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Does the general topology of Minkowski space-time change under a Lorentz transformation? Open balls in $\mathbb{R}^{4}$ (with the standard topology) are not invariant under Lorentz transformations. Does this mean for example that observers in one reference frame would have different notions of convergence, continuity etc?

Note: I'm asking from the perspective of a curious undergraduate who just finished introductory analysis and modern physics. Please answer appropriately.

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No, because a Lorentz transformation is continuous with a continuous inverse. While an open ball is not mapped to itself, it is mapped to some other open set, in an invertible way. (That a Lorentz transformation is continuous of course follows from that it is linear.)

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    $\begingroup$ Thanks! So I could phrase it this way: Lorentz transformations are homeomorphisms, so even though they open sets not invariant, all topological notions are still preserved? $\endgroup$ Commented Jun 10, 2014 at 20:27
  • $\begingroup$ Yes, that is correct. $\endgroup$ Commented Jun 10, 2014 at 21:46
  • $\begingroup$ @RobinEkman My answer is not meant to be a criticism of yours, it's just that in my experience the fact that linear is not needfully continuous in an infinite dimensional vector space comes as a bit of a surprise to some people, so I wanted to make sure that the OP understands this for when he looks at QM more deeply. $\endgroup$ Commented Jul 1, 2014 at 10:20
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This is simply a short addendum to Robin Ekman's answer and response to your comment

So I could phrase it this way: Lorentz transformations are homeomorphisms, so even though they open sets not invariant, all topological notions are still preserved?

Homeomorphism is indeed the key concept here, and I wish to add a very slight nitpick with Robin's answer so that there is no risk of your being confused in contexts other than SR/GR (for example, in quantum mechanics): you also need the information that Minkowski spacetime is finite dimensional to infer continuity from linearity and homeomorphism from linear and invertible (which of course is a given in Minkowski spacetime). In infinite dimensions, not all linear maps are continuous: witness the Dirac delta on $\mathcal{L}^2(\mathbb{R})$ for example. The difference between the concepts of general linear and the strictly more specialised "linear continuous" in, say the standard, countably infinite dimensional Hilbert space $\mathcal{L}^2(\mathbb{R})$ is actually the very reason for being of distributions and the framework of rigged Hilbert space for talking about them; see my answer here for more information.

As I said, none of this is any worry in classical relativity. Linear and linear continous are the same notions in this field.

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