# Elementary Superconductivity in Nonlinear Electrodynamics Coupled to Gravity

Authors: Irina Dymnikova
Journal: Journal of Gravity
 (2015)

---

## Abstract

Source-free equations of nonlinear electrodynamics minimally coupled to gravity admit regular axially symmetric asymptotically Kerr-Newman solutions which describe charged rotating black holes and electromagnetic spinning solitons (lumps). Asymptotic analysis of solutions shows, for both black holes and solitons, the existence of de Sitter vacuum interior which has the properties of a perfect conductor and ideal diamagnetic and displays superconducting behaviour which can be responsible for practically unlimited lifetime of the electron. Superconducting current flows on the equatorial ring replacing the Kerr ring singularity of the Kerr-Newman geometry. Interior de Sitter vacuum supplies the electron with the finite positive electromagnetic mass related to the interior de Sitter vacuum of the electroweak scale and to breaking of space-time symmetry, which allows explaining the mass-square
differences for neutrino and the appearance of the minimal length scale in the annihilation reactione+e-→γγ(γ).


---

## Body

## 1. Introduction

Quantum electrodynamics applies the point-like idealization for leptons, which well describes in- and out-states of particles at the distances sufficiently large as compared with their eventual sizes. In experiments on high energy scattering, leptons are found structureless down to ~10−16 cm. There exist however experiments, in which particles approach each other so close that their annihilation results in their complete destruction. Study of the electromagnetic reaction e+e-→γγ(γ), with using the data from VENUS, TOPAZ, ALEPH, DELPHI, L3, and OPAL, reveals with the 5σ significance the existence of the minimal length le=1.57×10-17 cm at the scale E=1.253 TeV [1]. The annihilation reaction can be a source of information about possible internal structure of leptons, which requires an extended model for the electron.In 1962 Dirac proposed to assume the electron to have a finite size, with no a priori constraints fixing its size and shape [2]. In his model the electron is visualized as a spherical shell which serves as a source of electromagnetic field and is supplied with a cohesive force (Poincaré stress) of a nonelectromagnetic origin, needed to prevent the electron from flying apart under the Coulomb repulsion [2].The Kerr-Newman solution to the source-free Maxwell-Einstein equations found in 1965 [3]:(1)ds2=2mr-e2-ΣΣdt2+ΣΔdr2+Σdθ2-2a2mr-e2sin2⁡θΣdtdϕ+r2+a2+2mr-e2a2sin2⁡θΣsin2⁡θdϕ2;Δ=r2-2mr+a2+e2,where Σ-function and the associated electromagnetic potential read(2)Σ=r2+a2cos2⁡θ;Ai=-erΣ1;0,0,-asin2⁡θ,inspired the further search since Carter discovered in 1968 that the parameter a couples with the mass m to give the angular momentum J=ma and independently couples with the charge e to give an asymptotic magnetic dipole moment μ=ea, so that the gyromagnetic ratio e/m is exactly the same as predicted for a spinning particle by the Dirac equation [4].At the same time Carter discovered the big trouble of the Kerr-Newman geometry just in the case appropriate for the electron,a2+e2>m2; when there are no Killing horizons, the manifold is geodesically complete (except for geodesics which reach the singularity), and any point can be connected to any other point by both a future and a past directed time-like curve. Closed time-like curves originate in the region where gϕϕ<0, can extend over the whole manifold and cannot be removed by taking a covering space [4].The source models for the Kerr-Newman exterior fields, involving a screening or covering of causally dangerous region and Poincaré stress of different origins, can be roughly divided into disk-like [5–8], shell-like [9–12], bag-like [13–19], and string-like ([20] and references therein). The problem of matching the Kerr-Newman exterior to a rotating material source does not have a unique solution, since one is free to choose arbitrarily the boundary between the exterior and the interior [5] as well as an interior model.The Dirac proposal to approach the electron without a priori constraints on its size and shape can be applied in the context of the Coleman lump (physical soliton) as a nonsingular, nondissipative solution of finite energy holding itself together by its own self-interaction [21]. An appropriate instrument to shed some light on the purely electromagnetic reaction of e+e- annihilation is nonlinear electrodynamics coupled to gravity (NED-GR) (NED theories appear as low-energy effective limits in certain models of string/M-theories [22–24].).Nonlinear electrodynamics was proposed by Born and Infeld as founded on two basic points: to consider electromagnetic field and particles within the frame of one physical entity which is electromagnetic field; to avoid letting physical quantities become infinite [25]. In their theory a total energy is finite and particles are considered as singularities of the field, but it is also possible to obtain the finite electron radius by introducing an upper limit on the electric field [25].The Born-Infeld program can be realized in nonlinear electrodynamics minimally coupled to gravity. Source-free NED-GR equations admit regular causally safe axially symmetric asymptotically Kerr-Newman solutions which describe regular rotating charged black holes and electromagnetic spinning solitons (lumps) [26, 27].For any gauge-invariant LagrangianL(F), stress-energy tensor of electromagnetic field(3)κTνμ=-2LFFναFμα+12δνμL;κ=8πG,where Fμν=∂μAν-∂νAμ (Greek indices run from 0 to 3) and LF=dL/dF, in the spherically symmetric case, has the algebraic structure(4)T00=T11pr=-ρ,since the only essential components of Fμν are a radial electric field F01 and a radial magnetic field F23. Regular spherically symmetric solutions with stress-energy tensors specified by (4) satisfying the weak energy condition (nonnegativity of density as measured by any local observe) have obligatory de Sitter center with p=-ρ [28–31]. In NED-GR regular spherical solutions the weak energy condition is always satisfied and de Sitter vacuum provides a proper cut-off on self-interaction divergent for a point charge [26, 32]. They can be transformed into regular axially symmetric solutions by the Gürses-Gürsey algorithm [33, 34].Here we outline the generic properties of regular rotating charged black holes and solitons.


