Devin
- 24
- 1
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 centers on the implications of relativistic mass oscillation and its effect on gravitational fields at a distance R. It establishes that for an oscillating mass, the covariant derivative of the energy-momentum tensor, ##\nabla_a T^{ab}##, does not equal zero, while the covariant derivative of the Einstein tensor, ##\nabla_a G^{ab}##, does equal zero. This discrepancy indicates that energy-momentum conservation, expressed as ##\nabla_a T^{ab} = 0##, is essential for applying Einstein's field equations, thus necessitating an external mechanism to facilitate the oscillation. The discussion concludes that without such a mechanism, one cannot derive solutions for an oscillating mass.
PREREQUISITESThis discussion is beneficial for theoretical physicists, researchers in general relativity, and students studying advanced mechanics, particularly those interested in the interplay between mass oscillation and gravitational fields.
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.