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Understanding Gauge

Published online by Cambridge University Press:  01 January 2022

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Abstract

I consider two usages of the expression “gauge theory.” On one, a gauge theory is a theory with excess structure; on the other, a gauge theory is any theory appropriately related to classical electromagnetism. I make precise one sense in which one formulation of electromagnetism, the paradigmatic gauge theory on both usages, may be understood to have excess structure and then argue that gauge theories on the second usage, including Yang-Mills theory and general relativity, do not generally have excess structure in this sense.

Type
Formal Methods
Copyright
Copyright © The Philosophy of Science Association

1. Introduction

The word “gauge” is ubiquitous in modern physics. Our best physical theories are described, in various contexts, as “gauge theories.” The “gauge argument” allegedly reveals the underlying “logic of nature” (Martin Reference Martin2002). Our theories regularly exhibit “gauge freedom,” “gauge structure,” and “gauge dependence.” Unfortunately, however, it is far from clear that the term has some univocal meaning across the many contexts in which it appears. It is a bit like “liberal” in American political discourse: it shows up everywhere, and no one knows what it means.

Here I focus on two strands of usage.Footnote 1 On the first strand, a “gauge theory” is a theory that exhibits excess structure or, in Earman’s words, “descriptive fluff” (Reference Earman2004).Footnote 2 On this way of thinking about gauge, there is a mismatch between the mathematical structure used in the theory and the structure we take the world to have, in such a way that (perhaps) one could remove some structure from the theory without affecting its descriptive or representational power. Most famously, Earman and Norton (Reference Earman and Norton1987) argue that the so-called hole argument shows that general relativity is a gauge theory in just this sense; some have taken this as motivation for moving to a different, perhaps undiscovered, formalism for representing space-time (Earman Reference Earman1989).Footnote 3 Similar considerations have motivated some views on Yang-Mills theory (Healey Reference Healey2007; Rosenstock and Weatherall Reference Rosenstock and Weatherall2015).

The second strand of usage concerns a specific class of theories. Here one uses “gauge theory” to refer to various generalizations of classical electromagnetism that share a certain mathematical structure.Footnote 4 For instance, Trautman (Reference Trautman and Held1980) defines “gauge theory” as follows: “For me, a gauge theory is any physical theory of a dynamic variable which, at the classical level, may be identified with a connection on a principal bundle” (26). This turns out to be a large class containing most of our fundamental theories, including all Yang-Mills theories, general relativity, and Newton-Cartan theory. It is in this context that physicists seem to speak most often of gauge theories, usually as a synonym for “Yang-Mills theories.”

It is easy to imagine that the two strands are closely related and, in particular, that all gauge theories in the second sense are also gauge theories in the first sense. But as I argue below, this is a mistake. In particular, I will articulate a precise sense in which electromagnetism—the paradigmatic example on both strands—may be understood to have excess structure, and thus to be a gauge theory in the first sense. I then consider whether other theories, such as Yang-Mills theory and general relativity, have excess structure in the same sense. I will argue that they do not. It follows that on at least one precise sense of what it means for a theory to have excess structure, the two strands of usage described above come apart.

2. Two Approaches to Electromagnetism

In what follows, we consider electromagnetism on the fixed background of Minkowski space-time, (M,ηab).Footnote 5 In this setting, there are two ways of characterizing models of ordinary electromagnetism.Footnote 6

On one characterization, the principal dynamical variable is the electromagnetic field, represented by a two-form Fab on space-time. The electromagnetic field is required to satisfy Maxwell’s equations, which may be expressed as [aFbc]=0 and aFab=Jb, where is the Minkowski derivative operator and Ja is a smooth vector field representing the charge-current density on space-time. A model of the theory on this characterization might be written as a triple (M,ηab,Fab), where Fab is any closed two form (i.e., any two form satisfying the first of Maxwell’s equations).Footnote 7 Call this formulation of the theory EM1.

On the second characterization, the dynamical field is the four-vector potential, represented by a one-form Aa on space-time. This field is required to satisfy a single differential equation: aaAbbaAa=Jb, where again Ja is the charge-current density. A model of the theory may again be represented by a triple, (M,ηab,Aa), where Aa is any one form.Footnote 8 I call this formulation of the theory EM2.

