Patching DFT, T-duality and Gerbes

We clarify the role of the dual coordinates as described from the perspectives of the Buscher T-duality rules and Double Field Theory. We show that the T-duality angular dual coordinates cannot be identified with Double Field Theory dual coordinates in any of the proposals that have been made in the literature for patching the doubled spaces. In particular, we show with explicit examples that the T-duality angular dual coordinates can have non-trivial transition functions over a spacetime and that their identification with the Double Field Theory dual coordinates is in conflict with proposals in which the latter remain inert under the patching of the B-field. We then demonstrate that the Double Field Theory coordinates can be identified with some C-space coordinates and that the T-dual spaces of a spacetime are subspaces of the gerbe in C-space. The construction provides a description of both the local $O(d,d)$ symmetry and the T-dual spaces of spacetime.


Introduction
One of the requirements for the consistent formulation of double and exceptional field theories is a description of the patching conditions of doubled and exceptional spaces that underpin these theories. Let us for simplicity focus on doubled spaces as many more results for these are known. Doubled spaces arise by adding to the spacetime coordinates x a set of dual coordinatesx. In double field theory (DFT), the new coordinates are as many as those of the spacetime.
The question that arises is how these new coordinates patch. There are two main approaches in the literature for this. In the first approach, it is proposed that the dual coordinatesx patching transformations depend on the transition functions of the B-field. There are various suggestions for such dependence. Two such suggestions can be found in [1] and [2].
Another approach, advocated in [3], asserts that the patching conditions of the dual coordinatesx can be arranged such that they do not depend on the transition functions of the B-field. In such a case, the doubled space of any string background spacetime M is either a product space M × Q, where Q can be chosen as R n or T n , or the cotangent bundle T * M. The dual coordinates in this case become forgetful, in the sense that they are inert under B-field gauge transformations.
In addition, a recent proposal for DFT for some coset spaces was made in [4], following on from an analysis of DFT for Wess-Zumino-Witten models presented in [5,6].
One of the difficulties in deciding the way that the dual coordinates should patch is the uncertainty of which criteria one should apply. A selection of such criteria is as follows: • The doubled spaces patch in such a way that is consistent with the dual spaces obtained via the Buscher T-duality rules.
• The patching of double spaces is such that it requires for consistency the Dirac quantisation property of the 3-form flux.
• The doubled spaces satisfy the topological geometrisation condition.
• Doubled spaces can be constructed for all backgrounds with 3-form flux.
• Generalised geometry emerges naturally on doubled spaces.
The first criterion is perhaps the most conservative one. Whatever the patching of doubled spaces is, it should reproduce both locally and globally the results that arise after applying the Buscher T-duality rules. After all these produce the only explicit examples we know. Locally this is indeed the case through the use of O(d, d) duality transformations [7,8,9] on the fields. However, we shall see that globally the patching conditions of the doubled spaces do not reproduce the results obtained from Buscher rules.
Moreover, it is worth mentioning that DFT has raised the expectations of what can be described. As the transformations of DFT make no mention of isometries that are instrumental in the Buscher rules, there is some expectation that the doubled spaces can be used to describe a dual space which arises after dualising all spacetime directions. Another aspect of the dualisation of the whole spacetime is the idea of geometrisation, i.e. the notion that the theory which includes the spacetime metric and the 3-form field strength can be described in terms of metric data only. This is analogous to Kaluza-Klein theory which provides a geometrisation for a 2-form field strength.
The second criterion is an extrapolation of a similar result that arises in Kaluza-Klein theory. The construction of the Kaluza-Klein space is achieved after restricting the 2-form field strength to represent the first Chern class of a line bundle. In turn the flux of the 2-form is required to obey the Dirac quantisation condition.
The third criterion is also posed in analogy with the Kaluza-Klein theory. It states that the pull-back of the 3-form field strength on whatever a consistent description of doubled space is, or a generalisation of it, must represent the trivial cohomology class [11]. This has several consequences such as, for example, that the dual coordinates must have a non-trivial topology and non-trivial transition functions over the spacetime.
The fourth criterion is a natural one from the point of view of DFT. In all proposals made in the literature for the theory, there is no restriction mentioned on the backgrounds.
The fifth criterion is introduced because in generalised geometry the T-duality group O(d, d) arises naturally as the (sub)group of automorphisms of a vector bundle. So the expectation is that in a consistent formulation of the doubled space this bundle should arise naturally. In fact it is expected to be related to, if not identified with, its tangent bundle.
