- #1
JustinLevy
- 895
- 1
Let us restrict ourselves to SR for the moment at least. So we have a flat spacetime.
Now consider a proper force of the form:
[tex]\frac{dp^\mu}{d\tau} = a v^\mu[/tex]
where [itex]a[/itex] is a scalar.
It seems to be coordinate system independent due to the definition being in tensor notation. But it seems to not have any of the poincare symmetries. How do I show this explicitly?
I'm confused since if I did a Lorentz transformation, the form is still the same, but it doesn't seem to have any conserved quantities. I know I'm confusing something very simple here. Can you help?
Now consider a proper force of the form:
[tex]\frac{dp^\mu}{d\tau} = a v^\mu[/tex]
where [itex]a[/itex] is a scalar.
It seems to be coordinate system independent due to the definition being in tensor notation. But it seems to not have any of the poincare symmetries. How do I show this explicitly?
I'm confused since if I did a Lorentz transformation, the form is still the same, but it doesn't seem to have any conserved quantities. I know I'm confusing something very simple here. Can you help?