1. The 3+1 Decomposition
The ADM formalism (Arnowitt-Deser-Misner) reformulates general relativity by splitting 4D spacetime into 3D space evolving in time. This is essential for canonical quantization and numerical relativity.
2. ADM Variables
The 4D metric g_uv is decomposed into:
| Variable | Symbol | Meaning |
|---|---|---|
| Spatial metric | gamma_ij | 3D geometry of each slice |
| Lapse | N | Proper time between slices |
| Shift | N^i | Coordinate drift between slices |
The ADM Metric
This decomposes the 10 components of g_uv into:
- 6 components in gamma_ij (symmetric 3x3 matrix)
- 1 component in N (lapse function)
- 3 components in N^i (shift vector)
3. Extrinsic Curvature
The extrinsic curvature K_ij measures how each spatial slice is embedded in 4D spacetime - how much it curves in the time direction.
4. Constraints
Not all (gamma_ij, K_ij) configurations are valid initial data for Einstein's equations. They must satisfy constraint equations:
Hamiltonian Constraint
Relates the spatial curvature and extrinsic curvature to energy density. This constraint generates time evolution.
Momentum Constraints
Relates the gradient of extrinsic curvature to momentum density. These generate spatial diffeomorphisms.
Physical Meaning
- - H = 0: Energy is conserved (no creation from nothing)
- - H_i = 0: Momentum is conserved (gauge invariance)
- - 4 constraints reduce 12 variables to 8 physical degrees of freedom
- - 2 polarizations of gravitational waves (4 more gauge freedoms)
5. Evolution Equations
Given valid initial data, the ADM formalism provides evolution equations:
6. Connection to Z2 Framework
Why ADM Matters for Z2
- - Canonical quantization: Path to quantum gravity
- - Constraint algebra: Tests consistency of compactification
- - Moduli dynamics: Extra dimension sizes as dynamical variables
- - Cosmology: FLRW metric in ADM form gives Friedmann equations
7. BSSN Formulation
For numerical stability, the ADM equations are often recast in the BSSN(Baumgarte-Shapiro-Shibata-Nakamura) form:
Exercises
- Write the Minkowski metric ds^2 = -dt^2 + dx^2 + dy^2 + dz^2 in ADM form. What are N and N^i?
- For the Schwarzschild solution in Schwarzschild coordinates, find the lapse N(r).
- Show that a flat spatial slice (K_ij = 0) in flat spacetime satisfies both constraints.
- How many independent components does K_ij have? (Hint: it is symmetric)
- Why are the constraints called "initial value" constraints?