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Exact Solutions and Scalar Fields in Gravity - Instituto Avanzado de ...

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80 EXACT SOLUTIONS AND SCALAR FIELDS IN GRAVITY<br />

where Simple calculation gives<br />

the conservation law<br />

Hence, there exists function such that<br />

Thus we are led to an iteration procedure. Given the nth currents<br />

<strong>and</strong> satisfy<strong>in</strong>g the equation for one <strong>de</strong>f<strong>in</strong>es<br />

the function such that <strong>and</strong> Then<br />

the currents are <strong>de</strong>f<strong>in</strong>ed by<br />

<strong>and</strong> we get the follow<strong>in</strong>g conservation law<br />

Thus one arrives at an <strong>in</strong>f<strong>in</strong>ite number of nonlocal conservation laws for<br />

The term nonlocal st<strong>and</strong>s for the fact that the currents<br />

<strong>and</strong> are <strong>de</strong>f<strong>in</strong>ed by <strong>in</strong>tegration <strong>and</strong> differentiation of lower<br />

currents. For the nth charge we get<br />

So the (n+l)th currents read<br />

[The natural question arises what the relations are between the above<br />

conservations laws <strong>and</strong> the ones obta<strong>in</strong>ed by C.P.Boyer <strong>and</strong><br />

[22, 23] for heavenly equation <strong>in</strong> 4 dimensions.]<br />

3. LINEAR SYSTEMS FOR ME<br />

Here we show how one can adopt some results obta<strong>in</strong>ed for SDYM<br />

equations (L.L.Chau et al [20], L.L.Chau [21]) to get the l<strong>in</strong>ear systems<br />

connected with ME. Def<strong>in</strong>e

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