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The timelike Killing current and the charge of a three-chain

Physical scope

The charge associated with a timelike Killing symmetry of the smooth classical branch of the gravitational framework: the Killing current built from a smooth stress-energy tensor and its flux through finite smooth singular three-chains on a chosen oriented domain. It has an energy reading in joules when the Killing field is normalized with a length-valued flow parameter under the length-coordinate convention; other normalizations carry the corresponding scale in the charge's units. The item asserts no conservation, no finiteness for unbounded chains, no positivity and no measurement. With divergence-free T and Killing symmetry, the current lemma supplies conservation up to side flux; the field law is one possible source of that divergence condition. The definition applies only where the stated timelike Killing field exists.

Definition

Let (M,g,N) be a time-oriented smooth Lorentzian four-manifold (Smooth time-oriented Lorentzian four-manifolds: the geometric objects of the model), let U⊆M be a nonempty open subset carrying the restricted smooth structure of An open subset of a smooth manifold has a canonical restricted smooth structure, choose an orientation on U and its metric volume form (independent of the time orientation), let T be a smooth symmetric covariant 2-tensor field on U (Smooth covariant 2-tensor fields on a smooth manifold) — in an application this is the stress-energy tensor field of the model's matter sector (Stress-energy tensor field of a model) — and let ξ be a Killing field of (M,g) on U (Killing fields of a Lorentzian metric, Killing fields and conserved currents, and on-shell conservation of the Hilbert stress-energy tensor clause (a)) that is everywhere timelike and future-directed,

gp(ξp,ξp)<0,gp(ξp,Np)<0for every p∈U.

Put X:=−g(ξ,ξ)>0 on U and n:=ξ/X, an observer congruence on U: g(n,n)=−1 and g(n,N)=g(ξ,N)/X<0 (Observer congruences, their observer curves and adapted charts).

(a) Killing current. The Killing current of the pair (T,ξ) is the smooth vector field on U

Jξa:=Tabξb.

Since ξ=Xn and Ja=−Tabnb, one has Tabξb=−XJa, where J=−T(⋅,n) is the measured energy-momentum current of The observer split of a symmetric two-tensor: energy density, energy-momentum current, flux and stress; no conservation of Jξ is asserted by this definition.

(b) Killing charge of a three-chain. For every finite smooth singular 3-chain Σ of M contained in U, the Killing charge of Σ with respect to ξ is the real number

Qξ(Σ):=−ΦJξ(Σ),

where ΦJξ is the flux of the current Jξ through 3-chains on the oriented open submanifold U in the sense of The metric volume form, current flux through 3-faces and finite-chain charges clause (b).

When ξ is normalized with a length-valued flow parameter in the SI length-coordinate convention, this charge is read as a Killing energy.

(c) Relation to the measured energy current. Since Jξ=−XJ,

Qξ(Σ)=ΦXJ(Σ),

the flux of the redshift-weighted measured energy current XJ. For a 3-simplex σ that is non-null with velocity basis (v1,v2,v3) and adapted unit normal ν∗ (so that (ν∗,v1,v2,v3) is positively oriented and ε:=g(ν∗,ν∗)∈{−1,1}), the pullback of ιXJvolg is ε g(XJ,ν∗)∣det⁡(g(vi,vj))∣ dt1∧dt2∧dt3 (Divergence, Stokes flux balance and the non-null face formula for a Lorentzian current clause (c)); when ν∗=−n and the vi span n⊥ this coefficient equals −Xμ∣det⁡(g(vi,vj))∣, so up to the orientation sign carried by the adapted normal, Qξ(Σ) is the integral of the redshift-weighted measured energy density Xμ over Σ. The factor X carries the normalization and units of ξ.

(d) Reading and scope. Qξ(Σ) is the charge that the model assigns to the chain Σ under the symmetry ξ, in the framework of the postulates Adopted spacetime model and classical domain of the gravitational framework, Adopted matter-content assumptions: fields, equations, stress-energy and energy conditions with the assigned tensor and symmetry; it does not require the field law for its definition. Under the unit conventions of SI unit and coordinate conventions of the classical gravitational framework, if T is read in J m−3 and the flow parameter of ξ is measured in metres, then X is dimensionless and Qξ(Σ) is read in J. More generally, if that parameter has unit S, then in a length-coordinate chart X has units m/S and Qξ has units J m/S; converting it to an energy requires an explicitly specified normalization factor. The value depends on the model, on ξ (replacing ξ by a dimensionless constant multiple λξ with λ>0 multiplies X, Jξ and Qξ by λ), and on the chain Σ. The definition asserts no conservation, no positivity, no finiteness for unbounded chains and no measured value. If additionally ∇aTab=0 on U, the Killing current lemma gives conservation up to the side flux. The field law (Adopted Einstein field equation in the direct-equation presentation or Adopted classical gravitational action and variational field law) is one way to supply this divergence condition; it is not necessary for the mathematical conservation implication. If no timelike Killing field exists on U, Qξ is not defined by this item.

Depends on

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