for the second type of interior is shown in Figure 4 [27, 28].

In the cavities between its upper and down boundaries and the bridge [p.sub.[perpendicular to]] + [rho] < 0, the weak energy condition is violated and cavities are filled with a phantom energy which is defined by the condition p + [rho] < 0 ; in the considered case, it is satisfied for [p.sub.[perpendicular to]].

As we have shown, the form of the de Sitter S-surfaces is generic. Here we plotted it for the particular exact solution [27, 28] which originates from the spherically symmetric solution 

[mathematical expression not reproducible], (21)

with a phenomenologically regularized Newtonian  or Coulomb  density profile, dependent on identification of the parameter [B.sup.2]/[r.sup.4.sub.v] = [[??].sub.0] which represents the cut- off on self-interaction energy by the de Sitter vacuum density [[??].sub.0] at r = 0. The density [[??].sub.0] is related to the mass M by the formula M = (4[pi]/3)[[??].sub.0] [r.sup.2.sub.0] [r.sub.g] = (4[pi]/3)[[??].sub.0] [r.sup.3.sub.*]. The length scale [r.sub.*] = [([r.sup.2.sub.0] [r.sub.g]).sup.1/3] which appears here in the natural way is characteristic for a geometry with the de Sitter interior and the Schwarzschild exterior [15, 17, 19].

Relation between the width of the S-surface in the equatorial plane [W.sub.S] = a and its height [H.sub.S] = [[absolute value of z].sub.max] = [square root of ([ar.sub.v])], defines the form of the S-surface by the oblateness parameter [eta] = [H.sub.S]/[W.sub.S]. For [eta] < 1 the S-surface is oblate (shown in Figure 4). It can be the case of electrically neutral quickly rotating de Sitter-Kerr blackholes and solitons . For [eta] > 1 the de Sitter S-surface is prolate; it maybe the case of a slowly rotating black hole (more details in [27, 28]).

4. Electrically Charged Regular Black Holes and Solitons

4.1. Basic Equations. Objects related by the electromagnetic and gravitational interaction are governed by nonlinear electrodynamics coupled to gravity.

Nonlinear electrodynamics was proposed by Born and Infeld as founded on two basic principles: to consider electromagnetic field and particles within the frame of one physical entity which is electromagnetic field and to avoid letting physical quantities become infinite . In this theory, finite values of the field energy are achieved by imposing an upper limit on the electric field, but geometry remains singular.

The program based on two above principles can be realized in nonlinear electrodynamics coupled to gravity (NED-GR) in the frame of the standard minimal coupling of gravitational and electromagnetic field, that is, without introducing some hypothetical nonminimal coupling which could be essential at the Planck energies, since in the modern string/M-theories nonlinear electrodynamics appears as low-energy effective limits [35, 36].

Electrically charged regular objects are described by the source-free NED-GR equations. The source of the gravitational fields in the Einstein equations is the stress-energy tensor of a nonlinear electromagnetic field.

For any gauge-invariant Lagrangian L(F), stress-energy tensor of electromagnetic field reads

[mathematical expression not reproducible], (22)

where [F.sub.[mu]v] = [[partial derivative].sub.[mu]] [A.sub.v] - [[partial derivative].sub.v] [A.sub.[mu]] and [L.sub.F] = dL/dF. In the spherically symmetric case, it has the algebraic structure (3) and metrics belong to the Kerr-Schild class (2).

Nonlinear electrodynamics minimally coupled to gravity is described by the action

[mathematical expression not reproducible] (23)

where R is the scalar curvature and g is the determinant of the metric tensor. The Lagrangian L(F) is an arbitrary function of F which should have the Maxwell limit, L [right arrow] F, [L.sub.F] [right arrow] 1, in the weak field regime. Variation with respect to [A.sup.[mu]] and [g.sub.[mu]v] yields the dynamic equations

[[nabla].sub.[mu]]([L.sub.F] [F.sup.[mu]v]) = 0; [[nabla].sub.[mu]] [sup.*] [F.sup.[mu]v]) = 0, (24)

where [sup.*][F.sup.[mu]v] = (1/2)[[eta].sup.[mu]v[alpha][beta]]; [F.sub.[alpha][beta]]; [[eta].sup.0123] = -1/[square root of (-g)], and the Einstein equations [G.sub.[mu]v] = -[kappa][T.sub.[mu]v], with the electromagnetic source given by the stress-energy of a nonlinear electromagnetic field (22).

