Killing tensor

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Short description: Tensor in general relativity

In mathematics, a Killing tensor or Killing tensor field is a generalization of a Killing vector, for symmetric tensor fields instead of just vector fields. It is a concept in Riemannian and pseudo-Riemannian geometry, and is mainly used in the theory of general relativity. Killing tensors satisfy an equation similar to Killing's equation for Killing vectors. Like Killing vectors, every Killing tensor corresponds to a quantity which is conserved along geodesics. However, unlike Killing vectors, which are associated with symmetries (isometries) of a manifold, Killing tensors generally lack such a direct geometric interpretation. Killing tensors are named after Wilhelm Killing.

Definition and properties

In the following definition, parentheses around tensor indices are notation for symmetrization. For example:

T(αβγ)=16(Tαβγ+Tαγβ+Tβαγ+Tβγα+Tγαβ+Tγβα)

Definition

A Killing tensor is a tensor field K (of some order m) on a (pseudo)-Riemannian manifold which is symmetric (that is, Kβ1⋯βm=K(β1⋯βm)) and satisfies:[1][2]

∇(αKβ1⋯βm)=0

This equation is a generalization of Killing's equation for Killing vectors:

∇(αKβ)=12(∇αKβ+∇βKα)=0

Properties

Killing vectors are a special case of Killing tensors. Another simple example of a Killing tensor is the metric tensor itself. A linear combination of Killing tensors is a Killing tensor. A symmetric product of Killing tensors is also a Killing tensor; that is, if Sα1⋯αl and Tβ1⋯βm are Killing tensors, then S(α1⋯αlTβ1⋯βm) is a Killing tensor too.[1]

Every Killing tensor corresponds to a constant of motion on geodesics. More specifically, for every geodesic with tangent vector uα, the quantity Kβ1⋯βmuβ1⋯uβm is constant along the geodesic.[1][2]

Examples

Since Killing tensors are a generalization of Killing vectors, the examples at Killing vector field § Examples are also examples of Killing tensors. The following examples focus on Killing tensors not simply obtained from Killing vectors.

FLRW metric

The Friedmann–Lemaître–Robertson–Walker metric, widely used in cosmology, has spacelike Killing vectors corresponding to its spatial symmetries, in particular rotations around arbitrary axes and in the flat case for k=1 translations along x, y, and z. It also has a Killing tensor

Kμν=a2(gμν+UμUν)

where a is the scale factor, Uμ=(1,0,0,0) is the t-coordinate basis vector, and the −+++ signature convention is used.[3]

Kerr metric

The Kerr metric, describing a rotating black hole, has two independent Killing vectors. One Killing vector corresponds to the time translation symmetry of the metric, and another corresponds to the axial symmetry about the axis of rotation. In addition, as shown by Walker and Penrose (1970), there is a nontrivial Killing tensor of order 2.[4][5][6] The constant of motion corresponding to this Killing tensor is called the Carter constant.

Conformal Killing tensor

Conformal Killing tensors are a generalization of Killing tensors and conformal Killing vectors. A conformal Killing tensor is a tensor field K (of some order m) which is symmetric and satisfies[4]

∇(αKβ1⋯βm)=k(β1⋯βm−1gβmα)

for some symmetric tensor field k. This generalizes the equation for conformal Killing vectors, which states that

∇αKβ+∇βKα=λgαβ

for some scalar field λ.

Every conformal Killing tensor corresponds to a constant of motion along null geodesics. More specifically, for every null geodesic with tangent vector vα, the quantity Kβ1⋯βmvβ1⋯vβm is constant along the geodesic.[4]

The property of being a conformal Killing tensor is preserved under conformal transformations in the following sense. If Kβ1⋯βm is a conformal Killing tensor with respect to a metric gαβ, then K~β1⋯βm=umKβ1⋯βm is a conformal Killing tensor with respect to the conformally equivalent metric g~αβ=ugαβ, for all positive-valued u.[7]

Killing–Yano tensor

An antisymmetric tensor of order p, fa1a2...ap, is a Killing–Yano tensor :fr:Tenseur de Killing-Yano if it satisfies the equation

∇bfca2...ap+∇cfba2...ap=0.

While also a generalization of the Killing vector, it differs from the usual Killing tensor in that the covariant derivative is only contracted with one tensor index.

Killing–Yano tensors are the square root of Killing tensors because of satisfying certain theorems[8] which are put below:

  • For a Killing–Yano tensor, fμ1…μp, the Killing tensor of rank 2 is kμν=fμμ2…μpfνμ2…μp
  • fμμ2…μppμp is parallel transported along the geodesic with tangent vector, pμp

Conformal Killing–Yano tensors are a generalization of Killing–Yano tensors.[8] It states that a Conformal Killing–Yano tensor of rank p is totally antisymmetric tensor kμ2...μp with p-form if it fulfills:

∇μkμ1…μp=∇[μkμ1…μp]+pgμ[μ1kμ2…μp]¯

where k¯μ2…μp is an asymmetrical tensor of rank p - 1. By doing a contraction of μ and μ1, we get:

k¯μ2…μp=1D−p+1∇μkμ2…μpμ

Closed Conformal Killing–Yano tensors are a special case of Conformal Killing–Yano tensor when ∇μk∣μ2…μp∣=0 where k=db and b is some p - 1 form.[8] This follows the Hodge duality transformation result which is:

The Hodge dual k⋆ of a rank p Closed Conformal Killing–Yano tensor k is a Killing–Yano tensor f≡⋆k of rank D - p and vice-versa.