These two formulations are systematically related. Given any model (M,ηab,Aa) of EM2, I can always define an electromagnetic field by Fab=[aAb]. Since any Fab thus defined is exact, it must also be closed, and thus the resulting triple (M,ηab,Fab) is a model of EM1; moreover, this Fab is associated with the same charge-current density as Aa. Conversely, given any model (M,ηab,Fab) of EM1, since Fab is closed, it must also be exact, and thus there exists a one-form Aa such that Fab=[aAb].Footnote 9 The triple (M,ηab,Ab) is then a model of EM2, again with the same charge-current density.

However, there is an important asymmetry in this relationship. Given any model of EM2, there exists a unique corresponding model of EM1, because any smooth one form has a unique exterior derivative. But the converse is not true: given a model (M,ηab,Fab) of EM1, there will generally be many corresponding models of EM2, since if Aa is such that Fab=[aAb], then Aa=Aa+aχ, for any smooth scalar field χ, also satisfies Fab=[aAb]=[aAb]+[ab]χ, because for any smooth scalar field, [ab]χ=0. Transformations AaAa of this form are sometimes known as gauge transformations.

It is this asymmetry that, I claim, supports the common view that electromagnetism has excess structure. The idea is that EM1 and EM2 both have all of the resources necessary to represent classical electromagnetic phenomena. Indeed, in both cases, one may take the empirical content of electromagnetism to be fully exhausted by the electromagnetic field associated with a given model—either directly in the case of EM1 or as derived above in the case of EM2. But there are prima facie distinct models of EM2 associated with the same electromagnetic field. Thus, it would seem that these models of EM2, although they differ in their mathematical properties, should be taken to have the same representational capacities. Intuitively, then, whatever structure distinguishes models of EM2 related by gauge transformations must be irrelevant to the representational capacities of the models, at least as long as the empirical content is exhausted by the associated electromagnetic field. It is in this sense that electromagnetism—or really, EM2—has excess structure.

3. Comparing Structure

In the next section, I make the intuitive argument just given precise. First, however, I take a detour through pure mathematics. Mathematical objects often differ in how much structure they have. For instance, topological spaces have more structure than sets: a topological space (X, τ) consists in a set X, along with something more, namely, a collection τ of open subsets of X satisfying certain properties. Similarly, an inner product space has more structure than a vector space, and a Lie group has more structure than a smooth manifold. In this section, I use some basic category theory to capture these judgments as mathematical relationships between the theories.Footnote 10

To begin, recall that various mathematical theories may be associated with categories. For instance, there is a category Set, whose objects are sets and whose arrows are functions. There is a category Top, whose objects are topological spaces and whose arrows are continuous functions. There are also functors between such categories. For instance, there is a functor F:TopSet that takes every topological space (X, τ) to the set X and takes every continuous map f:(X,τ)(X,τ) to the function f:XX. Functors of this sort are often called “forgetful,” because, intuitively speaking, they take objects of one category and forget something about them: in this case, they take topological spaces (X, τ) and forget about τ.

How can one tell whether a given functor is forgetful? There is a simple but insightful theory available, due to Baez, Bartel, and Dolan (Reference Baez, Bartel and Dolan2004; see also Barrett Reference Barrett2013). It requires a few further definitions, concerning properties that a functor F:CD may have. First, we will say that F is full if for all objects A, B of C, the map (f:AB)(F(f):F(A)F(B)) induced by F is surjective. Similarly, F is faithful if for all pairs of objects in C, the induced map on arrows is injective. And F is essentially surjective if for every object X of D, there is some object A of C and arrows f:F(A)X and f1:XF(A) such that f1f=1F(A) and ff1=1X. (Such an arrow f is an isomorphism, so essentially surjective functors are surjective on objects “up to isomorphism.”)

If a functor F:CD is full, faithful, and essentially surjective, then the functor is said to realize an equivalence of categories. In such cases, F forgets nothing. Otherwise a functor is forgetful. In particular, a functor forgets (only) structure if it is faithful and essentially surjective but not full. A functor forgets (only) properties if it is full and faithful but not essentially surjective. And a functor forgets (only) stuff if it is full and essentially surjective but not faithful. In general, a given functor may be forgetful in more than one of these ways, but not in any other ways: any functor may be written as the composition of three functors that forget (no more than) structure, properties, and stuff, respectively.