4.2. Generic Features of the Lagrange Dynamics. The key point is that regularity requires F [right arrow] -0 as r [right arrow] 0, while the Maxwell limit implies F [right arrow] -0 at infinity. Indeed, in the spherically symmetric case F = -2[q.sup.2] /[L.sup.2.sub.F] [r.sup.4] , which results in F [L.sup.2.sub.F] [right arrow] -[infinity] as r [right arrow] 0. The structure of stress-energy tensor implies [p.sub.[perpendicular to]] + [rho] = F[L.sub.F], regular solutions have obligatory de Sitter center, where [p.sub.[perpendicular to]] + [rho] = 0, and hence F[L.sub.F] = 0 . Requirement of regularity demands that [L.sub.F] [right arrow] [infinity] and F [right arrow] -0 when r [right arrow] 0. Nonmonotonic behavior of the invariant F leads inevitably to branching of a Lagrangian L(F) [33, 37].

This problem is solved by the correct description of the Lagrange dynamics for regular electrically charged structures by the nonuniform variational problem with proper internal boundary conditions on the surface where the invariant F has the minimum . The nonuniform variational problem is described by the action

[mathematical expression not reproducible]. (25)

Each part of the manifold, [[OMEGA].sub.int] and [[OMEGA].sub.ext], is confined by the space-like hypersurfaces t = [t.sub.in] and t = [t.sub.fin] and by the time-like 3-surface at infinity, where electromagnetic fields vanish in the Maxwell limit. Internal boundary between [[OMEGA].sub.int] and [[OMEGA].sub.ext] is defined as a time-like hypersurface [[summation].sub.c] at which the field invariant F achieves its extremum.

In the case of the minimal coupling variation in the action (25) results in the dynamical equations (24) in both [[OMEGA].sub.int] and [[OMEGA].sub.ext], and in the boundary conditions on the surface [[summation].sub.c] 

[mathematical expression not reproducible]. (26)

The particular solution (21) can be obtained with the NED-GR Lagrangians.

[L.sub.int](F) = 2(1 - [z.sub.2]([beta]))/[([z.sub.2]([beta])+1).sup.3] with [mathematical expression not reproducible] with [z.sub.1] = (2[square root of (1 - 6[beta])]/3[beta])cos([alpha]/3) - 1 + 1/3[beta], where the invariant F is normalized on [q.sup.2]/[r.sup.4.sub.q], [r.sub.q] = ([pi]/8)([q.sup.2]/m); [beta] = [square root of (-F/2)], [beta] [member of] (0,4/27), and [alpha] = arccos((2 - 18[beta] + 27[[beta].sup.2])/2[(1 - 6[beta]).sup.3/2]) .

The same behavior of the invariant F is generic for regular axisymmetric solutions, F = -0 on the disk r = 0  and in the Maxwell limit at r [right arrow] [infinity]. As a result, the basic generic feature of the regular electrically charged structures is the existence of a characteristic surface separating regions described by different Lagrangians of the nonuniform variational problem.

4.3. Dynamics of Electromagnetic Fields. Nonzero field components compatible with the axial symmetry are [F.sub.01], [F.sub.02], [F.sub.13], [F.sub.23]. In geometry with the metric (4) they are related by

[F.sub.31] = a [sin.sup.2] [theta][F.sub.10]; [F.sub.23] = ([r.sup.2] + [a.sup.2]) [F.sub.02]. (27)

Due to (27), (24) form the system of four equations for two independent functions 

[mathematical expression not reproducible]. (28)

Solutions to this system should satisfy the compatibility condition 

[mathematical expression not reproducible] (29)

as the necessary and sufficient condition of compatibility of (28) and hence the necessary condition for the existence of solutions .

The field invariant F = [F.sub.[mu]v] [F.sup.[mu]v] in the axially symmetric case reduces to

F = 2([F.sup.2.sub.20]/[a.sup.2][sin.sup.2][theta] - [F.sup.2.sub.10]). (30)

Equations (28) and compatibility condition (29) are satisfied by the functions 

[[summation].sup.2] ([L.sub.F] [F.sub.01]) = -q ([r.sup.2] - [a.sup.2] [cos.sup.2] [theta]); [[summation].sup.2] ([L.sub.F] [F.sub.02]) = q[a.sup.2]r sin 2[theta]; (31)

[[summation].sup.2] ([L.sub.F] [F.sub.31]) = aq[sin.sup.2][theta] ([r.sup.2] - [a.sup.2] [cos.sup.2] [theta]); [[summation].sup.2] ([L.sub.F] [F.sub.23]) = aqr ([r.sup.2] + [a.sup.2]) sin 2[theta], (32)

in two limiting cases: in the linear regime [L.sub.F] = 1, when they coincide with the solutions to the Maxwell-Einstein equations [39,40], and in the strongly nonlinear regime, when (31)-(32) satisfy system (28) as the asymptotic solutions in the limit [L.sub.F] [right arrow] [infinity] .