## 2. Basic Equations

Nonlinear electrodynamics minimally coupled to gravity is described by the action(5)S=116πG∫d4x-gR-LF;F=FμνFμν,where R is the scalar curvature. The Lagrangian L(F) is an arbitrary function of F which should have the Maxwell limit, L→F, LF→1 in the weak field regime.Variation with respect toAμ and gμν yields the dynamic field equations(6)∇μLFFμν=0;∇μ∗Fμν=0;F∗μν=12ημναβFαβ;η0123=-1-gand the Einstein equation Gμν=-κTμν with Tμν given by (3).NED-GR equations do not admit regular spherically symmetric solutions with the Maxwell center [35], but they admit regular solutions with the de Sitter center [32]. The question of correct description of NED-GR regular electrically charged structures by the Lagrange dynamics is clarified in [36]. Regular solutions satisfying (4) are described by the metric(7)ds2=grdt2-dr2gr-r2dΩ2;gr=1-2Mrr;Mr=4π∫0rρ~xx2dx,with the electromagnetic density ρ~(r)=Ttt(r) from (3). This metric is asymptotically de Sitter as r→0, and asymptotically Reissner-Nordström as r→∞ [32].The regular spherical solutions generated by (4) belong to the Kerr-Schild class [18, 37, 38] and can be transformed by the Gürses-Gürsey algorithm [33] into regular axially symmetric solutions which describe regular rotating electrically charged objects, asymptotically Kerr-Newman for a distant observer [26, 34].In the Boyer-Lindquist coordinates the rotating metric reads (in the unitsG=c=1) [33](8)ds2=2fr-ΣΣdt2+ΣΔdr2+Σdθ2-4afrsin2⁡θΣdtdϕ+r2+a2+2fra2sin2θΣsin2⁡θdϕ2,where Δ=r2+a2-2f(r). A function f(r)=rM(r) comes from a spherically symmetric solution [33]. For the Kerr-Newman geometry 2f(r)=2mr-e2 is responsible for causality violation related to regions where gϕϕ<0 in (1). For NED-GR regular solutions satisfying the weak energy condition, M(r) is nonnegative function monotonically growing from 4πρ~(0)r3/3 as r→0 to m-e2/2r as r→∞ [32]. This guarantees the causal safety on the whole manifold due to f(r)≥0 and gϕϕ>0 in (8).The coordinater is defined as an affine parameter along either of two principal null congruences, and the surfaces of constant r are the oblate confocal ellipsoids of revolution(9)r4-r2x2+y2+z2-a2-a2z2=0,which degenerate, for r=0, to the equatorial disk(10)x2+y2≤a2,z=0,centered on the symmetry axis and bounded by the ring x2+y2=a2 (r=0, θ=π/2) [39].