There are several proposals in the literature on how the doubled spaces might patch and some analysis of how they measure against the criteria mentioned above. In particular, the patching of doubled spaces under the transformations proposed in [1] has been investigated in [10] where it was shown that consistency on 4-overlaps requires that the 3-form field strength H must be exact. To resolve the patching issue, C-spaces, essentially local descriptions of gerbes, have been proposed in [11]. They exhibit consistent patching with a cohomologically non-trivial H and locally contain the doubled spaces, but generically they have more coordinates than doubled spaces. Indeed, in the case of non-trivial H-fields they do not have well-defined global dimensionalities.
More recently, two new proposals for patching doubled spaces have been put forward [2], [3]. In this paper, we shall consider these two proposals and investigate them in the light of the criteria mentioned above. First we shall clarify some aspects of the patching conditions proposed in [2] and demonstrate that, up to an allowed redefinition of the dual coordinates and choice of transition functions for B at double overlaps, the patching conditions of the dual coordinates do not depend on the transition functions of the Bfield. As a result, for these choices, the dual coordinates of the doubled space remain inert under patching which in turn implies that this proposal is related to that of [3].
The proposal made in [3] states that the dual coordinates of a doubled space remain inert under patching and the transformations induced by the form part of a generalised vector acting infinitesimally with a generalised Lie derivative on the fields are not coordinate transformations but rather gauge transformations of the B-field. As a result the dual coordinates can be forgetful and the spacetime geometry is described by a generalised geometry structure and a splitting of the generalised geometry bundle induced by the B field interpreted as a gerbe connection.
In the proposal of [4] for DFT on group manifolds, the doubled space is a group manifold with the physical space embedded into it as a Lagrangian type of submanifold, after the strong section condition is imposed, while the T-dual space corresponds to a different embedding. In this case both the physical and dual coordinates are non-trivially patched.
In what follows we give a detailed analysis of the T-duality pair of S 3 with N units of H-charge and the lens space L 3 N = S 3 /Z N with 1 unit of H charge. We show that the dual circle twists topologically non-trivially over the spacetime L 3 N and therefore that either DFT dual coordinates cannot be identified 1 with the T-duality angular coordinates, or that the doubled spaces patching proposed in [2] and [3] is not consistent globally with the T-duality rules. We also generalise this to other T-dual pairs including an example of T-dual spaces constructed from the 3-torus with H-flux background.
Note that a conflict between T-duality and the strong section condition in doubled spaces had been pointed out before from a different perspective in [12,13]. There a resolution was proposed by allowing additional transformations which preserve the split signature metric on the doubled space but do not satisfy the strong section condition.
We then go on to propose a scenario based on C-spaces and the Hitchin-Chatterjee definition of a gerbe in which both the local O(d, d) symmetry and the Buscher T-dual spaces can be consistently described. We propose an identification of the DFT coordinatẽ x of [3], which transforms as a 1-form, with a coordinate that arises in the C-space construction [11]. We then demonstrate how the T-dual spaceM of a spacetime M with H-flux and which is a circle fibration can be identified as a subspace of the total space of the gerbe associated to H on M. We also provide explicit examples of this which include the description of the T-dual lens space L 3 N = S 3 /Z N of S 3 with N units of H-charge as a subspace of the total space of a gerbe on S 3 . The latter can be described as the union of S 3 with a circle bundle with first Chern class N over an open neighbourhood of the equatorial S 2 of S 3 . The L 3 N subspace of the gerbe is the restriction of this circle bundle over the equatorial S 2 of S 3 . We also give a similar construction for a T-dual space associated 3-torus background with H-flux. As the angular coordinates that arise naturally in the gerbe construction, and which are required for the identification of the T-dual spaces of spacetime as subspaces of gerbes, are not included in doubled spaces and therefore not in DFT, we conclude that, for the consistent description of a theory with manifest Buscher T-duality symmetry, additional coordinates are required in addition to those of doubled spaces.
