Implement a self-consistent Einstein-matter coupling solver to replace prescribed potentials with dynamically determined solutions.
Motivation
Current implementation uses prescribed Rodal-style potentials. A full solver would:
- Ensure consistency between geometry and matter distribution
- Enable exploration of physically realizable configurations
- Provide stronger validation against known exact solutions
Technical Approach
- Implement iterative ADM constraint solver
- Add matter stress-energy tensor computation from prescribed sources
- Couple potential φ evolution to Einstein equations
- Validate against:
- Schwarzschild metric (static limit)
- Boosted Schwarzschild (kinematic check)
- Known warp-drive solutions
Dependencies
- Robust PDE solver (consider FEniCS or custom finite-difference)
- Convergence criteria for constraint satisfaction
- Comprehensive test suite with known solutions
References
- Baumgarte & Shapiro (2010): Numerical Relativity
- Alcubierre (2008): Introduction to 3+1 Numerical Relativity
Priority: High (v0.2.0 target)
Complexity: High
Implement a self-consistent Einstein-matter coupling solver to replace prescribed potentials with dynamically determined solutions.
Motivation
Current implementation uses prescribed Rodal-style potentials. A full solver would:
Technical Approach
Dependencies
References
Priority: High (v0.2.0 target)
Complexity: High