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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
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Weāve said a bit about group actions, but I havenāt 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 ā 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^ ā Rn^ preserves this extra structure iff:
We say f is linear. We get a group of diffeomorphisms f : X ā X preserving the vector space structure:
G = GL(n) = {f : Rn^ ā 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 ā GL(n) : ||f (x)|| = ||x||}
If we also demand that our transformations preserve an āorientationā 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 ā E(n) can be written as:
f (x) = Rx + v
for R ā O(n), v ā Rn, but
f f ā²(x) = R(Rā²x + vā²) + v = RRā²x + Rvā²^ + v
with f, f ā²^ ā E(n), instead of merely RRā²x + v + vā²^ which we would have in O(n) Ć 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^ Ć R: it is the group generated by:
What structure on spacetime (Rn^ Ć R) is preserved precisely by this action of G(n + 1)?
When Einstein came up with special relativity, he saw that the Galiliei group is not really the correct group of symmetries of spacetime ā the correct group is much simpler! The correct group preserves āspacetime distancesā, or more precisely
d((x, y, z, t) ā (xā², yā², zā², tā²)) =
(x ā xā²)^2 + (y ā yā²)^2 + (z ā zā²)^2 ā c^2 (t ā tā²)^2
where c is the speed of light. This group āapproachesā the Galilei group as c ā ā.