Understanding Lie Groups' Impact on Riemannian Metrics: Preserving Manifold Structures, Exercises of Classical and Relativistic Mechanics

The concept of group actions on manifolds and how various structures on a manifold give rise to specific groups. The preservation of riemannian metrics and introduces important groups such as gl(n), o(n), so(n), and e(n). It also discusses the relationship between these groups and the galilei group, leading to the discovery of the correct group of symmetries in special relativity.

Typology: Exercises

2011/2012

Uploaded on 07/19/2012

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1 Group Actions Preserving Structures
We’ve said a bit about group actions, but I haven’t explained the most important part: how any
structure on a manifold gives a group action!
Given a manifold Xwith some extra structure (for example: a Riemannian metric - a very nice
distance function), you can ask: which diffeomorphisms f:X→Xpreserves this extra structure?
Such diffeomorphisms form a group! We get lots of interesting groups, including a lot of Lie groups.
Example: Take X=Rnand let the extra structure be the structure of the vector space. Then
f:Rn→Rnpreserves this extra structure iff:
•f(0) = 0
•f(x+y) = f(x) + f(y)
•f(αx) = αf (x)
We say fis linear. We get a group of diffeomorphisms f:X→Xpreserving the vector space
structure:
G= GL(n)
={f:Rn→Rn:fis linear and invertible}
Example: Let X=Rnbut with its vector space structure and its usual metric. The group
preserving this structure is
G= O(n)
={f∈GL(n) : ||f(x)|| =||x||}
If we also demand that our transformations preserve an ā€˜orientation’ on Rn, we get a smaller group
that excludes reflections: SO(n).
Example: Let X=Rnwith its usual metric. The group preserving this structure is the Euclidean
group
G=E(n)
= O(n)n Rn
In other words, any f∈E(n) can be written as:
f(x) = Rx +v
for R∈O(n), v∈Rn, but
ff0(x) = R(R0x+v0) + v=RR0x+Rv0+v
with f, f 0∈E(n), instead of merely RR0x+v+v0which we would have in O(n)ƗRn.
We can turn this game around: given a group (e.g. a Lie group) Gacting on a manifold X
we can ask: what structure on Xdoes this group preserve? We have seen that the Galilei group
G(n+ 1) acts on RnƗR: it is the group generated by:
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1 Group Actions Preserving Structures

We’ve said a bit about group actions, but I haven’t explained the most important part: how any structure on a manifold gives a group action! Given a manifold X with some extra structure (for example: a Riemannian metric - a very nice distance function), you can ask: which diffeomorphisms f : X → X preserves this extra structure? Such diffeomorphisms form a group! We get lots of interesting groups, including a lot of Lie groups. Example: Take X = Rn^ and let the extra structure be the structure of the vector space. Then f : Rn^ → Rn^ preserves this extra structure iff:

  • f (0) = 0
  • f (x + y) = f (x) + f (y)
  • f (αx) = αf (x)

We say f is linear. We get a group of diffeomorphisms f : X → X preserving the vector space structure:

G = GL(n) = {f : Rn^ → Rn^ : f is linear and invertible}

Example: Let X = Rn^ but with its vector space structure and its usual metric. The group preserving this structure is

G = O(n) = {f ∈ GL(n) : ||f (x)|| = ||x||}

If we also demand that our transformations preserve an ā€˜orientation’ on Rn, we get a smaller group that excludes reflections: SO(n). Example: Let X = Rn^ with its usual metric. The group preserving this structure is the Euclidean group

G = E(n) = O(n) n Rn

In other words, any f ∈ E(n) can be written as:

f (x) = Rx + v

for R ∈ O(n), v ∈ Rn, but

f f ′(x) = R(R′x + v′) + v = RR′x + Rv′^ + v

with f, f ′^ ∈ E(n), instead of merely RR′x + v + v′^ which we would have in O(n) Ɨ Rn. We can turn this game around: given a group (e.g. a Lie group) G acting on a manifold X we can ask: what structure on X does this group preserve? We have seen that the Galilei group G(n + 1) acts on Rn^ Ɨ R: it is the group generated by:

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  • spatial translations (Rn)
  • rotations and reflections (O(n))
  • time translations (R)
  • Galilei boosts (Rn)

What structure on spacetime (Rn^ Ɨ R) is preserved precisely by this action of G(n + 1)?

  1. ā€œSimultaneous distancesā€ - i.e. distance between points (x, t) and (x′, t), namely ||x āˆ’ x′||.
  2. ā€œTime intervalsā€ - the time intervals between (x, t) and (x′, t′) is t āˆ’ t′.
  3. ā€œLinesā€ - all lines in Rn+1^ are mapped to lines. Or: it suffices to demand that the paths of free particles are mapped to paths of free particles.

When Einstein came up with special relativity, he saw that the Galiliei group is not really the correct group of symmetries of spacetime — the correct group is much simpler! The correct group preserves ā€˜spacetime distances’, or more precisely

d((x, y, z, t) āˆ’ (x′, y′, z′, t′)) =

(x āˆ’ x′)^2 + (y āˆ’ y′)^2 + (z āˆ’ z′)^2 āˆ’ c^2 (t āˆ’ t′)^2

where c is the speed of light. This group ā€˜approaches’ the Galilei group as c → āˆž.

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