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The problem posed here is to shorten the time measured by a traveller in his rest-frame, beyond the shortenning ensured by the Special Relativity. It seems that electromagnetic fields may be of help. The question is whether enough strong fields can be realized in practice.

The question whether a worm-hole can be created in our 4D space-time was asked frequently and it was proved that the answer is negative. It would necessitate a 5th dimension, and no such dimension is known to us. As an analogy, between two points on the surface of a simple sphere - a 2D surface - one could dig a worm-hole by passing through the body of the sphere, i.e. exploiting the fact that the sphere is imbedded in the 3D space.

The relativistic interval between two neighbor points P1 and P2 in the flat 4D space-time is given by

(1) F = (c dt)2 - Σi=1,2,3 (dxi)2

If F > 0 it can be denoted as (c dτ)2 where τ is the proper time, the time recorded by a traveller between P1 and P2, in his rest-frame of coodinates. Obviously, in this case (dτ)2 < (dt)2. However, for shortenning dτ significantly with respect to dt, the velocity V of the traveller has to be of the order of magnitude of the light velocity.

The problem posed here is whether there is a possibility to shorten dτ even more, by means of strong fields. Indeed, Einstein's Field Equations (EFE) contain in their RHS, fields. They change the metric from (1) to

(2) F' = Σi,j=0 3 gi,j dxi dxj

If F' is positive and smaller than F, one can denote F' = (c dτ')2, and F - F' = (dϕ)2, and get

(3) (c dτ')2 = (c dt)2 - Σi=1,2,3 (dxi)2 - (dϕ)2.

Thus, the effect of ϕ is analogous to a 5th dimension.

The equation (3) can be written in the more useful form

(4) (dτ')2 = { 1 - V2/c2 - [dϕ/(cdt)]2 } (dt)2.

Fields that render F' < F can be generated, but the question is whether enough big intensities can be obtained for [dϕ/(cdt)]2 to be significant.

For instance, the contribution of the gravitational field is is not significant. In the Schwarzchsild metric [dϕ/(cdt)]2 = 2GM/c2R. At the surface of the Earth this is of the order 10-11.

The electromagnetic (e.m.) field seems to offer a better value. For instance in the Reissner–Nordström metric [dϕ/(cdt)]2 is proportional with Q2/(2 c2 M) where Q is the electric charge confined to a mass M. It does not take into consideration magnetic fields.

Can somebody indicate a reference which calculates the metric in the complete e.m. field? Also, how much charge Q can be confined, say, in a box of dielectric of 1m3 volume?

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