Eguchi–Hanson space

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Short description: Concept in mathematics and theoretical physics

In mathematics and theoretical physics, the Eguchi–Hanson space is a non-compact, self-dual, asymptotically locally Euclidean (ALE) metric on the cotangent bundle of the 2-sphere T*S2. The holonomy group of this 4-real-dimensional manifold is SU(2). The metric is generally attributed to the physicists Tohru Eguchi and Andrew J. Hanson; it was discovered independently by the mathematician Eugenio Calabi around the same time in 1979.[1][2]

The Eguchi-Hanson metric has Ricci tensor equal to zero, making it a solution to the vacuum Einstein equations of general relativity, albeit with Riemannian rather than Lorentzian metric signature. It may be regarded as a resolution of the A1 singularity according to the ADE classification which is the singularity at the fixed point of the C2/Z2 orbifold where the Z2 group inverts the signs of both complex coordinates in C2. The even dimensional space of dimension [math]\displaystyle{ d }[/math] can be described using complex coordinates [math]\displaystyle{ w_i \in \mathbb C^{d/2} }[/math] with a metric

[math]\displaystyle{ g_{i \bar j} = \bigg(1+\frac{\rho^d}{r^{d}}\bigg)^{2/d}\bigg[\delta_{i\bar j}-\frac{\rho^d w_i \bar w_{\bar j}}{r^2(\rho^d+r^{d})}\bigg], }[/math]

where [math]\displaystyle{ \rho }[/math] is a scale setting constant and [math]\displaystyle{ r^2 = |w|^2_{\mathbb C^{d/2}} }[/math].

Aside from its inherent importance in pure geometry, the space is important in string theory. Certain types of K3 surfaces can be approximated as a combination of several Eguchi–Hanson metrics since both have the same holonomy group. Similarly, the space can also be used to construct Calabi–Yau manifolds by replacing the orbifold singularities of [math]\displaystyle{ T^6/\mathbb Z_3 }[/math] with Eguchi–Hanson spaces.[3]

The Eguchi–Hanson metric is the prototypical example of a gravitational instanton; detailed expressions for the metric are given in that article. It is then an example of a hyperkähler manifold.[2]

References

  1. Eguchi, Tohru; Hanson, Andrew J. (1979). "Selfdual solutions to Euclidean gravity". Annals of Physics 120 (1): 82–105. doi:10.1016/0003-4916(79)90282-3. Bibcode1979AnPhy.120...82E. http://www.slac.stanford.edu/cgi-wrap/getdoc/slac-pub-2213.pdf. 
  2. 2.0 2.1 Calabi, Eugenio (1979). "Métriques kählériennes et fibrés holomorphes". Annales Scientifiques de l'École Normale Supérieure Quatrième Série, 12 (2): 269–294. doi:10.24033/asens.1367. http://www.numdam.org/item?id=ASENS_1979_4_12_2_269_0. 
  3. Polchinski, J. (1998). "17". String Theory Volume II: Superstring Theory and Beyond. Cambridge University Press. p. 309-310. ISBN 978-1551439761.