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Mean-curvature variation and the stationary lapse equation
Statement
Let be a smooth time-oriented Lorentzian four-manifold, and let be a smooth local variation through spacelike embeddings of a smooth spacelike hypersurface , with the inclusion. Write for the future unit normal, for the induced metric, , and . Let the variational vector field be , where is tangent and . Then the derivative at of the pulled-back mean curvature is . Here and .
If on and a Killing field decomposes along it as , then . This local identity asserts no boundary values or normalization at an end.
Statement references
Spacelike sections, maximality and lapse–shift data
Normal graphs and the nonlinear mean-curvature map
Stationary Lorentzian data and tensor conventions
Laplace–Beltrami operator as the trace of the Hessian
Gradient hessian and divergence connection formulas
The algebraic symmetries of the curvature tensor and the symmetry of the Ricci and Einstein tensors
A tensor field is flow-invariant exactly when its Lie derivative vanishes
Facts & Assumptions
The spacelike hypersurface data give the future normal, induced metric, sign convention for , mean curvature and normal–tangential decomposition. Spacelike sections, maximality and lapse–shift data
The mean-curvature map pulls the mean curvature of each admissible spacelike graph back to the original hypersurface. Normal graphs and the nonlinear mean-curvature map
A Killing field has local flow preserving , and the curvature convention is , with . The Killing condition and curvature convention are supplied by the stationary data; flow invariance follows from vanishing metric Lie derivative on each local flow domain. Stationary Lorentzian data and tensor conventions A tensor field is flow-invariant exactly when its Lie derivative vanishes
The smooth nondegenerate metric has a unique torsion-free metric-compatible connection, extended to tensor fields. Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields
For the smooth induced Riemannian metric , the intrinsic operators satisfy , , and , where is the Levi–Civita connection of . Thus . Gradient hessian and divergence connection formulas Laplace–Beltrami operator as the trace of the Hessian
The curvature tensor of a smooth time-oriented Lorentzian four-manifold with its metric-selected connection has the algebraic curvature symmetries, in particular , with the curvature and Ricci conventions used here. The algebraic symmetries of the curvature tensor and the symmetry of the Ricci and Einstein tensors
Proof
Given: The variation and geometric data in the Statement.
Goal: Derive the variation formula and its consequence for a maximal hypersurface moved by a Killing flow.
First suppose . In local coordinates on , put and at . Differentiating and , using torsion-freeness and , gives at . Metric compatibility also gives and .
Commuting the covariant derivatives by the curvature convention and differentiating gives , where is the Levi–Civita connection of . Using from F5, tracing this identity and including yields . The displayed Ricci convention and the curvature symmetries of the metric-compatible torsion-free connection give , proving the formula for a normal variation.
For a general variation, locally reparametrize the domain by a time-dependent diffeomorphism whose initial velocity cancels . The resulting variation has initial velocity ; differentiating the scalar pullback under the inverse reparametrization adds . This proves the stated formula for arbitrary ; the graph mean-curvature map uses the same pullback convention.
By F3 the local flow of a Killing field consists of local isometries. Transporting by a local isometry gives a torsion-free metric-compatible connection, which equals by uniqueness in F4. The flow starts at the identity and hence preserves future direction on its local flow domain. It therefore carries the future normal and mean curvature of to those of the image hypersurface. Its pulled-back mean curvature is therefore constant in the flow parameter. Its variational field is ; if , then , and the variation formula gives the stated lapse equation. The calculation is local and imposes no boundary or asymptotic condition.
External input
Gourgoulhon records the maximal-slicing lapse equation under the 3+1 Einstein-equation conventions; the more general geometric variation above is derived locally.
Depends on
- Spacelike sections, maximality and lapse–shift data
- Normal graphs and the nonlinear mean-curvature map
- Stationary Lorentzian data and tensor conventions
- Existence and uniqueness of the metric-selected connection of a nondegenerate metric, and its extension to tensor fields
- Laplace–Beltrami operator as the trace of the Hessian
- Gradient hessian and divergence connection formulas
- The algebraic symmetries of the curvature tensor and the symmetry of the Ricci and Einstein tensors
- A tensor field is flow-invariant exactly when its Lie derivative vanishes
- E. Gourgoulhon, 3+1 Formalism and Bases of Numerical Relativity (2007) · Section 9.2.2, equations (9.4) and (9.15), printed pp. 153–155
Used by · 8
- Remark 1.3: lapse bounds and stationary product
- Mean-curvature linearization, weighted regularity and fixed-boundary graph map
- Transformed lapse equation and bounds
- Identification of the spherical exterior and its positive stationary lapse
- The global Dirichlet mean-curvature map is continuously differentiable
- Flattening a smooth fixed boundary preserves the elliptic graph equation
- Compact estimates for arbitrary sequences of individually existing slices
- A supplied complete maximal slice has zero extrinsic curvature in the zero-shift case
Dependency tree · 2 levels
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External dependencies
A maximal slicing has zero mean curvature and obeys the displayed elliptic lapse equation when the maximal condition is maintained.
Hypotheses: The 3+1 foliation and Einstein-equation conventions used in the cited section.
Reading limits: Consulted Section 9.2.2, equations (9.4) and (9.15), printed pp. 153 and 155 (PDF pages 153 and 155). These equations record maximal slicing and its elliptic lapse equation under the stated Einstein-equation conventions. This is background only; the full geometric variation formula and its sign conventions are proved locally below.
Sources
- E. Gourgoulhon, 3+1 Formalism and Bases of Numerical Relativity (2007) · Section 9.2.2, equations (9.4) and (9.15), printed pp. 153–155