Devin
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Let a mass oscillate with relativistic acceleration (sinusoidal) by means which are irrelevant. What does the gravitational field look like a distance R away?
The discussion revolves around the gravitational field produced by a mass oscillating with relativistic acceleration, specifically in the context of general relativity and Einstein's field equations. Participants explore the implications of oscillation on energy-momentum conservation and the necessity of specifying the mechanism behind the oscillation.
Participants generally agree on the necessity of a mechanism for oscillation to be meaningful in the context of gravitational fields, but there is no consensus on the specifics of such mechanisms or their implications.
The discussion highlights the dependence on definitions and the need for detailed specifications of mechanisms involved in oscillation, as well as the unresolved mathematical implications of energy-momentum conservation in this context.
What if perhaps we had a mechanism that made it such that the mass oscillates with constant /omegapervect said:If one considers a sinusoidal mass oscillating in isolation, one finds that ##\nabla_a T^{ab}## is not equal to zero, while ##\nabla_a G^{ab} = 0##. As a consequence one cannot satisfy Einstein's field equations ##T^{ab} = 8 \pi G^{ab}## as taking the covariant derivative of each side yields the result that ##\nabla_a T^{ab} = \nabla_a G^{ab}##, but this is not possible.
Thus one is lead to the conclusion that the means by which the mass is made to osscilate cannot be ignored.. Another way of saying this that may be simpler - one needs the source to conserve energy-momentum (the precise mathematical statement of this idea is that ##\nabla_a T^{ab} = 0## ) in order to be able to apply Einstein's field equations in the first place. And an oscillating mass doesn't do that by itself, it needs help.