In terms of the 3-vectors defined as [25, 41]

[E.sub.j] = {[F.sub.j0]}; [D.sup.j] = {[L.sub.F] [F.sup.0j]}; [B.sup.j] = {* [F.sup.j0]}; [H.sub.j] = {[L.sub.F] * [F.sub.0j]}; j = 1,2,3 (33)

the field equations (24) take the form of the source-free Maxwell equations 

[nabla] x D = 0; [nabla] x H = [partial derivative]D/[partial derivative]t; [nabla] x B = 0; [nabla] x E = - [partial derivative]B/[partial derivative]t. (34)

The electric induction D and the magnetic induction B are related to the electric and magnetic field intensities by

[D.sup.j] = [[epsilon].sup.j.sub.k] [E.sup.k]; [B.sup.j] = [[mu].sup.j.sub.k] [H.sup.k], (35)

where [[epsilon].sup.j.sub.k] and [[mu].sup.k.sub.j] are the tensors of the electric and magnetic permeability given by 

[mathematical expression not reproducible]. (36)

The relation connecting density and pressure with the electromagnetic fields reads 

[mathematical expression not reproducible]. (37)

Applying (31)-(32) in the limit [L.sub.F] [right arrow] [infinity], we obtain

[kappa] ([p.sub.[perpendicular to]] + [rho]) = 2[q.sup.2]/[L.sub.F] [[summation].sup.2]. (38)

It follows that [L.sub.F] [right arrow] [infinity] at the S-surface, where [p.sub.[perpendicular to]] + [rho] = 0. As a result, the magnetic permeability vanishes and electric permeability goes to infinity, so that the S-surface displays the properties of a perfect conductor and ideal diamagnetic. The magnetic induction B also vanishes on the S-surface in accordance with (35), (33) and (31)-(32).

Violation of the weak energy condition within the internal cavities of the S-surface leads to [L.sub.F] <0 in (37) and to negative values of the electric and magnetic permeability in (36). This can be avoided for the electrically charged regular structures satisfying the basic requirement of electrodynamics of continued media which is positivity of the electric permeability . The compatibility conditions (29) admit solutions (31)-(32) for electromagnetic fields in two limiting regimes, which allows for extension of the equation state ([p.sub.[perpendicular to]] + [rho]) to interior cavities of S-surface in two possible cases. The first case is similar to the shell-like models ( and references therein) with the flat vacuum interior, zero fields, and in consequence zero density and pressures. For the NED-GR regular structures in this case the field invariant F which vanishes on the S-surface by virtue of (31)-(32) vanishes also in its interiors, and magnetic permeability is zero at and within the S-surface, but the electric permeability breaks from infinity on S-surface to zero in its interior.

The second case, favored by the underlying idea of nonlinearity regularizing singularity, compatible with the existence of solutions for electromagnetic fields, and suggested by vanishing of magnetic induction on the surrounding S-surface, is the extension of [L.sub.F] [right arrow] [infinity] to the whole interior of the S-surface [26, 27] leading to regular models with the de Sitter core, p = -[rho], similar to baglike models ( and references therein). The condition [p.sub.[perpendicular to]] + [rho] = 0 and field equations are satisfied in the limit [L.sub.F] [right arrow] [infinity], so that the de Sitter vacuum core has the properties of a perfect conductor and ideal diamagnetic and zero magnetic induction.

4.4. Nondissipative Source of Electromagnetic Fields. On the de Sitter disk r = 0 where [L.sub.F] [right arrow] [infinity], we obtain from (36) [[mu].sup.r.sub.r] = [[mu].sup.[theta].sub.[theta]] = [L.sub.F.sup.-1] = [mu] right arrow] [infinity]. The magnetic induction B in (35) also vanishes with taking into account (33) and (31) [25, 26]. This suggests that an uncertainty can appear in the expression for a surface current [j.sub.s] = ((1 - [mu])/4[pi][mu])[nB], where n is the normal to the surface, which could testify for transition to a superconducting state . However, both these quantities, B and [mu], depend on [L.sub.F], and to decide whether some uncertainty appears, we have to calculate the exact value of a current in the region of the maximal density.