The best way to make this categorization plausible is by considering examples. For instance, the functor we have already considered, F:TopSet, forgets only structure. This is because every set corresponds to some topological space (or other), which means that F is essentially surjective. Similarly, any distinct continuous functions f,f:(X,τ)(X,τ) must be distinct as functions, so F is faithful. But F is not full, because not every function f:XX is continuous, given topologies on X and X′. So in this case, the classification captures the pretheoretic intuition with which we began.

Similarly, we can define categories Grp and AbGrp, whose objects are groups and Abelian groups, respectively, and whose arrows are group homomorphisms; then, there is a functor G:AbGrpGrp that takes Abelian groups and group homomorphisms to themselves. This functor is full and faithful, since it just acts as the identity on group homomorphisms between Abelian groups. But it is not essentially surjective because not every group is Abelian. So this functor forgets only properties—namely, the property of being Abelian. And finally, we can define a functor H:Set1, where 1 is the category with one object and one arrow (the identity on the one object). This functor takes every set to the unique object of 1 and every arrow to the unique arrow of 1. It is clearly full and essentially surjective, but not faithful, so it forgets only stuff. To see how, note that we may think of 1 as the category with the empty set as its only object; thus, H forgets all of the elements of the sets.

This classification of functors gives us a criterion for when a mathematical theory T 1 may be said to have more structure than another theory T 2, namely, when there exists a functor from the category associated with T 1 to the category associated with T 2 that forgets structure. Given two categories, there may be multiple functors between them, and it may be that not all such functors forget structure, even if there exists one that does. This means that comparative judgments of “amount of structure” between theories should be understood as relative to a choice of functor. This flexibility is a virtue: it allows us to explore various ways in which theories may be related.

4. A Diagnostic Tool

I now return to the question of interest. To begin, I use the criterion just developed to make the intuitive argument at the end of section 2 precise. I define two categories, corresponding to the two formulations of electromagnetism already discussed, and then define a functor between them that captures the relationship already discussed between EM1 and EM2.

The first category, EM1, has models (M,ηab,Fab) of EM1 as objects and as arrows has maps that suitably preserve this structure. For present purposes, we take these to be isometries of Minkowski space-time that preserve the electromagnetic field, so that given two models, (M,ηab,Fab) and (M,ηab,Fab), an arrow χ:(M,ηab,Fab)(M,ηab,Fab) will be an isometry of (M,ηab) such that χ*(Fab)=Fab. Likewise, we may define a category EM2 whose objects are models (M,ηab,Aa) of EM2 and whose arrows are isometries of Minkowski space-time that preserve the four-vector potential. Given these categories, the map defined above, taking models (M,ηab,Aa) of EM2 to models (M,ηab,[aAb]) of EM1, becomes a functor F:EM2EM1 that take arrows of EM2—which, recall, are isometries of Minkowski space-time with an additional property—to the arrow of EM1 corresponding to the same isometry. (This action on arrows is well defined because, given any arrow χ:(M,ηab,Aa)(M,ηab,Aa) of EM2, [aAb]=[a(χ*(Ab]))=χ*([aAb]).)Footnote 11 We then have the following result.

Proposition 1. F forgets only structure.

Proof. F is clearly faithful and essentially surjective. To see that it is not full, consider the object A=(M,ηab,0) of EM1. The object X=(M,ηab,0) of EM2 maps to A. But now consider any nonconstant scalar field ψ. Then X=(M,ηab,aψ) is a model of EM2, and F(X)=F(X)=A. If F were full, then, there would have to be an arrow f:XX such that F(f)=1A, but this is impossible, since by construction, there are no arrows between X and X′. QED

Proposition 1 provides a precise sense in which EM2 has more structure than EM1: the functor realizing the natural relationship between the theories forgets (only) structure. Recall that the intuitive argument was that there are distinct models of EM2 corresponding to a single model of EM1, and thus there must be features of the models of EM2 that distinguish them, without making any difference to their empirical content. The present argument, meanwhile, is that there are models of EM2 that fail to be isomorphic—by the standard of isomorphism used in defining EM2—even though the corresponding models of EM1 are isomorphic or even identical. This is captured in the formalism by the fact that there are arrows in EM1, which we may interpret as “structure-preserving maps” between models of EM1, that are not structure-preserving maps between models of EM2. The structure that these maps do not preserve is the structure that, on the intuitive argument, distinguished models of EM2.

