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 Z is given by[4]

ℜ(Z)∇2Z=∇Z⋅∇Z

where ∇ is the two-dimensional gradient operator with axisymmetry; for instance, if Z=Z(ρ,z), then

ℜ(Z)[1ρ∂∂ρ(ρ∂Z∂ρ)+∂2Z∂2z]=(∂Z∂ρ)2+(∂Z∂z)2.

and if Z=Z(t,ρ) (with c=1), then[5]

ℜ(Z)[∂2Z∂2t−1ρ∂∂ρ(ρ∂Z∂ρ)]=(∂Z∂t)2+(∂Z∂ρ)2.

where ℜ(Z) is the real part of Z. If Z is a solution of the Ernst's equation, then Z/(1+icZ) (so is Z−1) is also a solution where c is an arbitrary real constant. The transformation Z→Z/(1+icZ) belongs to the so-called Ehlers transformation.

Often, one introduces

Z=−1+E1−E

so that we have

(1−|E|2)∇2E=−2E∗∇E⋅∇E.

The Ernst equation is derivable from the Lagrangian density

ℒ=∇Z⋅∇Zℜ(Z)2=∇E⋅∇E∗(1−|E|)2.

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

  1. ↑ Weisstein, Eric W, Ernst equation, MathWorld--A Wolfram Web.
  2. ↑ Ernst, F. J. (1968). New formulation of the axially symmetric gravitational field problem. Physical Review, 167(5), 1175.
  3. ↑ Template:Cite web
  4. ↑ Chandrasekhar, S. (1998). The mathematical theory of black holes (Vol. 69). Oxford university press.
  5. ↑ Chandrasekhar, S. (1986). Cylindrical waves in general relativity. Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences, 408(1835), 209-232.
  6. ↑ Template:Cite journal
  7. ↑ Template:Cite conference

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