The surface current on the disk is defined by [mathematical expression not reproducible] , where [e.sup.[alpha].sub.(k)] are the base vectors related to the intrinsic coordinates on the disk t, [phi], 0 [less than or equal to] [xi] [less than or equal to] [pi]/2; the vector [n.sub.[alpha]] = [[delta].sup.1.sub.[alpha]] [(1 + [q.sup.2]/[a.sup.2]).sup.- 1/2] cos [xi] is the unit normal to the disk, and the symbol [x]denotes a jump across its surface in the direction orthogonal to it. Using on the disk the solutions (31)-(32) and taking into account the fact that [mu] = 1/[L.sub.F] there, we obtain the exact expression for the surface current 

[mathematical expression not reproducible]. (39)

Here a is the radius of the disk; intrinsic coordinate on the disk [xi] changes within 0 [less than or equal to] [xi] [less than or equal to] [pi]/2. Themagneticpermeability [mu] = 0 on the disk. Therefore, the current is zero throughout the disk except the ring [xi] = [pi]/2, where both terms in the second fraction go to zero independently. As a result, the surface currents on the ring can be any and amount to a nonzero total value; hence, the general condition for transition to a superconducting state  is satisfied.

The superconducting current (39) replaces the ring singularity of the Kerr-Newman geometry and represents a nondissipative source of the exterior fields , which can in principle provide a practically unlimited life time of an object .

4.5. Electromagnetic Soliton. The Kerr-Newman geometry inspired a flow of models of the electron since Carter found in 1968 that the parameter a couples with the mass M to give the angular momentum J = Ma and independently couples with the charge q to give an asymptotic magnetic dipole moment [mu] = qa, so that the gyromagnetic ratio q/M is exactly the same as predicted for a spinning particle by the Dirac equation . At the same time Carter discovered the main disaster of the Kerr-Newman geometrywhich is the total causality violation in the case of a charged particle when there are no Killing horizons, and any point can be connected to any other point by both a future and a past directed time-like curve . Existing models involving screening or covering of causally dangerous regions require introduction of cohesive forces of nonelectromagnetic origin and are typically constructed by matching the exterior Kerr-Newman solution with some hypothetic internal sources ([47, 48] and references therein).

Electromagnetic soliton of NED-GR describes in general setting a regular spinning object related by electromagnetic and gravitational radiation and can be applied as the model for the extended electron without additional assumption. According to Carter , for the electron q = -e and a = [[lambda].sub.e]/2, where [[lambda].sub.e] = [??]/[m.sub.e] is its Compton wavelength . In the observer region r [much greater than] [[lambda].sub.e], the fields are described by the Kerr-Newman limit of solutions (31)-(32) which gives 

[mathematical expression not reproducible]. (40)

The Planck constant appears due to ability of the Kerr-Newman solution, discovered by Carter, to present the electron as seen by a distant observer. In terms of the Coleman lump, (40) describes the following situation: the leading term in Er gives the Coulomb law as the classical limit [??] = 0, and the higher terms represent the quantum corrections.

5. Summary and Discussion

All regular rotating objects described by the axially symmetric solutions obtained from spherical solutions with using the Newman-Janis translation are asymptotically described by the Kerr or Kerr-Newman metrics and contain de Sitter vacuum in their deepest interior (the disk r = 0).

Regular rotating back holes can have at most two horizons. Geometry of the rotating black holes and solitons includes ergoregions where processes of extraction of rotational energy can occur which can explain energetic activity of a wide class of cosmic objects. For black holes, ergospheres and ergoregions exist for any density profile. In the case of a soliton, the existence of ergospheres depends on the density profile. Solitons can have two ergospheres and ergoregion between them, one ergosphere and ergoregion involving the whole interior, or no ergospheres.

Regular rotating black holes and solitons have two types of interior. The fist type of interior reduces to the de Sitter vacuum disk r = 0. The weak energy condition is satisfied for regular objects with the interiors of the first type. The second type of interiors exists if the related spherical solution satisfies the dominant energy condition. This type of interior is presented by de Sitter vacuum S-surface specified by p = -[rho], which contains de Sitter disk as the bridge. In the internal cavities of the S-surface the weak energy condition is violated.

The basic generic property of regular neutral objects described by the de Sitter-Kerr solutions is the existence of a phantom energy in the second type interiors .

Phantom energy, which inevitably has negative density for a certain class of observers, was introduced  in order to model the observed acceleration of our universe. In the most of models phantom energy originates from scalar field(s) with negative kinetic energy  and may involve extra dimensions (for a review ). For regular rotating black holes and solitons with second type interiors phantom equation of state appears without involvement of additional entities in the internal regions of strong gravitational field.