## 3. Geometry

The Cartesian coordinatesx, y, and z are related to the Boyer-Lindquist coordinates r, θ, and ϕ by(11)x2+y2=r2+a2sin2⁡θ;z=rcos⁡θ.The anisotropic stress-energy tensor responsible for (8) can be written in the form [33](12)Tμν=ρ+p⊥uμuν-lμlν+p⊥gμνin the orthonormal tetrad(13)uμ=1±ΔΣr2+a2δ0μ+aδ3μ,lμ=±ΔΣδ1μ,nμ=1Σδ2μ,mμ=-1Σsin⁡θasin2⁡θδ0μ+δ3μ.The sign plus refers to the regions outside the event horizon and inside the Cauchy horizon where vector uμ is time-like, and the sign minus refers to the regions between the horizons where vector lμ is time-like. Vectors mμ and nμ are space-like in all regions.The eigenvalues of the stress-energy tensor (3) in the corotating frame where each of ellipsoidal layers rotates with the angular velocity ω(r)=uϕ/ut=a/(r2+a2) [18] are defined by(14)Tμνuμuν=ρr,θ;Tμνlμlν=pr=-ρ;Tμνnμnν=Tμνmμmν=p⊥r,θ,in the regions outside the event horizon and inside the Cauchy horizon where density is defined as the eigenvalue of the time-like eigenvector uμ. They are related to function f(r) [18] as κΣ2ρ=2f′r-f; κΣ2p⊥=2f′r-f-f′′Σ [18]. This gives(15)κρr,θ=r4Σ2ρ~r;κp⊥+ρ=2r4Σ2-r2Σρ~r-r32Σρ~′r=2r2Σ2Σr4ρ~′-ρ~a2cos2⁡θ,where ρ~(r) is a relevant spherically symmetric density profile. The prime denotes the derivative with respect to r.


### 3.1. Horizons, Ergospheres, and Ergoregions

Horizons are defined by zeros of functionΔ(r) given by(16)Δr=r2+a2-2fr=a2+r2gr.Δ=a2 at zero points of the metric function g(rh)=0 and changes from Δ=a2 as r=0 to Δ→∞ as r→∞.Ergosphere is a surface of a static limitgtt=0 given by(17)gttr,θ=r2+a2cos2⁡θ-2fr=0.It follows that z2=(2r2f(r)-r4)/a2. Each point of the ergosphere belongs to some of confocal ellipsoids (9) covering the whole space as the coordinate surfaces r = const. At the z-axis (16) and (17) are identical, so that the minor axis of ergosphere is equal to r+.For black holes ergoregions (the regions wheregtt<0) exist for any density profile. Black holes have at most two horizons. Ergoregions exist between the event horizon and ergosphere. Solitons are objects without horizons; they can have two, one, or no ergospheres, this depends on the particular form of a density profile ρ~(r) and on the values of parameters [27].


### 3.2. De Sitter Vacuum Interiors

Rotation transforms the de Sitter center to the de Sitter equatorial disk (10) which exists in each regular axially symmetric geometry. In the limit r→0, on disk (10), r2/Σ→1 [26]. For the spherical solutions regularity requires ρ~(r)<∞, rρ~′(r)→0, and 2f(r)→κρ~(0)r4/3 as r→0 [32], so that disk r=0 is intrinsically flat [26]. Equation (15) gives in this limit the equation of state on the disk(18)p⊥+ρ=0⟶p⊥=pr=-ρ,which represents the rotating de Sitter vacuum [26].Equation (15) implies a possibility of generic violation of the weak energy condition (WEC) which was reported for several particular models of regular rotating objects [18, 40–42]. WEC can be violated beyond the vacuum surface E(r,z)=0 on which p⊥+ρ=0 and the right-hand side in (15) can change its sign [27]. It can be expressed through the pressure of a related spherical solution, p⊥~=-ρ~-rρ~′/2 [32], which gives [27](19)κp⊥+ρ=rρ~′2Σ2Er,z=0;Er,z=r4-z2Pr;Pr=2a2rρ~′ρ~-p⊥~.The existence of vacuum surfaces is directly stipulated by fulfillment of the dominant energy condition (ρ~≥pk~) for related spherical solutions. Each vacuum E-surface contains the de Sitter disk as a bridge and is entirely confined within the r∗-ellipsoid whose minor axis coincides with |z|max for the E-surface [27]. The squared width of the E-surface WE2=(x2+y2)E=(a2+|z|P(r))(1-|z|/P(r)). For regular solutions rρ~′→0, p⊥→-ρ as r→0 [32], and P(r)→A2r-(n+1) with the integer n≥0 as r→0. Function WE(z) has the cusp at approaching the disk and at least two symmetric maxima between z=±r∗ and z=0 [27].In Figure1 [27] E-surface is plotted for the electromagnetic soliton with the regularized Coulomb profile [32]:(20)ρ~=q2r2+rq22;rq=πq28m.Its width in the equatorial plane WE=a and the height HE=|z|max=arq. For the electron WE=λe/2, where λe≃3.9×10-11 cm, HE≃0.038λe and η=WE/HE=a/rq≃13.2.Figure 1
Electromagnetice-lump from nonlinear electrodynamics coupled to gravity [27].