The paper is organised as follows: in section 2, we give the necessary and sufficient conditions for the T-dual circle to (topologically) twist over a spacetime in a manner consistent with the Buscher rules. We also prove that the dual circle of the lens space L 3 N , viewed as a circle fibration over S 2 , and that of T 3 with H-flux, topologically twist over the spacetime. In section 3, we review the proposals for patching DFT that have appeared in the literature and in section 4 we investigate them from a patching point of view concluding that they do not describe the topological twist of the dual circles. In section 5, we explore the relation between doubled spaces and C-spaces, explain how local O(d, d) symmetry arises, and present a gerbe construction for all spacetimes which are circle fibrations and have some H-flux which allows for the identification of the T-dual space as a subspace of the gerbe. We also present explicit examples based on S 3 and T 3 with H-flux backgrounds. In section 6, we present our conclusions.

T-duality rules
To describe the Buscher T-duality rules one assumes that the spacetime M admits an S 1 group action generated by a vector field X which leaves the common sector fields, the metric g, 3-form field strength H and dilaton Φ, invariant. Adapting coordinates along X = ∂ ∂θ , the metric and 2-form gauge potential can be written as After performing a T-duality transformation, the dual metric, 2-form gauge potential and dilaton read where a new angular coordinateθ has now been introduced. This is referred as the Tdual coordinate of θ and the associated circle as the dual circle, which we denoteS 1 . The coordinates of (x i ,θ) are those of a new spacetimeM which, apart from having different geometry, can also have different topology to that of M. FurthermoreM again admits aS 1 action given by translations inθ. Another significant issue, which will be of central focus in what follows, is that the T-dual coordinateθ can have non-trivial patching conditions over the original spacetime M (or vice versa). These are given by some of the transition functions of the B-field. As can be seen from (2.1), p i will transform under a B-field transformation and this will induce a transformation ofθ in (2.2) in order for the T-dual metric to remain invariant. The original spacetime M together with its dualM can be put together to construct an enhanced space. To see this observe that the space of orbits of the S 1 action on M and of theS 1 action onM are the same, M/S 1 =M /S 1 = Q. To avoid complications with fixed points, let us assume from now on that the action of S 1 on both spaces is free 2 . In such a case, one can construct a torus bundle P (Q, T 2 ) over Q. The torus bundles are classified by elements in H 2 (Q, Z) ⊕ H 2 (Q, Z) which are the first Chern classes of M and M viewed as circle bundles over Q. In [15], P (Q, T 2 ) is referred to as the correspondence space. In particular, the first Chern classes are represented by the 2-forms 1 2π dq and 1 2π dp, respectively, with p = p i dx i and similarly for q.
We therefore have the diagram We can also define two-forms F andF on Q by integratingH overS 1 and H over S 1 respectively. Here, from the T-duality rules, Equations (2.4) and (2.5), together with the fact that both M andM have the same quotient Q as circle bundles, were specified as the required conditions for the two spaces to be T-dual in [16].

The T-dual circle topologically twists over the spacetime
Although the T-dual coordinatesθ have non-trivial transition functions over Q, it does not necessarily mean that they are (topologically) twisted over the spacetime M. To settle this question, let us examine an example in detail. This is the well-known T-dual pair of S 3 with N-units of H flux and the 3-dimensional lens space L 3 N with 1-unit of H charge. It is useful to note that L 3 N is the space of orbits of Z N on S 3 where the generator g = exp 2πi/N of Z N acts as v r → gv r , where v r are complex numbers such that v 1v1 + v 2v2 = 1.
Both spaces S 3 and L 3 N are circle fibrations over S 2 , Q = S 2 . Moreover the first Chern class of these fibrations is c 1 (S 3 ) = u and c 1 (L 3 N ) = Nu, respectively, where u is the generator of H 2 (S 2 , Z). Furthermore the cohomology groups of S 3 and L 3 N are Next consider the T 2 fibration P = P (T 2 , S 2 ) with first Chern classes c 1 (P ) = u and c 1 (P ) = Nu. In fact P = S 1 × S 3 /Z N , where now the generator g of Z N acts as (a, v r ) → (ga, gv r ) and |a| = 1, a ∈ C. It turns out that the cohomology of P can be computed and can be found that In particular observe that the middle cohomology of P vanishes.
To continue observe that P can be viewed as a circle fibration over either S 3 or L 3 N . Consider first P as a circle fibration over S 3 . This fibration is obtained after considering the group action [a, v r ] → [az, zv r ], where z ∈ S 1 ⊂ C, |z| = 1 is the group element and [a, v r ] denotes the orbit of Z N represented by (a, v r ). In fact notice that S 1 /Z N = S 1 acts freely. As H 2 (S 3 , Z) = 0, all circle bundles over S 3 are topologically trivial. As a result P is a topological product S 1 × S 3 . One therefore concludes that the dual coordinateθ does not twist over the spacetime S 3 .