I take this to be strong evidence that the formal criterion given by forgetful functors captures the sense in which electromagnetism has excess structure. And since electromagnetism is the paradigmatic example of a gauge theory, I take this to be the sense of “excess structure” associated with the first strand of usage.Footnote 12 Of course, there may be other senses in which a theory might be thought to have excess structure, but I will not consider that question further here. Rather, I stipulate that the criterion developed here is salient and turn to a different question. Do gauge theories in the second sense—that is, the theories Trautman identifies—have excess structure?

No. First, consider electromagnetism, formulated now as a theory whose dynamical variable is a connection on a principal bundle over Minkowski space-time—that is, electromagnetism formulated as a gauge theory in Trautman’s sense. Call this theory EM3. Models of EM3 may be written (P, ωα), where P is the total space of the (unique, trivial) principal bundle U(1)PπM over Minkowski space-time and ωα is a principal connection.Footnote 13 This theory is closely related to both EM1 and EM2 as already discussed: given any (global) section σ:MP, we may define a four-vector potential Aa as the pullback along σ of ωα: Aa=σ*(ωα). Similarly, we may define an electromagnetic field tensor Fab as the pullback along σ of the curvature of the connection, defined by Ωαβ=dαωβ, where d is the exterior derivative on P: Fab=σ*(Ωαβ). Thus, Aa and Fab may be thought of as representatives on M of the connection and curvature on P. In general, Aa will depend on the choice of section σ, whereas Fab will not depend on that choice because U(1) is an Abelian group.

Given this characterization of the theory, we can define yet another category, EM3, as follows: the objects of EM3 are models of EM3, and the arrows are principal bundle isomorphisms (Ψ,ψ) that preserve both the connection on P and the metric on M: that is, pairs of diffeomorphisms Ψ:PP and ψ:MM such that ψ*(ηab)=ηab, Ψ*(ωα)=ωα, πΨ=ψπ, and Ψ(xg)=Ψ(x)g for any xP and any gU(1). Then we may define a functor F˜:EM3EM1 as follows: F˜ acts on objects as (P,ωα)(M,ηab,σ*(Ωαβ)), for any global section σ:MP, and F˜ acts on arrows as (Ψ,ψ)ψ. (Again, this action on arrows is well defined. Choose any section σ:MP. Then Ψ1σψ is also a section of P. But since Fab=σ*(Ωαβ) and Fab=σ*(Ωαβ) are independent of the choice of section, Fab=(Ψ1σψ)*(Ωαβ)=ψ*σ*Ψ1*(Ωαβ)=ψ*σ*(Ωαβ)=ψ*(Fab).)

Proposition 2. F˜ forgets nothing.

Proof. First, consider an arbitrary object (M,ηab,Fab) of EM1 and pick some Aa such that F:EM2EM1. Then given any section σ:MP and any one-form Aa, we can define a connection ωα on P by assigning to each point xσ[M] the one-form π*(Aa) and then extending this field on σ[M] to all of P by requiring it to be equivariant. It follows that F˜ is essentially surjective. Now consider any two objects (P,ωα) and (P,ωα) of EM3 and suppose there exist arrows (Ψ,ψ),(Ψ,ψ):(P,ωα)(P,ωα) such that F˜((Ψ,ψ))=ψ=ψ=F˜((Ψ,ψ)). It follows that (ΨΨ1,1M) is a vertical bundle automorphism such that (ΨΨ1)*(ωα)=ωα. But by the equivariance of ωα, this is only possible if ΨΨ1=1P. Since Ψ and Ψ1 are bijective, it follows that Ψ=Ψ. Thus, F˜ is faithful. Finally, suppose there is an arrow ψ:F˜((P,ωα))F˜((P,ωα)). Then ψ is an isometry of Minkowski space-time such that, for any section σ:MP, ψ*(σ*(dαωβ))=σ*(dαωβ). Fix σ:MP. It follows that there exists a section σ˜:MP such that σ˜*(ωα)=ψ*(σ*(ωα)). We may then define a diffeomorphism Ψ:PP as follows. For any xP, there exists some gU(1) such that x=σ˜π(x)g. This relationship determines a smooth map g:PU(1) satisfying g(xh)=g(x)h for any hU(1). We then define Ψ by xσψπ(x)g(x) for all xP. This map Ψ:PP is a diffeomorphism such that Ψ(xh)=σψπ(xh)g(xh)=σψπ(x)g(x)h=Ψ(x)h and πΨ=πσψπ=ψπ. Thus, (Ψ,ψ):PP is a principal bundle isomorphism. Moreover, since for any xσ˜[M], (Ψx)*(ωα)=(πx)*(ψπ(x))*σψπ(x)*(ωα)=(πx)*(σ˜π(x))*(ωα)=(ωα)|x, it follows by the equivariance of ωα and ωα that Ψ*(ωα)=ωα. So F˜ is full. QED

