Math 2.0

Relativity and gravitational theory Exact solutions Example

Ellis wormhole

Builds on Ricci curvatureEnergy conditions

Example

Use units where the gravitational constant and the speed of light equal 11. Fix n>0n > 0. On ℝ×ℝ×S2\R \times \R \times S^2 with coordinates (t,ℓ,θ,ϕ)(t, \ell, \theta, \phi), the Ellis wormhole is the metric g=−dt2+dℓ2+(ℓ2+n2)(dθ2+sin⁡2θ dϕ2).g = -dt^2 + d\ell^2 + \left(\ell^2 + n^2\right)\left(d\theta^2 + \sin^2\theta\, d\phi^2\right).

Check that it is a wormhole: the areal radius r(ℓ)=ℓ2+n2r(\ell) = \sqrt{\ell^2 + n^2} has its minimum nn at ℓ=0\ell = 0, which is the throat. As ℓ→±∞\ell \to \pm\infty, r(ℓ)/∣ℓ∣→1r(\ell)/\abs{\ell} \to 1, so the two ends are asymptotically flat, and gtt=−1g_{tt} = -1 never vanishes, so there is no horizon.

Its Ricci curvature has one nonzero component, Rℓℓ=−2n2(ℓ2+n2)2.R_{\ell\ell} = -\frac{2n^2}{\left(\ell^2 + n^2\right)^2}. For the null vector k=∂t+∂ℓk = \partial_t + \partial_\ell this gives Rabkakb<0R_{ab}k^ak^b < 0 everywhere, so the null energy condition fails. This Ricci tensor is the one produced by a massless scalar field φ=14πarctan⁡(ℓ/n)\varphi = \frac{1}{\sqrt{4\pi}}\arctan(\ell/n) whose kinetic energy has the opposite of the usual sign, through Rab=−8π ∂aφ ∂bφR_{ab} = -8\pi\, \partial_a\varphi\, \partial_b\varphi. Indeed 8π(φ′)2=2n2/(ℓ2+n2)28\pi(\varphi')^2 = 2n^2/(\ell^2 + n^2)^2.

The Ellis wormhole has zero mass at both ends: gtt=−1g_{tt} = -1 means that a particle at rest feels no gravitational pull. A free particle can cross the throat from one end to the other in finite time.

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  1. Energy conditions concept
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Further reading

  1. Web https://en.wikipedia.org/wiki/Ellis_wormhole
About this page
TagNGK91EV37X
URIm2://NGK91EV37X
Kindexample
WritingW0 stub
MSC83C15, 83C99
Instance ofWormhole
UsesRicci curvature, Energy conditions
Same as
Changed3 November 2026

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