However the T-dual Lens space L 3 N can also be considered as the spacetime, and so S 3 can be thought as its T-dual. Note that H 2 (L 3 N , Z) = Z N and so L 3 N admits topologically non-trivial circle bundles. The fibration of P over L 3 N is constructed by considering the circle action [a, v r ] → [az, v r ]. If P was a trivial topological product S 1 ×L 3 N , the Künneth formula for computing the cohomology of the topological product of two spaces would have implied that This is a contradiction as the second cohomology of P vanishes (2.7). Therefore P is a topologically twisted product of S 1 and L 3 N . As a result, the dual θ coordinate has non-trivial patching conditions over the spacetime L 3 N . Incidentally, observe that P satisfies a partial version of the topological geometrisation condition of [11]. Both the S 3 backgrounds and its dual L 3 N have non-trivial H fluxes. As a result, the T-duality operation does not geometrise all of the B-flux, so that one does not expect that the pull back of H orH on P will represent the trivial class in H 3 (P, Z). Instead the topological geometrisation condition manifests itself as follows: pulling back H andH onto P , one may have expected that these represent two independent cohomology classes in H 3 (P, Z), but this is not the case. H 3 (P, Z) has one generator and the linear combination NH−H represents the trivial class in H 3 (P, Z), where we have suppressed the pull-back operations. This is because part of the information of the transitions functions of H andH is stored in the patching conditions of P .
The example we have given above can be generalised to include T n actions and thus T-duality in more than one direction. However, for the purpose of this paper, the example we have investigated will suffice.
To conclude, the Buscher T-duality rules allow for the possibility that the dual circle has a non-trivial topological twist over the spacetime, so that the dual angular coordinates can have non-trivial patching conditions over the spacetime. As we have seen, this situation does indeed arise in explicit examples.

A patching approach to T-duality
To give a bit more insight into the construction of circle bundle over a space and its relation to the T-dual pairs, let us first describe how the third cohomology group of the spacetime is constructed from the cohomology of S 1 and that of Q. 3 Assuming again that S 1 acts freely on the spacetime M and that Q is simply connected, one can use the method of spectral sequences to determine H 3 (M, Z) from H 1 (S 1 , Z), H 2 (Q, Z) and H 3 (Q, Z). The construction is rather intuitive. The elements of H 3 (M, Z) either are generated by au, where a is the generator of in H 1 (S 1 , Z) and u are generators of H 2 (Q), or they are pulled-back from elements in H 3 (Q, Z) with the projection map. This is precisely the case if H 4 (Q, Z) = 0. If on the other hand H 4 (Q, Z) = 0, then only some of classes generated by au may represent elements in H 3 (M, Z). In either case, the 3-form field strength H in cohomology can be written as [H] = aw + v, where w ∈ H 2 (Q, Z) and v ∈ H 3 (Q, Z), and where the pull-back operation on v has been suppressed.
It is clear from the T-duality rules stated in (2.1) and (2.2) that the component of H that take an active part in the T-duality transformations is represented by aw. Assuming that w ∈ H 2 (Q, Z), the dual spaceM as a circle bundle has first Chern class w. For later applications, let us assume that w is represented by a 2-formF 2 . The construction ofM can be made using a good cover {U α } α∈I on Q. Then, using the Poincaré lemma on U α , and on double and triple overlaps, where C is the 1-form gauge potential, a 0 are the transition functions on double overlaps and n are constants. The latter lie in 2πZ as 1 2π ω 2 represents a class in H 2 (Q, Z). Theñ M is constructed by introducing an angular coordinateθ and after imposing the patching conditionsθ These patching conditions are consistent on triple overlaps as n αβγ ∈ 2πZ. Making use of the above, we can state the criterion for whether the dual angular coordinate has non-trivial transition functions over the spacetime. Indeed, writing [H] = aw + v and [H] = aw +ṽ, we observe that the dual angular coordinateθ has non-trivial transition functions over the spacetime iff w represents a non-trivial class in H 2 (M, Z), where the pull-back operation from H * (Q, Z) to H * (M, Z) has been suppressed. Similarly, the angular coordinate θ has non-trivial transition functions over the dual spaceM iffw represents a non-trivial class in H 2 (M , Z). The classes w andw are represented by the formsF and F in (2.5) respectively.

