Locally Maximally Symmetric Spacetimes

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SUMMARY

Every general curved spacetime is locally Lorentz, allowing for a coordinate chart where the metric tensor \( g_{ab} = \eta_{ab} \) at a specific event, with all connection coefficients vanishing at that point. However, this does not imply that the curvature scalar \( R \) is zero, nor does it mean that the spacetime is locally maximally symmetric. In fact, most general curved spacetimes lack symmetries, such as Killing vector fields, and cannot be classified as locally maximally symmetric, even in high curvature scenarios.

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HomerSimpson
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Can one say that every general curved spacetime, locally is maximally symmetric?
I know that one can say that every general curved spacetime is locally flat (and therefore maximally symmetric with R=0), but I'm talking about a very high curvature spacetime, where still we can consider nonzero curvatures.
 
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HomerSimpson said:
Can one say that every general curved spacetime, locally is maximally symmetric?

What do you mean by "maximally symmetric"? Most general curved spacetimes have no symmetries at all (i.e., no Killing vector fields).

HomerSimpson said:
I know that one can say that every general curved spacetime is locally flat (and therefore maximally symmetric with R=0)

No, you can't say that. What you can say is that every general curved spacetime is locally Lorentz, meaning that at a given event, you can choose a coordinate chart that makes ##g_{ab} = \eta_{ab}## at that event, and makes all of the connection coefficients (first derivatives of ##g_{ab}##) vanish at that event. But that doesn't make ##R = 0##.
 
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Thanks for you replay Peter, but I'm still a little bit confused.

PeterDonis said:
What do you mean by "maximally symmetric"? Most general curved spacetimes have no symmetries at all (i.e., no Killing vector fields).

I know it, but I meant "locally" not globally.


PeterDonis said:
No, you can't say that. What you can say is that every general curved spacetime is locally Lorentz, meaning that at a given event, you can choose a coordinate chart that makes ##g_{ab} = \eta_{ab}## at that event, and makes all of the connection coefficients (first derivatives of ##g_{ab}##) vanish at that event. But that doesn't make ##R = 0##.

What you mention here, looks like the Riemann normal coordinate, is it?

PeterDonis said:
But that doesn't make ##R = 0##.

Can we assume that R is almost constant as in maximally symmetric spacetimes and therefore R_{ab}\propto Rg_{ab}?


What I get from your answer, is we can not say that a general high curved spacetime, is "locally" maximally symmetric. Am I right?
 
HomerSimpson said:
What I get from your answer, is we can not say that a general high curved spacetime, is "locally" maximally symmetric. Am I right?
That's right. And you can strike the word "high". A general curved spacetime is not locally maximally symmetric.

Since the Riemann tensor has dimension L-2, curvature only sets a length scale, and you can only say it's large or small in comparison to some other length.
 
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