## 3.1. Horizons, Ergospheres, and Ergoregions

Horizons are defined by zeros of functionΔ(r) given by(16)Δr=r2+a2-2fr=a2+r2gr.Δ=a2 at zero points of the metric function g(rh)=0 and changes from Δ=a2 as r=0 to Δ→∞ as r→∞.Ergosphere is a surface of a static limitgtt=0 given by(17)gttr,θ=r2+a2cos2⁡θ-2fr=0.It follows that z2=(2r2f(r)-r4)/a2. Each point of the ergosphere belongs to some of confocal ellipsoids (9) covering the whole space as the coordinate surfaces r = const. At the z-axis (16) and (17) are identical, so that the minor axis of ergosphere is equal to r+.For black holes ergoregions (the regions wheregtt<0) exist for any density profile. Black holes have at most two horizons. Ergoregions exist between the event horizon and ergosphere. Solitons are objects without horizons; they can have two, one, or no ergospheres, this depends on the particular form of a density profile ρ~(r) and on the values of parameters [27].


## 3.2. De Sitter Vacuum Interiors

Rotation transforms the de Sitter center to the de Sitter equatorial disk (10) which exists in each regular axially symmetric geometry. In the limit r→0, on disk (10), r2/Σ→1 [26]. For the spherical solutions regularity requires ρ~(r)<∞, rρ~′(r)→0, and 2f(r)→κρ~(0)r4/3 as r→0 [32], so that disk r=0 is intrinsically flat [26]. Equation (15) gives in this limit the equation of state on the disk(18)p⊥+ρ=0⟶p⊥=pr=-ρ,which represents the rotating de Sitter vacuum [26].Equation (15) implies a possibility of generic violation of the weak energy condition (WEC) which was reported for several particular models of regular rotating objects [18, 40–42]. WEC can be violated beyond the vacuum surface E(r,z)=0 on which p⊥+ρ=0 and the right-hand side in (15) can change its sign [27]. It can be expressed through the pressure of a related spherical solution, p⊥~=-ρ~-rρ~′/2 [32], which gives [27](19)κp⊥+ρ=rρ~′2Σ2Er,z=0;Er,z=r4-z2Pr;Pr=2a2rρ~′ρ~-p⊥~.The existence of vacuum surfaces is directly stipulated by fulfillment of the dominant energy condition (ρ~≥pk~) for related spherical solutions. Each vacuum E-surface contains the de Sitter disk as a bridge and is entirely confined within the r∗-ellipsoid whose minor axis coincides with |z|max for the E-surface [27]. The squared width of the E-surface WE2=(x2+y2)E=(a2+|z|P(r))(1-|z|/P(r)). For regular solutions rρ~′→0, p⊥→-ρ as r→0 [32], and P(r)→A2r-(n+1) with the integer n≥0 as r→0. Function WE(z) has the cusp at approaching the disk and at least two symmetric maxima between z=±r∗ and z=0 [27].In Figure1 [27] E-surface is plotted for the electromagnetic soliton with the regularized Coulomb profile [32]:(20)ρ~=q2r2+rq22;rq=πq28m.Its width in the equatorial plane WE=a and the height HE=|z|max=arq. For the electron WE=λe/2, where λe≃3.9×10-11 cm, HE≃0.038λe and η=WE/HE=a/rq≃13.2.Figure 1
Electromagnetice-lump from nonlinear electrodynamics coupled to gravity [27].