T-duality on T 3 with flux
We can use the results of the previous section to demonstrate that the T-dual angular coordinate of T 3 with flux also is twisted over the spacetime. For this denote the angular coordinates of T 3 with (ψ 1 , ψ 2 , ψ 3 ), 0 ≤ ψ i < 2π, i = 1, 2, 3. The metric and flux are given as 11) where N ∈ Z. If we choose as a T-duality direction ψ 1 and solve for the gauge potential as B = N 4π 2 ψ 2 dψ 1 ∧ dψ 3 , then where the Killing vector field along the T-duality has been normalised as 2π∂ ψ 1 . As it has been explained in the previous section, the dual coordinate topologically twists over the spacetime iff the pull-back of dp represents a non-trivial cohomology class. Indeed and its pull-back on T 3 is a non-trivial class as 1 2π dψ 2 ∧ dψ 3 represents one of the three generators of H 2 (T 3 , Z).

Double Field Theory Finite Transformations
There has been extensive work in the literature to determine the allowed finite transformations of DFT. A concise description of all possibilities and the sources can be found in [3]. Here after imposing the strong section condition, we shall briefly summarise the finite transformations proposed as well as their induced action on the B-field. This will suffice for the purpose of the analysis that follows below.
First let us begin with the proposal of [1]. In this proposal, the doubled space coordinates (x i ,x i ) transform as and the induced transformation on the B field is Observe that the spacetime coordinates transform with the usual diffeomorphisms while the dual coordinates transform with a shift whose parameter depends only on the spacetime coordinates. A modification of this proposal in the context of DFT was suggested in [14]; however, the transformations given in [14] reduce to the above after the strong section condition has been imposed. Another proposal for the finite transformation of DFT was put forward in [2]. For this, a closed 2-form was introduced b, db = 0 which transforms as while B := B − b is taken to transform tensorially: This implies that the B-field transforms as i.e. in the same way as b. In these equations v depends only on the spacetime coordinates. The doubled space coordinate transformations are taken to be More recently a new proposal has been put forward [3]. The doubled space coordinates transform as i.e. the spacetime coordinates transform with diffeomorphisms while the dual coordinates remain inert with respect to B-field gauge transformations.
The B-field transforms as i.e. in the same way as in [2]. The reason that the dual coordinatesx do not transform under the B-field gauge transformations is because the componentṽ j of the generalised infinitesimal vector, that enters in the generalised Lie derivative acting on the fields, is identified as the parameter of an infinitesimal gauge transformation of the B field viewed as a gerbe connection. In other wordsṽ j is viewed as (the parameter of) a gauge transformation rather than as a coordinate transformation. Moreover the gerbe connection introduces a splitting in the short exact sequence which describes the extension of T M by T * M. This allows E to be split as E = T M ⊕T * M and to thereby identify the sections of T M and T * M in E which now transform as vectors and forms. The calculation of how this can be done has been described explicitly in [3] and amounts to going from W generalised tensors toŴ ones in the notation of [3]. This is related to the notion of the B-transform in generalised geometry [18,19]. As the dual coordinates of the doubled spacex do not transform, or just transform as 1-forms, they are inert under B-field gauge transformations. It has been argued in [3] that to describe DFT it is sufficient to consider the diffeomorphisms of the spacetime together with the generalised geometry structure described above which includes a splitting of the exact sequence that determines the B field.

Patching
Let us now turn to investigate the implications of patching doubled spaces with the transformations proposed in the previous section on the topology and geometry of spacetime.
Before we do this, let us describe a few properties of the de Rham-Čech theory as applied to closed 3-forms H. Let {U α } α∈I a good cover, then on the open sets U α and the n-fold overlaps U α 0 ...α n−1 = U α 0 ∩ · · · ∩ U α n−1 , n = 2, 3, 4, one has respectively, where n αβγδ are constants. The last condition arises from the requirement that on 4-fold overlaps If n αβγδ ∈ 2πZ, then H represents a class in H 3 (M, Z). The left-hand sides of all but the first of equations (4.1) involve theČech differential δ. It acts on form-valued fields defined on p-fold overlaps and takes them to forms on (p + 1)-fold overlaps, e.g. (δB) αβ = −B α + B β ; (δa) αβγ = a αβ + a βγ + a γα , and so on, and squares to zero, δ 2 = 0. We emphasise that the 2-form gauge potential B as well as the transition functions a 1 , a 0 are not unique in the above decomposition. In fact the decomposition is invariant under the local "gauge" transformations where u 1 are 1-forms and f 0 are functions defined on the indicated overlaps.

