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gravity.txt
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| Gravity Theories Dichotomy Tree | |
| (Branching based on key decision points: conceptual, mathematical, and physical choices leading to each theory's existence) | |
| Root: Fundamental View of Gravity | |
| ├── As a Field (Classical, Force-based) | |
| │ ├── Non-Relativistic (Absolute time/space) | |
| │ │ ├── Scalar Potential (Newtonian Gravity) | |
| │ │ │ - Decision: Instantaneous action? Yes → Poisson's equation (∇²φ = 4πGρ) | |
| │ │ │ - Exists due to: Empirical laws (e.g., inverse square) + field concept from EM analogy | |
| │ │ └── Tensorial Reformulation (To geometrize) | |
| │ │ ├── Degenerate Metrics (Rank-deficient) | |
| │ │ │ - Decision: Separate time/space? Yes → Newton-Cartan (NC) | |
| │ │ │ - Equations: R_{μν} = 4πG ρ t_{μν} | |
| │ │ │ - Exists due to: Need for diff-invariance in Newtonian limit + GR inspiration (Cartan/Ehlers) | |
| │ │ └── Non-Degenerate (But still non-rel) | |
| │ │ - Decision: Add extra dims? → Bargmann lift (5D non-deg for NC) | |
| │ │ - Exists due: Resolve degeneracy for math tractability | |
| │ └── Relativistic (Finite speed, Lorentz inv) | |
| │ ├── Weak Field Approximation | |
| │ │ - Decision: Linearize GR? Yes → Effective Field Theory (EFT) for gravity | |
| │ │ - Exists due: Quantum field theory needs + low-energy GR | |
| │ └── Full Tensor Field (But geometric) | |
| │ - (Merges into Geometry branch below) | |
| └── As Geometry (Curvature-based) | |
| ├── Non-Relativistic (Galilean inv) | |
| │ - Decision: Geometrize Newtonian? Yes → Newton-Cartan (as above, unified branch) | |
| │ - Exists due: Bridge Newtonian to GR (1920s, Cartan) | |
| ├── Relativistic (Lorentz inv) | |
| │ ├── Classical (No quanta) | |
| │ │ ├── Vacuum Solutions Focus | |
| │ │ │ - Decision: Matter curves space? Yes → General Relativity (GR) | |
| │ │ │ - Equations: G_{μν} = 8πG/c⁴ T_{μν} | |
| │ │ │ - Exists due: Equivalence principle + special rel (Einstein 1915) | |
| │ │ └── With Torsion/Non-Metricity | |
| │ │ - Decision: Allow spin/torsion? Yes → Einstein-Cartan Theory | |
| │ │ - Exists due: Couple to fermionic matter (1920s, Cartan) | |
| │ └── Quantum (Incorporate quanta) | |
| │ ├── Background-Dependent (Perturbative) | |
| │ │ - Decision: Quantize metric perturbations? Yes → Quantum GR (non-renorm) | |
| │ │ - Exists due: Semiclassical attempts (e.g., Hawking radiation) | |
| │ ├── Background-Independent (Non-pert) | |
| │ │ ├── Discrete Space | |
| │ │ │ - Decision: Loop quantize? Yes → Loop Quantum Gravity (LQG) | |
| │ │ │ - Exists due: Canonical quantization of GR (1980s, Ashtekar) | |
| │ │ └── String-Based | |
| │ │ - Decision: Higher dims/vibrations? Yes → String Theory/M-Theory | |
| │ │ - Exists due: Unify all forces (1970s, superstrings) | |
| │ └── Broken Symmetry (e.g., for UV completion) | |
| │ - Decision: Anisotropic scaling? Yes → Hořava-Lifshitz Gravity | |
| │ - Exists due: Renormalizable quantum gravity + NC limit (2009, Hořava) | |
| └── Beyond Standard (Modified/Alternative) | |
| ├── For Dark Phenomena | |
| │ - Decision: Modify Newtonian? Yes → MOND (Modified Newtonian Dynamics) | |
| │ - Exists due: Galactic rotation curves (1980s, Milgrom) | |
| └── Emergent Gravity | |
| - Decision: Gravity from entropy? Yes → Verlinde's Entropic Gravity | |
| - Exists due: Holographic/thermodynamic views (2010s) |
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