Ernst equation

Equation used in general relativity From Wikipedia, the free encyclopedia

In general relativity, the Ernst equation[1] is an integrable non-linear partial differential equation, named after the American physicist Frederick J. Ernst [sl] who published it in 1968.[2][3]

Description

The Ernst's equation governing the complex scalar function is given by[4]

where is the two-dimensional gradient operator with axisymmetry; for instance, if , then

and if (with ), then[5]

where is the real part of . If is a solution of the Ernst's equation, then (so is ) is also a solution where is an arbitrary real constant. The transformation belongs to the so-called Ehler's transformation.

Often, one introduces

so that we have

The Ernst equation is derivable from the Lagrangian density

For its Lax pair and other features see e.g. [6][7] and references therein.

Usage

The Ernst equation is employed in order to produce exact solutions of the Einstein's equations in the general theory of relativity.

References

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