Regular rotating electrically charged black holes and spinning solitons are described by nonlinear electrodynamics coupled to gravity. For a distant observer, electromagnetic and gravitational fields asymptotically coincide with the Kerr-Newman fields. The nondissipative source of electromagnetic fields (which in turn form a source of gravitational fields) is a superconducting current (replacing a ring singularity) predicted in the model-independent way by dynamical equations governing regular objects related by electromagnetic and gravitational interactions.

All regular electrically charged rotating objects contain de Sitter vacuum disk r = 0 which have the properties of the ideal conductor and ideal diamagnetic. For the objects with the second type of interiors, these properties are characteristic for the whole S-surface. The violation of the weak energy condition in its internal cavities leads to negative values of the electric and magnetic permeability. For objects satisfying the basic requirement of electrodynamics of continued media (positivity of electric permeability), this can be avoided by extension of the equation of state p = -[rho] to the whole interior, confined by the S-surface, in agreement with the conditions for the existence and admissible behavior of solutions for electromagnetic fields.

Mass of regular objects with the de Sitter interior is related to breaking of space-time symmetry from the de Sitter group [18,25,33,51]. De Sitter vacuum appears in the particle theory as a false vacuum state p = -[rho] of the Higgs field responsible for a particle mass. This relation allows us to explain the observable effect of the negative mass-square differences for neutrinos by applying de Sitter group for space-time symmetry in the interaction vertex and calculating particles masses as the eigenvalues of the Casimir operator in de Sitter space .

Experimental data reveal with a 5[sigma] significance the existence of a minimal length scale [l.sub.e] = 1.57 x [10.sup.-17] cm at the energy E = 1.253 TeV in the annihilation reaction [e.sup.+] [e.sup.-] [right arrow] [gamma][gamma]([gamma]) . It corresponds to the minimum in the [chi square]-fit and characterizes the region of the closest approach of annihilating particles specified by the finite length [l.sub.e] which cannot be made smaller. Hypotheses of quantum electrodynamics applied in the [chi square]-test assume a scattering center as a point. If the electron is an extended object, its structure would modify the QED cross-section if the test distances are smaller than its characteristic size. The results indicate decreasing cross-section with respect to that predicted by QED and testify for extended particles rather than point-like. The reaction [e.sup.+] [e.sup.-] [right arrow] [gamma][gamma]([gamma]) is purely electromagnetic and can be considered as the process of interaction of extended particles related by electromagnetic and gravitational interactions. The definite feature of the annihilation process is that at its final stage a region of interaction is neutral and spineless. It can be roughly modeled by a spherical lump with de Sitter vacuum interior [16,18]. For all structures with the de Sitter interior, there exists the characteristic zero gravity surface [r.sub.s] [equivalent] [([r.sup.2.sub.0] [r.sub.g]).sup.1/3] at which the strong energy condition ([rho] + [summation] [p.sub.k] [greater than or equal to] 0 ) is violated and beyond which the gravitational acceleration becomes repulsive . The gravitational radius [r.sub.g] related to the energy E = 1.253 TeV and de Sitter radius [r.sub.0] related to the Higgs vacuum expectation value responsible for the electron mass at the scale [E.sub.EW] = 246 GeV give [r.sub.*] [equivalent] 0.86 x [10.sup.-16] cm. The scale [l.sub.e] = 1.57 x [10.sup.-17] cm fits inside a region where gravity is repulsive and can be thus understood as a distance at which electromagnetic attraction is balanced by the gravitational repulsion of the interior de Sitter vacuum .

https://doi.org/10.1155/2017/1035381

Conflicts of Interest

The authors declare that there are no conflicts of interest regarding the publication of this paper.

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Irina Dymnikova (1,2) and Evgeny Galaktionov (1)

(1) A. F. Ioffe Physico-Technical Institute, Politekhnicheskaja 26, St. Petersburg 194021, Russia

(2) Department of Mathematics and Computer Science, University of Warmia and Mazury, Sloneczna 54,10-710 Olsztyn, Poland

Correspondence should be addressed to Irina Dymnikova; irina@uwm.edu.pl

Received 30 April 2017; Revised 14 June 2017; Accepted 29 August 2017; Published 16 October 2017

Caption: Figure 1: Typical behavior of spherical metric function g(r). Here m is the mass parameter M normalized to its certain critical value which specifies the double-horizon state.

Caption: Figure 2: Four cases for the existence of ergospheres and ergoregions.

Caption: Figure 3: First type of the de Sitter interior for regular rotating objects.

Caption: Figure 4: Second type of interior for regular rotating black holes and solitons.
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