Undergrad Help Understand Retarded Function: Einstein Eq. Linearized

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The discussion centers on the linearization of the Einstein equations, leading to the weak field Einstein equations, which describe gravitational waves. The solution involves the Retarded function, where the spacetime coordinates are crucial for understanding the relationship between the observation point and the source. The expression for the Retarded function indicates that the distance between the observation point and the source is analogous to the potential calculation in electromagnetism. The conversation emphasizes the application of the retarded Green's function to solve the wave equation for each component. Understanding these concepts is essential for grasping the implications of weak gravitational fields.
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Hi people, help here please
When the Einstein equation are linearized the results are the weak field Einstein equations

$$
\left ( -\frac{\partial^{2}}{\partial t^{2}} + \nabla^{2} \right ) \bar h^{\mu\nu}=-16\pi T^{\mu\nu}
$$
a solution for this equations considering the source are the Retarded function
$$
\bar h^{\mu\nu} (t,\vec x)=4 \int d^{3}x' \frac{[T^{\mu\nu}(t',\vec x')]_{[ret]}}{|\vec x - \vec x'|}
$$
with

$$t' = t_{ret} = t-|\vec x - \vec x'|$$

until i know "t" and "x" in spacetime are the same but what physical situation describes
$$
|\vec x - \vec x'|
$$
Is similar to electromagnestism, when $$\vec x$$ represent the place where you want calculate the potencial and $$\vec x'$$ represent the place where the charge is located?

Thanks in advance
 
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Your weak field equation is just a separate wave equation for every individual component. The solution is just applying the retarded Green's function of the wave equation.
 
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