This result shows that EM3 does not have excess structure in the sense that EM2 does. To extend this to other gauge theories in the second sense, however, requires more work. The reason is that the criterion we have been using requires us to have two formulations, both of which are taken to be descriptively adequate and empirically equivalent, which we then compare. In other cases of interest, though, such as non-Abelian Yang-Mills theory or general relativity, it is not clear that we have a plausible second theory to consider.

Still, there is something one can say. It concerns the role of “gauge transformations” between models of EM2, as described at the end of section 2. These are maps that relate models of EM2 that have the same representational capacities even though they are not isomorphic. The criterion of excess structure described here, meanwhile, requires the existence of a functor between categories of models that fails to be full—or in other words, a standard of comparison between the theories relative to which one formulation has “more” arrows than the other or, alternatively, relative to which one of the formulations is “missing” arrows.Footnote 14 This suggests a rule of thumb for whether a theory, or a formulation of a theory, has excess structure in the sense described here, namely, the theory has models that are not isomorphic but that nevertheless we interpret as having precisely the same representational content. Indeed, whereas the criterion discussed above tells us when one theory or formulation has more structure than another, this second criterion evaluates whether any alternative formulation could have less structure and still do the same descriptive work—at least without equivocating between physical situations we now think are distinct.

How can we put this rule of thumb to work? Suppose you are given a theory and a collection of maps taking models to models with the same representational capacities—that is, one is presented with a candidate “gauge theory” and a class of “gauge transformations.” One may then ask: are these gauge transformations naturally construed as isomorphisms of the models of the theory, understood as mathematical objects? If the answer is yes, then it would seem that these maps do not signal excess structure, since these maps would not be “missing” from a natural category of models; conversely, if the answer is no, then there likely is excess structure in the formulation.

Applying this diagnostic to some examples of gauge theories in the second sense above, we immediately see that the moral concerning EM3 generalizes to other Yang-Mills theories. For instance, models of an arbitrary Yang-Mills theory with structure group G may be written (P,ωAα), where P is a principal G-bundle over some space-time (M, gab) and ωAα is a principal connection on P.Footnote 15 In this setting, a “gauge transformation” is often defined as a (vertical) principal bundle automorphism (Ψ,1M) relating models (P,ωAα) and (P,Ψ*(ωAα)) (see, e.g., Bleecker Reference Bleecker1981, sec. 3.2). But these maps are just a special class of connection- and metric-preserving principal bundle isomorphisms, and so although they do map between models with the same representational resources, they are not “extra” maps, in the sense of the gauge transformations of EM2. So Yang-Mills theory does not have excess structure in the sense discussed here.

Likewise, for general relativity, we characterize models of the theory as relativistic space-times, (M, gab). Here “gauge transformations” are often taken to be diffeomorphisms φ:MM relating models (M,gab) and (M,φ*(gab)) (see, e.g., Wald Reference Wald1984; Earman and Norton Reference Earman and Norton1987). But once again, these maps are just isometries (i.e., they are just isomorphisms of Lorentzian manifolds). So here, too, there is no excess structure.