## 4. Electromagnetic Fields

Nonzero field components compatible with the axial symmetry areF01, F02, F13, and F23. In geometry with the metric (8) they are related by(21)F31=asin2⁡θF10;aF23=r2+a2F02.The field invariant F=FμνFμν in the axially symmetric case reduces to(22)F=2F202a2sin2⁡θ-F102.In terms of the 3 vectors, denoted by Latin indices running from 1 to 3 and defined as(23)Ej=Fj0;Dj=LFF0j;Bj=F∗j0;Hj=LFF∗0j,the field equations (6) take the form of the Maxwell equations. The electric induction D and the magnetic induction B are related with the electric and magnetic field intensities by [26](24)Dj=ϵkjEk;Bj=μkjHk,where ϵjk and μjk are the tensors of the electric and magnetic permeability given by [26](25)ϵrr=r2+a2ΔLF;ϵθθ=LF;μrr=r2+a2ΔLF;μθθ=1LF.The dynamical equations (6) are satisfied by the functions [26](26)F10=qΣ2LFr2-a2cos2⁡θ;F02=qΣ2LFa2rsin⁡2θ;F31=asin2⁡θF10;aF23=r2+a2F02in the weak field limit LF=1, where they coincide with the Kerr-Newman fields [4, 16], and an integration constant q is identified as the electric charge. For the electron q=-e, ma=ħ/2 [4], a=λe/2, where λe=ħ/(mec) is the Compton wavelength. In the observer region r≫λe,(27)Er=-er21-ħ2me2c23cos2⁡θ4r2;Eθ=eħ2me2c2sin⁡2θ4r3;Br=-eħmeccos⁡θr3=2μecos⁡θr3;Bθ=-μesin⁡θr4.The Planck constant appears here due to ability, discovered by Carter, of the Kerr-Newman solution to present the electron as seen by a distant observer. In terms of the Coleman lump (27) describes the following situation: the leading term in Er gives the Coulomb law as the classical limit ħ=0; the higher terms represent the quantum corrections.With taking into account connection between the field components (21), we have four dynamical equations (6) for two field components, F01, F02, and the nonlinearity function LF. Condition of compatibility of system of four equations for three function reduces to the constraint on the nonlinearity which has the form [27](28)∂∂r1LF∂LF∂θ∂∂θ1LF∂LF∂r+4a2sin2⁡θΣ21LF2r∂LF∂r+cot⁡θ∂LF∂θ2=0.The functions (26) present asymptotic solutions to the dynamical equations (6) in the limit LF→∞ and LFΣ2→∞. In this limit they satisfy the system (6) and the condition of their compatibility (28) [27].


## 5. Interior Dynamics and Elementary Superconductivity

The relation connecting density and pressure with the electromagnetic fields reads [26](29)κp⊥+ρ=2LFF102+F202a2sin2⁡θ.In the limit LF→∞, (6) have asymptotic solutions (26) [26, 27]. It results in [26](30)κp⊥+ρ=2q2LFΣ2.Equation of state on the disk (18) dictated by geometry for regular spinning solutions requires p⊥+ρ=0. It follows that LFΣ2→∞ and hence LF→∞, since Σ→0 on the disk.The magnetic inductionB vanishes in this limit, so that B→0 on the disk [26]. The electric permeability in (25) goes to infinity; the magnetic permeability μ=LF-1 vanishes, so that the de Sitter vacuum disk has both perfect conductor and ideal diamagnetic properties.In electrodynamics of continued media the transition to a superconducting state corresponds to the limitsB→0 and μ→0 in a surface current js=(1-μ/4πμ)[nB] where n is the normal to the surface; the right-hand side then becomes indeterminate, and there is no condition which would restrict the possible values of the current [43]. Definition of a surface current for a charged surface layer is 4πjk=[e(k)αFαβnβ] [5], where [·] denotes a jump across the layer; e(k)α are the tangential base vectors associated with the intrinsic coordinates on the disk t,ϕ, 0≤ξ≤π/2; nα=1+q2/a2-1/2cos⁡ξδα1 is the unit normal directed upwards [5]. With using asymptotic solutions (26) and magnetic permeability μ=1/LF, we obtain the surface current [44](31)jϕ=-q2πa1+q2a2sin2⁡ξμcos3⁡ξ.At approaching the ring r=0, ξ=π/2, both terms in the second fraction go to zero quite independently. As a result the surface currents on the ring can be any and amount to a nonzero total value [26, 44].The superconducting current (31) replaces the Kerr ring singularity of the Kerr-Newman geometry and can be considered as a source of the Kerr-Newman fields. This kind of a source is nondissipative, so that electrovacuum solitons present actually e-lumps in accordance with the Coleman definition of the lump as a nonsingular, nondissipative solution of finite energy holding itself together by its own self-interaction [21]. Lifetime of e-lump is unlimited.De Sitter disk exists in the interior of any regular charged black hole and soliton. When a related spherical solution satisfies the dominant energy condition, it exists as a bridge inside theE-surface, defined by p⊥+ρ=0. It follows that LF→∞ by virtue of (30). The magnetic permeability vanishes and electric permeability goes to infinity, so that E-surface displays the properties of a perfect conductor and ideal diamagnetic. Also magnetic induction vanishes on E-surface by virtue of the asymptotic solutions (26), so that the Meissner effect occurs there [26]. Within E-surface, in cavities between its upper and down boundaries and the bridge, negative value of (p⊥+ρ) in (29) would mean negative values for electric and magnetic permeabilities inadmissible in electrodynamics of continued media [43]. The case, favored by the underlying idea of nonlinearity replacing a singularity and suggested by vanishing of magnetic induction on the surrounding E-surface, is extension of LF→∞ to its interiors. Then we have de Sitter vacuum core, p=-ρ, with the properties of a perfect conductor and ideal diamagnetic and magnetic fields vanishing throughout the whole core, and the weak energy condition is satisfied for regular rotating charged black holes and solitons.


