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Volume 2 - LENR-CANR

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Here / 2 M is the reduced mass of monopole. From last two equations it follows that<br />

g g<br />

the motion of monopole (antimonopole) inside the pair is nonrelativistic:<br />

nonrel rel<br />

2<br />

T , T M c .<br />

max max<br />

g<br />

From formulas (7-9) it also follows that the ratio of kinetic and potential energies in each pair<br />

is very small both in nonrelativistic and relativistic cases<br />

T V r c g , (10)<br />

nonrelat<br />

max / | 0( min)<br />

| ( /<br />

2 2<br />

) / 2 1<br />

relat<br />

max / | 0( min ) | ( /<br />

2<br />

) / 2 1<br />

T V r c g<br />

(11)<br />

This result proves that monopole-antimonopole pair is very stable neutral system.<br />

The total mass of such system in stable bound state<br />

g g<br />

M ( r ) ( p / c ) 4 M ( / 4 r c ) 4M<br />

<br />

2 2<br />

min<br />

2<br />

max<br />

2 2<br />

g 2<br />

rminc 2<br />

<br />

2<br />

min<br />

2 2<br />

g 2<br />

rminc c<br />

M<br />

M g <br />

2 g<br />

<br />

(137)<br />

is very small.<br />

2<br />

g<br />

2 2<br />

In fact such pair is an invisible electro- and magneto- uncharged and extremely light object.<br />

It is possible that such objects have existed (unnoticed) in the universe from the moment of the<br />

Big Bang.<br />

2. Break of monopole-antimonopol pair in a strong magnetic field<br />

In Fig. 4 the structure of the potential hole of monopole-antimonopole bounded pair in the<br />

cases of presence and absence of external locally homogeneous magnetic field H0 is presented.<br />

Under the external magnetic field action the essential deformation of potential hole takes<br />

place. It leads to the possibility of tunneling of one monopole and to the spontaneous brake of<br />

the monopole-antimonopole pair. The probability PH and the life-time H of such tunneling<br />

effect is similar to the probability of nuclear alpha-decay<br />

P 1/ ( v / r ) e ; v p / M ;<br />

2W<br />

H H max min max max g<br />

r2<br />

1<br />

W 2 g<br />

| V0( r) VH ( r) Emin | dr, Emin V0( r1 ) VH<br />

( r1<br />

),<br />

<br />

r1<br />

V g / r, V gH<br />

r,<br />

2<br />

o H<br />

0<br />

r1 and r2 are the classical turning points for the potential energy V(r) = V0(r) + VH(r)<br />

488<br />

(12)<br />

(13)

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