🌌 Scalaron Screening Mechanism
Scalaron gradients renormalize Newton's G at large r, yielding a logarithmic tail that screens the 1/r² fall-off.
📐 From Field Equation to Modified Gravity
Klein-Gordon equation for the scalaron field Φ with mass m_s
Weak-field limit gives modified Poisson equation with logarithmic screening
Show 4-step derivation
- Start from \\(f(R) = R + \\beta R^2\\) → introduce scalar field via \\(e^{2\\kappa\\phi}\\tilde{g}_{\\mu\\nu}\\)
- Linear weak-field limit: \\(g_{\\mu\\nu} = \\eta_{\\mu\\nu} + h_{\\mu\\nu}\\), retain terms to \\(\\mathcal{O}(h,\\phi)\\)
- Identify scalaron mass: \\(m_s^{-2} = 6\\beta\\) ⇒ Klein-Gordon \\((\\Box - m_s^2)\\phi = -\\kappa T\\)
- Static Green's function in 3-D: \\(\\phi(r) = -\\frac{\\kappa M}{4\\pi r}\\left[1 + \\alpha\\ln\\left(\\frac{r}{r_0}\\right)\\right]\\) with \\(\\alpha = \\frac{\\kappa^2 M}{4\\pi m_s^2}\\)
Substituting \\(\\Phi = \\phi + \\Phi_N\\) yields the modified force law quoted above.
The full algebra is omitted here for clarity — see Math Ref §5 or open the Jupyter notebook for the complete derivation.
Source keys: 13.2 §B eq (17) → 13.99 §C eq (3)
🔄 Modified Force Law & Gravitational Potential
Modified Gravitational Force
Screened Potential
Think gelatin: near a spoon (high density) it flows, far away it stiffens. Scalaron's curvature-coupling makes the effective G run with scale, so gravity 'fat-tails' instead of fading.
🎮 Interactive Rotation Curve Explorer
Select a galaxy or enter a flat velocity to see how scalaron screening creates the rotation curve
📊 Galaxy Parameters
Galaxy | v_flat (km/s) | α | r₀ (kpc) | Reference |
---|---|---|---|---|
Milky Way | 220 | 5.4 × 10⁻⁷ | 1.1 | SPARC Database |
M33 | 180 | 3.8 × 10⁻⁷ | 0.9 | SPARC Database |
NGC 2403 | 135 | 2.0 × 10⁻⁷ | 0.8 | SPARC Database |
M31 (Andromeda) | 250 | 6.9 × 10⁻⁷ | 1.5 | Corbelli et al. 2010 |
NGC 3198 | 155 | 2.7 × 10⁻⁷ | 1.0 | SPARC Database |
NGC 2841 | 230 | 5.9 × 10⁻⁷ | 1.2 | SPARC Database |
UGC 2885 | 300 | 1.0 × 10⁻⁶ | 2.0 | Rubin et al. 1985 |
NGC 6503 | 120 | 1.6 × 10⁻⁷ | 0.7 | SPARC Database |
IC 2574 | 70 | 5.4 × 10⁻⁸ | 0.5 | SPARC Database |
NGC 7331 | 245 | 6.7 × 10⁻⁷ | 1.3 | SPARC Database |