5. Conclusion

I have isolated two strands of usage of the expression “gauge theory” in physics and philosophy of physics. According to one, a gauge theory is a theory that has excess structure; according to the other, a gauge theory is any theory whose dynamical variable is a connection on a principal bundle. I then endeavored to make precise the sense in which the paradigmatic example of a gauge theory (according to both strands)—classical electromagnetism—may be construed as having excess structure. From this discussion, I extracted a general criterion for when a theory has excess structure. From this criterion, I argued that gauge theories in the second sense need not have excess structure—and indeed, Yang-Mills theory and general relativity should not be construed as having excess structure in the sense that one formulation of electromagnetism does.

Footnotes

This material is based on work supported by the National Science Foundation under grant 1331126. Thank you to Thomas Barrett, Gordon Belot, Ben Feintzeig, Richard Healey, David Malament, Sarita Rosenstock, and David Wallace for helpful discussions related to the material in this article; to Thomas Barrett, Ben Feintzeig, David Malament, J. B. Manchak, and Sarita Rosenstock for comments on an earlier draft; and to my fellow symposiasts—Thomas Barrett, Hans Halvorson, and Sahotra Sarkar—for a stimulating session at the 2014 PSA biennial meeting, at which this work was presented.

1. There are still others—see, e.g., Weyl (Reference Weyl1952). But I will not attempt a taxonomy.

2. This way of speaking is common: see Ismael and van Fraassen (Reference Ismael, van Fraassen, Brading and Castellani2003), Redhead (Reference Redhead, Brading and Castellani2003), Rovelli (Reference Rovelli2014), and many others.

3. For an argument against this way of thinking about relativity theory, see Weatherall (Reference Weatherall2016b). For more on the relationship between the standard formalism of relativity theory and at least one widely discussed alternative, see Rosenstock, Barrett, and Weatherall (Reference Rosenstock, Barrett and Weatherall2015).

4. Although I will say somewhat more about principal bundles and principal connections below, this will not be the occasion to review this formalism. For more on this topic, see Bleecker (Reference Bleecker1981), Palais (Reference Palais1981), and Weatherall (Reference Weatherall2016a).

5. Minkowski space-time is a relativistic space-time where M is ℝ4 and ηab is flat and complete. We focus on this case for convenience; little of consequence turns on the limitation. Note that we work in the abstract index notation, following the sign conventions of Malament (Reference Malament2012).

6. These two ways of thinking about electromagnetism are described in somewhat more detail in Weatherall (Reference Weatherall2015). Of course, there are other ways of characterizing the models of electromagnetism—including using the principal bundle formalism discussed below.

7. One might also stipulate a source term, Jb, along with the model or perhaps limit attention to models for which the source term satisfies certain “physically reasonable” conditions. Here it suffices to permit arbitrary sources and to “read off” the charge-current density from the divergence of Fab, using the second of Maxwell’s equations.

8. The same remarks apply here as in n. 7.

9. This result holds globally because M is homeomorphic to ℝ4. In the case of more general space-times, one would have to work locally; this difference raises interesting issues, but they are not relevant to the current discussion.

10. For background on basic category theory, see Mac Lane (Reference Mac Lane1998) or Leinster (Reference Leinster2014); because of space constraints, I take notions like “category” and “functor” for granted.

11. See Weatherall (Reference Weatherall2015) for further details on this functor.

12. There are other examples of theories with excess structure in this sense, too—e.g., Newtonian gravitation, which is also sometimes described as a gauge theory (Malament Reference Malament2012, 248), may be understood to have excess structure in just this sense. To see this, consider the discussion in Weatherall (Reference Weatherall2015, sec. 6) and observe that the functor from NG1 to GNG given by the Trautman geometrization theorem is faithful and essentially surjective but not full.

13. Again, see Bleecker (Reference Bleecker1981), Palais (Reference Palais1981), or Weatherall (Reference Weatherall2016a) for more details on this theory.

14. This way of speaking may be made somewhat more precise, by showing how adding arrows corresponding to gauge transformations to EM2 can lead to a new category that is equivalent to EM1. See Weatherall (Reference Weatherall2015).

