Chapter 16: Weak Field Limit

The weak field limit connects general relativity to Newtonian gravity and provides the framework for understanding gravitational waves, gravitational lensing, and post-Newtonian corrections to orbital dynamics.

Linearized Gravity

For weak gravitational fields, the metric is a small perturbation of flat spacetime:

\(g_{\mu\nu} = \eta_{\mu\nu} + h_{\mu\nu}, \quad |h_{\mu\nu}| \ll 1\)

Ξ·ΞΌΞ½ = Minkowski metric, hΞΌΞ½ = perturbation

Weak-Field Metric: Flat Spacetime + Small PerturbationΞ·ΞΌΞ½ (Minkowski)Flat spacetime+hΞΌΞ½ (perturbation)MSlightly curvedhβ‚€β‚€ = -2Ξ¦/cΒ²|hΞΌΞ½| β‰ͺ 1The gravitational potential Ξ¦ maps directly to the time-time metric perturbation

To linear order in h, the Einstein tensor becomes:

\(G^{(1)}_{\mu\nu} = \frac{1}{2}\left( \partial^\rho \partial_\mu h_{\nu\rho} + \partial^\rho \partial_\nu h_{\mu\rho} - \Box h_{\mu\nu} - \partial_\mu \partial_\nu h - \eta_{\mu\nu}(\partial^\rho \partial^\sigma h_{\rho\sigma} - \Box h) \right)\)

where h = Ξ·ΞΌΞ½hΞΌΞ½ and β–‘ = βˆ‚ΞΌβˆ‚ΞΌ

Gauge Freedom

Infinitesimal coordinate transformations give gauge freedom in hΞΌΞ½:

\(h_{\mu\nu} \to h_{\mu\nu} + \partial_\mu \xi_\nu + \partial_\nu \xi_\mu\)

Lorenz Gauge (Harmonic)

\(\partial^\mu \bar{h}_{\mu\nu} = 0\)

where \(\bar{h}_{\mu\nu} = h_{\mu\nu} - \frac{1}{2}\eta_{\mu\nu}h\)

Wave Equation

\(\Box \bar{h}_{\mu\nu} = -\frac{16\pi G}{c^4} T_{\mu\nu}\)

Gravitational waves!

Gravitational Waves

In vacuum (TΞΌΞ½ = 0), the wave equation \(\Box \bar{h}_{\mu\nu} = 0\) has plane wave solutions:

\(h_{\mu\nu} = \epsilon_{\mu\nu} e^{ik_\rho x^\rho}\)

kΞΌkΞΌ = 0 (null wavevector)

Transverse-Traceless (TT) Gauge

For wave propagating in z-direction:

\(h^{TT}_{\mu\nu} = \begin{pmatrix} 0 & 0 & 0 & 0 \\ 0 & h_+ & h_\times & 0 \\ 0 & h_\times & -h_+ & 0 \\ 0 & 0 & 0 & 0 \end{pmatrix} \cos(\omega t - kz)\)

Two polarizations: plus (+) and cross (Γ—)

Interactive Simulation: Gravitational Wave Effects

Run this Python code to visualize how gravitational waves deform a ring of test masses. The simulation shows both plus (+) and cross (Γ—) polarizations at different phases, with the amplitude exaggerated for visibility. Try modifying the parameters!

Gravitational Wave Visualization

Python

Visualize GW effects on test masses in the weak field limit

weak_field_gw.py163 lines

Click Run to execute the Python code

Code will be executed with Python 3 on the server

Fortran: Linearized Gravity Analysis

This Fortran code demonstrates the weak field equations, calculates GW150914-like event parameters, and shows how LIGO detects gravitational waves through tiny length changes.

Gravitational Wave Visualization

Python

GW strain waveform and detection parameters

weak_field_plot.py149 lines

Click Run to execute the Python code

Code will be executed with Python 3 on the server

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