Ernst equation
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In general relativity, the Ernst equation[1] is an integrable non-linear partial differential equation, named after the American physicist Template:Ill 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 Ehlers 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
- ↑ Weisstein, Eric W, Ernst equation, MathWorld--A Wolfram Web.
- ↑ Ernst, F. J. (1968). New formulation of the axially symmetric gravitational field problem. Physical Review, 167(5), 1175.
- ↑ Template:Cite web
- ↑ Chandrasekhar, S. (1998). The mathematical theory of black holes (Vol. 69). Oxford university press.
- ↑ Chandrasekhar, S. (1986). Cylindrical waves in general relativity. Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences, 408(1835), 209-232.
- ↑ Template:Cite journal
- ↑ Template:Cite conference