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I was reading the last part this answer by John Rennie, and I am bit confused about magnitude of each component of 4-acceleration when standing on the surface of the Earth compared to standing in an elevator accelerating upwards in outer space by $g$. I want to check if I understood correctly.

In both situations, (assume the origin of the inertia reference frame is on the surface with positive $z$-axis oriented radially outward) the z-component of the 4-acceleration is

$$A^3=A_\text{SR}^3+A_\text{GR}^3=g$$

right?

When you're at rest on the Earth, $A_\text{SR}^3=0$ and $A_\text{GR}^3=g$. On the other hand, if you're at rest in an accelerating elevator, $A_\text{SR}^3=g$ and $A_\text{GR}^3=0$?

What about other components $A^0, A^1, A^2$? Are they all zero?

On a related note, the comments to the answer of the recent question of mine gave me some food for thought. In particular, I learned that the one reason why the components 4-acceleration vanish during free fall on Earth is because

$$A^\lambda=\frac{dU^\lambda }{d\tau } + \Gamma^\lambda {}_{\mu \nu}U^\mu U^\nu=-g+g=0$$

I wonder if it is true for $\lambda=3$ (z-component) only? For other components $\lambda=0,1,2$: $$\frac{dU^\lambda }{d\tau }=\Gamma^\lambda {}_{\mu \nu}U^\mu U^\nu=0$$ right?

Amit
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Jimmy Yang
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1 Answers1

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Yes, all of the other components of the four-acceleration are 0 in both cases. See the Catalogue of Spacetimes.

Section 2.1.6 describes accelerating coordinates in flat spacetime. Here they use $(\rho,y,z)$ for the spatial coordinates with the acceleration in the $\rho$ direction. Note that the Christoffel symbols involving $y$ and $z$ are all $0$.

Section 2.2.1 describes the usual coordinates in a spherically symmetric spacetime. Here the acceleration is in the $r$ direction. The Christoffel symbols involving the other directions are not all zero, so it isn't as clear as the previous case. However, note that only the $r$ direction has any Christoffel symbols with time $t$. So the Christoffel symbols involving the other directions are not related to fictitious forces but rather to the spherical instead of Cartesian spatial coordinates.

Dale
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