B-dependent patching for dual coordinates
If the coordinates for the doubled space,x, are taken to be one-forms patched together using the B-field transformations, i.e. −x α +x β ∝ a 1 αβ , (4.4) as in [1] and [14] (where the notation ζ αβ was used for a 1 αβ ), then, as shown in [10], this implies that the H-flux is trivial. It follows from (4.4) that (δa 1 ) αβγ = 0 which can be solved by a 1 αβ = (δu 1 ) αβ by the δ-Poincaré lemma. This in turn implies that B α can be shifted by (du 1 ) α on each patch so that the new B-field will be globally defined. So this construction of doubled spaces is not compatible with backgrounds with non-trivial H-flux in H 3 (M, Z). There are many examples of such backgrounds, for example those discussed in section 2.
Another patching proposal is that of [2] where it is asserted that the polarisation b, with db = 0, is defined on each patch U α of a good cover {U α } α∈I and patches as 4 As B transforms in the same way, the difference B = B − b transforms tensorially and one has H = dB = dB, as db = 0, and so H is exact.
One can reach the same conclusion by viewing the (3.5) as a patching condition on a good cover as Since b is closed, one can solve this locally as b α = du α and re-arrange the above equation using (4.5) as However, as we have already mentioned the definition of B is ambiguous up to a gauge transformation generated by u. As a result B can be chosen to be a globally defined 2-form leading to an exact H. This result is independent from the way that the dual coordinates transform and so it is not affected by the gauge transformation introduced in [17]. An alternative reading of the proposal made in [2], which is more tuned to the examples described later in that paper, is as follows. One introduces two different 2-form gauge potentials B and B for the 3-form field strength H, but where now B is no longer necessarily tensorial. If the transition functions with respect to B and B are denoted by a 1 and a 0 , and a 1 and a 0 in theČech-de Rham decomposition, respectively, we take the patching conditions of the dual coordinatesx to be those of the polarisation b = B − B. These are given by a 1 αβ − a 1 αβ :=â 1 αβ . So one can set −x α +x β =â 1 αβ . (4.8) on each U αβ . This is similar to (4.4) and implies thatâ 1 αβ = (δu 1 ) αβ . So if we redefine b by b α → b α − u 1 α on each patch b will be globally defined, while if we also redefine the new coordinates in a similar fashion,x α →x ′ α =x a − u 1 α the new coordinates will be inert under b (or B)-field gauge transformations. This is similar to the first case discussed above, but now does not require that the flux of H be trivial. So this interpretation leads to a patching condition which is equivalent to one which is independent of the B-field patching.

B-independent patching for dual coordinates
Such a proposal is that described in [3]. The patching conditions are just the diffeomorphisms of the spacetime and the patching conditions of the generalised geometry bundle E together with a choice of a splitting. The main point is that the patching conditions of the dual coordinates arex α =x β (4.9) i.e. they remain inert. As the generalised geometry data are by construction globally defined, the patching of such a doubled space is consistent.
However, this proposal and in particular the assertion thatx α =x β is in conflict with the patching results that are a consequences of the Buscher T-duality rules. As we have demonstrated with an explicit calculation in section 2, a T-dual circle can topologically twist over the spacetime. As this cannot happen to the DFT dual coordinates, one can only conclude that according to this proposal DFT either does not incorporate the Buscher T-duality rules or the DFT dual coordinatesx should not be identified with the Buscher dual angular coordinatesθ. If the former is not considered desirable, then one must conclude that the DFT dual coordinatesx is not the full story and additional coordinates must be introduced. There has been such a suggestion before in [11] where the basis of generalisedŴ generalised tensors has been identified and where it was shown how the generalised geometry emerges. If this case, one might argue that the motivation for the introduction of the DFT dual coordinates in the first place is somewhat weakened, or that they have only an auxiliary status.