An important property of Closed Conformal Killing–Yano tensor is that their wedge product is a Closed Conformal Killing–Yano tensor of higher rank. In other words, k≡a∧b is a Closed Conformal Killing–Yano tensor of rank p + q, where a is a Closed Conformal Killing–Yano tensor of rank p and b is a Closed Conformal Killing–Yano tensor of rank q.

Examples

Kerr spacetime

A particle moving in Kerr spacetime is closely related to Conformal Killing–Yano tensors of rank two. There is one solution for a rotating blackhole described by Kerr Metric in which the asymptomatic tensor looks like as follows:[9]

Y=r3sinθdθ∧dϕ+O(1)=⋆(τ0∧D)

where D is a dilation vector field with value xμ∂∂xμ and τ is a Killing field with value ∂∂xμ

Killing–Yano towers

From the wedge product property of Closed Conformal Killing–Yano tensors, many Conformal Killing–Yano tensors can be constructed which is known as Killing–Yano tensor tower. For a nth Closed Conformal Killing–Yano tensor, the Killing–Yano tensor tower is defined as:

h(j)≡h∧j=∧n=1jh

where h(j) is a Closed Conformal Killing–Yano tensor of rank 2j.[8]

Bosonic and spinning string

In the invariances of tensionless Bosonic string, the expression for the field equation for tension in the string vanishes when K is a killing vector.[10]

∇(μKν)=λGμν

The invariant of the tensionless spinning strings also involves super conformal Killing–Yano tensors.[10]

Supersymmetries

For a bosonic particle falling in a geodesic background, the supersymmetric transformation with respect to Killing–Yano tensor can be derived.[11] One such supersymmetry transform equation is as follows:

δxμ=−i∈ξμ

G-Structures

Killing–Yano tensors are also studied in G-Structures which are used in constructing supergravity solutions and also in holonomy manifolds.[11]

See also

References

  1. ↑ 1.0 1.1 1.2 Carroll 2003, pp. 136–137
  2. ↑ 2.0 2.1 Wald 1984, p. 444
  3. ↑ Carroll 2003, p. 344
  4. ↑ 4.0 4.1 4.2 Walker, Martin; Penrose, Roger (1970), "On Quadratic First Integrals of the Geodesic Equations for Type {22} Spacetimes", Communications in Mathematical Physics 18 (4): 265–274, doi:10.1007/BF01649445, https://projecteuclid.org/journals/communications-in-mathematical-physics/volume-18/issue-4/On-quadratic-first-integrals-of-the-geodesic-equations-for-type/cmp/1103842577.pdf 
  5. ↑ Carroll 2003, pp. 262–263
  6. ↑ Wald 1984, p. 321
  7. ↑ Dairbekov, N. S.; Sharafutdinov, V. A. (2011), "On conformal Killing symmetric tensor fields on Riemannian manifolds", Siberian Advances in Mathematics 21: 1–41, doi:10.3103/S1055134411010019 
  8. ↑ 8.0 8.1 8.2 8.3 https://www.nbi.dk/~obers/MSc_PhD_files/KillingYanoProject_Dennis_final.pdf
  9. ↑ Jezierski, Jacek; Łukasik, Maciej (2005-10-12). "Conformal Yano-Killing tensor for the Kerr metric and conserved quantities" (in en). https://arxiv.org/abs/gr-qc/0510058v2. 
  10. ↑ 10.0 10.1 Lindström, Ulf; Sarıoğlu, Özgür (2022-06-10). "Tensionless strings and Killing(-Yano) tensors". Physics Letters B 829. doi:10.1016/j.physletb.2022.137088. ISSN 0370-2693. https://www.sciencedirect.com/science/article/pii/S0370269322002222. 
  11. ↑ 11.0 11.1 Santillan, Osvaldo P. (2012-04-01). "Hidden symmetries and supergravity solutions" (in en). Journal of Mathematical Physics 53 (4). doi:10.1063/1.3698087. ISSN 0022-2488. https://pubs.aip.org/jmp/article/53/4/043509/232323/Hidden-symmetries-and-supergravity-solutions. 
  • Carroll, Sean (2003), Spacetime and Geometry: An Introduction to General Relativity, ISBN 0-8053-8732-3 
  • Wald, Robert M. (1984), General Relativity, Chicago: University of Chicago Press, ISBN 0-226-87033-2