## 6. Summary and Discussion

Nonlinear electrodynamics minimally coupled to gravity admits the regular axially symmetric solutions asymptotically Kerr-Newman for a distant observer, which describe regular charged rotating black holes and electromagnetic solitons.The basic generic feature of all these objects is the interior de Sitter vacuum disk withp=-ρ in the corotating frame, which has properties of a perfect conductor and ideal diamagnetic. Superconducting current flows on the equatorial ring replacing the Kerr singularity of the Kerr-Newman geometry. This current serves as a nondissipative source of the Kerr-Newman external fields and can be responsible for practically unlimited lifetime of the electron.In the case when related spherical solution satisfies the dominant energy condition, de Sitter disk is incorporated as a bridge in the vacuumE-surface with the equation of state p=-ρ, properties of the perfect conductor and ideal diamagnetic, and vanishing magnetic induction. This allows extending these properties to the interior of the E-surface, since otherwise the violation of the weak energy condition in its interior would lead to the negative values of the electric and magnetic permeabilities, inadmissible in electrodynamics of continued media. As a result the weak energy condition is satisfied for regular rotating objects of this type.Mass parameterm in a NED-GR spinning solution is the electromagnetic mass [26, 32], related to interior de Sitter vacuum and breaking of space-time symmetry from the de Sitter group for any solution specified by (4) [30]. This has been tested by application of Casimir invariants of the de Sitter group in the region surrounding the interaction vertex for the sub-eV particles, which predicts TeV scale for gravito-electroweak unification and explains the experimental results known as a negative mass-squared difference for neutrino [45].This conforms with the Higgs mechanism for generation of mass via spontaneous breaking of symmetry of a scalar field vacuum. The Higgs field is involved in mass generation in its false vacuum state satisfyingp=-ρ. Then the space-time symmetry around the interaction vertex is the de Sitter group, while in the observer region it is Poincaré group (strictly speaking another de Sitter with much less value of the cosmic vacuum density), which requires breaking of symmetry in between to the Lorentz radial boosts only [30]. Generation of mass by the Higgs mechanism must thus involve breaking of space-time symmetry [44].Interior de Sitter vacuum can explain the appearance of the minimal length in the reactione+e-→γγ(γ). The definite feature of annihilation process is that at its certain stage a region of interaction is neutral and spinless. We can roughly model it by a spherical bag with de Sitter vacuum interior asymptotically Schwarzschild as r→∞. For such a structure there exists a zero gravity surface at which the strong energy condition (ρ+∑k≥0‍) is violated and beyond which gravity becomes repulsive [29, 46]. The related length scale rs≃(r02rg)1/3 appears in any geometry with de Sitter interior and Schwarzschild exterior [28, 47]. Adopting for de Sitter interior the vacuum expectation value v=246 GeV responsible for the electron mass [48], we get de Sitter radius r0=1.37cm. Radius rs at the energy scale E≃1.253 TeV is rs≃0.86×10-16 cm, so that the scale le=1.57×10-17 cm fits inside a region where gravity is repulsive. Regular NED-GR solutions provide a de Sitter cutoff on electromagnetic self-energy, which can be qualitatively estimated by e2/rc4≃κρ0=3/r02. It gives the length scale rc at which electromagnetic attraction is balanced by de Sitter gravitational repulsion rc≃1.05×10-17 cm, sufficiently close to the experimental value le for such a rough estimate [1]. The minimal length scale le can be thus understood as a distance of the closest approach of annihilating particles at which electromagnetic attraction is stopped by the gravitational repulsion due to interior de Sitter vacuum.



---

*Source: 904171-2015-07-05.xml*