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hawkdron496
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- TL;DR Summary
- I've been working through a textbook on gauge theory and can't quite put my finger on what it feels like I'm missing. I briefly run through the concepts as I understand them and then ask about specific things I'm confused about.
So, recently I've been working through "Classical Theory of Gauge Fields" by Rubakov. I've more-or-less been able to do the exercises as they've come up, but every once in a while I feel like I'm symbol pushing to get the correct answer, or ignoring certain confusions I have in favour of doing computations. I'm not entirely sure what it is that I feel like I'm missing, but I'm going to try to ask it here. Part of my confusion, I think, is that I come from a mostly math background, and physics texts use words in ways that feel slightly different from how I understand them, but seems to assume that I know what they mean by those words.
So, my understanding:
A field theory consists of a field ##\phi##, which is a map from spacetime to some vector space (##\mathbb{R}## for a scalar field, but could be any vector space). You have the lagrangian density, ##\mathcal{L}##, which eats a field (and its derivatives) and gives a function ##M \rightarrow \mathbb{R}## that can be integrated over all of spacetime to give you an action.
Now, some lagrangian densities have the property that applying a transformation ##T## to the field doesn't change the action. That is, ##\mathcal{L} (T\phi) = \mathcal{L} (\phi)##. However, we can extend this idea, and make ##T## depend on the spacetime point we're at. Then, we need to change any derivatives in the lagrangian density to covariant derivatives, which we can do by introducing a new field, ##A## with its own transformation properties (specifically, if ##T## is in a Lie group ##G##, then ##A_\mu## is in its Lie algebra and##A_\mu \mapsto TA_\mu T^{-1} + T\partial_\mu T^{-1}##).
Then, we can construct different theories by saying (for example) "consider an SU(2) gauge theory", pick a representation of SU(2) (which is a group homomorphism from ##SU(2)## to the set of linear operators on some vector space ##V##, let our field ##\phi## be a map from spacetime to ##V##, and then let ##A_\mu## be an element of the induced representation of the Lie Algebra of SU(2). Then you just pick a lagrangian that's invariant under $$\phi \mapsto T(x) \phi$$ and $$A_\mu \mapsto TA_\mu T^{-1} + T\partial_\mu T^{-1}$$ and you've got yourself an SU(2) gauge theory.
So, that's great, but there are some things that I'm not entirely clear on.
1. It would be really nice to just have had a list of definitions at the start of this book. It feels like there are a lot of examples but very few definitions. Is the broad overview I gave above more-or-less correct?
2. What exactly do we mean by "An xyz field in the abc representation of G"? When I hear the term, say, "scalar field", I think we mean "A map from spacetime to ##\mathbb{R}##". However, Rubakov will say things like "Construct all invariants of order up to and including four, for the scalar field in the adjoint representation of the group SU(2)." and then I'm confused. As I understand it, for a field to transform in the adjoint representation of ##G##, the field must take values in the Lie algebra of ##G##, and then transforms as ##g \phi g^{-1}##. Since ##SU(2)##'s Lie Algebra is 3D (if I recall correctly), how can ##\phi## take values in it and still be a scalar field?
I believe that these are the best questions I can come up with that get closest to the heart of what I feel I don't understand, but if more questions become clear to me I'll edit them into the post. Thank you in advance for the answers.
So, my understanding:
A field theory consists of a field ##\phi##, which is a map from spacetime to some vector space (##\mathbb{R}## for a scalar field, but could be any vector space). You have the lagrangian density, ##\mathcal{L}##, which eats a field (and its derivatives) and gives a function ##M \rightarrow \mathbb{R}## that can be integrated over all of spacetime to give you an action.
Now, some lagrangian densities have the property that applying a transformation ##T## to the field doesn't change the action. That is, ##\mathcal{L} (T\phi) = \mathcal{L} (\phi)##. However, we can extend this idea, and make ##T## depend on the spacetime point we're at. Then, we need to change any derivatives in the lagrangian density to covariant derivatives, which we can do by introducing a new field, ##A## with its own transformation properties (specifically, if ##T## is in a Lie group ##G##, then ##A_\mu## is in its Lie algebra and##A_\mu \mapsto TA_\mu T^{-1} + T\partial_\mu T^{-1}##).
Then, we can construct different theories by saying (for example) "consider an SU(2) gauge theory", pick a representation of SU(2) (which is a group homomorphism from ##SU(2)## to the set of linear operators on some vector space ##V##, let our field ##\phi## be a map from spacetime to ##V##, and then let ##A_\mu## be an element of the induced representation of the Lie Algebra of SU(2). Then you just pick a lagrangian that's invariant under $$\phi \mapsto T(x) \phi$$ and $$A_\mu \mapsto TA_\mu T^{-1} + T\partial_\mu T^{-1}$$ and you've got yourself an SU(2) gauge theory.
So, that's great, but there are some things that I'm not entirely clear on.
1. It would be really nice to just have had a list of definitions at the start of this book. It feels like there are a lot of examples but very few definitions. Is the broad overview I gave above more-or-less correct?
2. What exactly do we mean by "An xyz field in the abc representation of G"? When I hear the term, say, "scalar field", I think we mean "A map from spacetime to ##\mathbb{R}##". However, Rubakov will say things like "Construct all invariants of order up to and including four, for the scalar field in the adjoint representation of the group SU(2)." and then I'm confused. As I understand it, for a field to transform in the adjoint representation of ##G##, the field must take values in the Lie algebra of ##G##, and then transforms as ##g \phi g^{-1}##. Since ##SU(2)##'s Lie Algebra is 3D (if I recall correctly), how can ##\phi## take values in it and still be a scalar field?
I believe that these are the best questions I can come up with that get closest to the heart of what I feel I don't understand, but if more questions become clear to me I'll edit them into the post. Thank you in advance for the answers.