15. Again, for more on the notation used here, see Weatherall (Reference Weatherall2016a).

References

Baez, John, Bartel, Toby, and Dolan, Jim. 2004. “Property, Structure, and Stuff.” Quantum Gravity Seminar, University of California, Riverside. http://math.ucr.edu/home/baez/qg-spring2004/discussion.html.Google Scholar
Barrett, Thomas. 2013. “How to Count Structure.” Philosophy of Physics Workshop, Carnegie Mellon University, September.Google Scholar
Bleecker, David. 1981. Gauge Theory and Variational Principles. Reading, MA: Addison-Wesley. Repr., Dover 2005.Google Scholar
Earman, John. 1989. World Enough and Space-Time. Cambridge, MA: MIT Press.Google Scholar
Earman, John 2004. “Laws, Symmetry, and Symmetry Breaking: Invariance, Conservation Principles, and Objectivity.” Philosophy of Science 71 (5): 1227–41.CrossRefGoogle Scholar
Earman, John, and Norton, John. 1987. “What Price Spacetime Substantivalism? The Hole Story.” British Journal for the Philosophy of Science 38 (4): 515–25.CrossRefGoogle Scholar
Healey, Richard. 2007. Gauging What’s Real: The Conceptual Foundations of Contemporary Gauge Theories. New York: Oxford University Press.CrossRefGoogle Scholar
Ismael, Jenann, and van Fraassen, Bas. 2003. “Symmetry as a Guide to Superfluous Structure.” In Symmetries in Physics: Philosophical Reflections, ed. Brading, Katherine and Castellani, Elena, 371–92. Cambridge: Cambridge University Press.Google Scholar
Leinster, Tom. 2014. Basic Category Theory. Cambridge: Cambridge University Press.CrossRefGoogle Scholar
Mac Lane, Saunders. 1998. Categories for the Working Mathematician. 2nd ed. New York: Springer.Google Scholar
Malament, David. 2012. Topics in the Foundations of General Relativity and Newtonian Gravitation Theory. Chicago: University of Chicago Press.CrossRefGoogle Scholar
Martin, Christopher A. 2002. “Gauge Principles, Gauge Arguments, and the Logic of Nature.” Philosophy of Science 69 (Proceedings): S221S234.CrossRefGoogle Scholar
Palais, Richard S. 1981. The Geometrization of Physics. Hsinchu: Institute of Mathematics, National Tsing Hua University.Google Scholar
Redhead, Michael. 2003. “The Interpretation of Gauge Symmetry.” In Symmetries in Physics: Philosophical Reflections, ed. Brading, Katherine and Castellani, Elena, 124–39. Cambridge: Cambridge University Press.Google Scholar
Rosenstock, Sarita, Barrett, Thomas, and Weatherall, James Owen. 2015. “On Einstein Algebras and Relativistic Spacetimes.” Studies in History and Philosophy of Modern Physics B 52:309–16.CrossRefGoogle Scholar
Rosenstock, Sarita, and Weatherall, James Owen. 2015. “A Categorical Equivalence between Generalized Holonomy Maps on a Connected Manifold and Principal Connections on Bundles over That Manifold.” Unpublished manuscript, arXiv. http://arxiv.org/abs/1504.02401.Google Scholar
Rovelli, Carlo. 2013. “Why Gauge?Foundation of Physics 44 (1): 91104.CrossRefGoogle Scholar
Trautman, Andrzej. 1980. “Fiber Bundles, Gauge Fields, and Gravitation.” In General Relativity and Gravitation, ed. Held, A., 287308. New York: Plenum.Google Scholar
Wald, Robert. 1984. General Relativity. Chicago: University of Chicago Press.CrossRefGoogle Scholar
Weatherall, James Owen. 2015. “Are Newtonian Gravitation and Geometrized Newtonian Gravitation Theoretically Equivalent?” Erkenntnis, forthcoming. doi:10.1007/s10670-015-9783-5.CrossRefGoogle Scholar
Weatherall, James Owen 2016a. “Fiber Bundles, Yang-Mills Theory, and General Relativity.” Synthese 193 (8): 23892424.CrossRefGoogle Scholar
Weatherall, James Owen 2016b. “Regarding the ‘Hole Argument.’” British Journal for Philosophy of Science, forthcoming. doi:10.1093/bjps/axw012.CrossRefGoogle Scholar
Weyl, Hermann. 1952. Space-Time-Matter. Mineola, NY: Dover.Google Scholar

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