To enforce the idea that a generalised geometry approach is not sufficient to describe the T-duality rules, observe that, although the generalised geometry bundle E is twisted over the spacetime, as a space it is contractible to the spacetime M. In other words the spacetime is fixed and the bundle transformations, which one might wish to identify with T-duality transformations, cannot change the topology of the underlying space. On the other hand, we have seen that T-duality changes the topology of spacetime, for example the sphere and the lens space have different cohomology groups, and moreover both spaces in the dual pair are smooth. This does not mean that the T-duality transformation is necessarily smooth, but a smooth transformation of E can never induce the T-dual geometry on the spacetime, i.e. only singular gauge transformations of E may be of interest as they may produce the desirable T-dual space.
The modified proposal of [2] discussed above also suffers a similar problem in that the patching condition (4.8) does not reproduce the Buscher rules and cannot accommodate dual angular coordinates.

C-spaces and DFT coordinates
Here we shall propose a scenario which illustrates the role of the various coordinates and how the Buscher T-dual spaces can be incorporated using the C-space construction of [11]. Given a good cover {U α } of the spacetime M, one introduces new coordinates y 1 α on every open set U α and angular coordinates θ αβ on every intersection U αβ and imposes the patching conditions −y 1 α + y 1 β + dθ αβ = a 1 αβ , θ αβ + θ βγ + θ γα + a 0 αβγ = 0 mod 2πZ , (5.1) on U αβ and U αβγ . Then consistency with (4.1) at triple and fourfold overlaps implies which is satisfied provided that 1 2π H represents a class in H 3 (M, Z). The angular coordinates at double intersections are associated with the fibre directions of the principal U (1) bundles that arise in the Hitchin-Chatterjee description of gerbes [20,21], explained in detail in [22].
Common sector theories with O(d, d) local gauge symmetry can be described solely in terms of generalised geometry, i.e. without the introduction of additional coordinates. Such theories can also be described in terms of C-spaces, as discussed in [11]. In this context of C-spaces additional one-form coordinates can be introduced, as we have seen above, and it was shown in [11] that the first patching condition in (5.1) can be used to introduce new one-form coordinates which are globally defined on the spacetime, i.e.ỹ 1 α =ỹ 1 β . Here {ρ α } is a partition of unity subordinate to the good cover. It seems reasonable on the grounds of their transformation properties to identify theỹ 1 α with the doubled coordinates of [3] which also transform as one-forms, i.e.x =ỹ, after suppressing the degree and open set labels onỹ. This incorporates the the DFT doubled coordinates into a C-space description.
However, we have shown that the Buscher T-dual spaces cannot be described in terms of the (x,x) coordinates alone. So the question that remains is where the Buscher T-dual spaces are hidden in this description. The C-space description contains in addition the angular coordinates θ which describe the gerbe part of the space. We shall argue that the Buscher T-dual spaces are hidden in the gerbe.

Gerbes and Buscher rules
Although in the construction of C-spaces a good cover has been used, for the definition of a Hitchin-Chatterjee gerbe any open cover 5 suffices. We shall use this to adapt an open cover such that the Buscher T-duals can be described as subspaces of gerbes.
To illustrate how gerbes can be constructed, consider the example of S 3 with N units of H flux. We have already seen that the T-dual space of this is the lens space L 3 N with one unit of flux. To describe this gerbe on S 3 [22], we can choose a stereographic cover of two open sets {U 0 , U 1 } on S 3 for which their intersection U 0 ∩ U 1 := U 01 is I × S 2 , I an open interval, and the Mayer-Vietoris description of H 3 (S 3 , Z) which uses representatives localised on U 01 , see e.g. [23]. Such representatives are constructed as follows. As U 01 is contractible to S 2 , choose a representative F 01 of the class Nu in H 2 (S 2 ×I, Z) = H 2 (S 2 , Z) where u is the generator of H 2 (S 2 × I, Z). A representative of 1 2π [H] can be chosen aŝ on U 0 and U 1 , respectively, where {ρ 0 , ρ 1 } is a partition of unity subordinate to the cover {U 0 , U 1 }. Observe that at the intersection As there are no more than double overlaps the rest of the compatibility conditions for the gerbe are trivially satisfied. The gerbe 6 associated to S 3 and H is then the union of S 3 together with the principal U(1) bundle on U 01 which has first Chern class Nu.
Observe that the principal bundle over U 01 when restricted on S 2 ⊂ U 01 ⊂ S 3 is the Lens space L 3 N . It is significant that the lens space L 3 N which is the T-dual to S 3 naturally appears in this gerbe construction. Prompted by this, it is tempting to identify the T-dual angular coordinateθ with the fibre coordinate of the lens space that appears in the gerbe construction. We shall provide a further explanation for this below.
Suppose next that the spacetime is a product M = S 1 × Q and the 3-form flux where now {ρ 0 , ρ 1 } is a partition of unity subordinate to the {V 0 , V 1 } cover.Ĥ is globally defined on M and it is a representative of the 3-form flux associated to the gerbe. The T-dual space of M is the bundle space of P 01 which is clearly a subspace of the total space of the gerbe. As a special case of the above take Q = T 2 . In this case, M = T 3 and H can be chosen as in section 2.4 in which the T-dual pair of T 3 with flux was described. In particular, we set In this case, the restriction of the principal U(1) gerbe bundle P 01 on Q = T 2 ⊂ U 01 ⊂ T 3 is the T-dual spaceT 3 as described by the Buscher T-duality rules. For a different treatment of this example, see [?]. As a final example we take M to be a circle bundle over Q with 3-form flux H that can be represented as [H] = aw, where w ∈ H 2 (Q, Z) and a is the generator of H 1 (S 1 , Z). Take an open cover {W α } on Q which trivialises the circle bundle M over Q, i.e. π −1 (W α ) = ϕ −1 α (W α × S 1 ), where π : M → Q is the projection and ϕ α : π −1 (W α ) → W α × S 1 is the trivilisation map, and write each W α × S 1 as the union of the open set W α × V 0 and W α × V 1 , where {V 0 , V 1 } are the two open sets that cover S 1 introduced above. It is clear that {ϕ −1 α (W α × V r )}, r = 0, 1, is a cover for M.

As the union of open sets is open
) are open and cover M. As in the case that M was a product, we consider a representative F of the class w ∈ H 2 (Q) and its pull back to M with the projection map π. Restricting F to the intersection of U 01 and denoting it by F 01 , we can construct a representativeĤ of the H flux as in (5.4), where again {ρ 0 , ρ 1 } is a partition of unity subordinate to the cover {U 0 , U 1 }.Ĥ is globally defined and represents [H] = aw as the derivatives of the partition functions at the intersection of open sets on the circle represent the generator of H 1 (S 1 , Z). It is clear that the gerbe is the union of spacetime with a circle bundle defined on the open set U 01 of M which is the restriction of the pull-back of a circle bundle over the base space Q with Chern class w. The circle bundle over Q is the T-dual space derived from the Buscher rules. If S 3 is viewed as a circle fibration over S 2 and H represents N units of flux, the above gerbe construction will also lead to the identification of the T-dual space as L 3 N . It is clear that the gerbes in all the above examples have simple descriptions because the spacetimes have been covered by only two open sets.

Summary of the proposal
The above results provide evidence to suggest that the double coordinatesx of DFT that transform like 1-forms [3] should be identified with theỹ coordinates that occur in Cspaces, eqn (5.3). DFT can be formulated with only these coordinates and will exhibit local O(d, d) symmetry as such a description accommodates generalised geometry both from the double spaces point of view and that of C-spaces. However, such a formulation will not describe the T-dual spaces of the spacetime. This is regardless of the choice of solution to the strong section condition that one makes on the doubled space.
Our results have also established that the T-dual space of a spacetime with H flux can be identified as a subspace of a gerbe which is part of the C-space. This has been done explicitly for the T-dual space derived after performing T-duality along the fibre direction of a spacetime which is a circle fibre bundle. This identification requires the presence of additional coordinates from those of doubled space which are the fibre coordinates of the principal U(1) bundles that lie on double intersections of an open cover of the spacetime and are required in the description of the gerbe.
We have given two gerbe descriptions of the T-dual space of S 3 with N units of H flux example. The first description was in terms of a stereographic cover and the other in terms of a cover adapted to the fibration over S 2 . In both cases, the T-dual space has been identified as the lens space L 3 N . In hindsight this may have been expected. The T-dual space should be independent from a large enough selection of covers on the spacetime that are used to describe the gerbe. This can be seen as the requirement for the construction of gerbes and that of T-dual spaces to be covariant. In turn one can view this as a covariant description of the Buscher T-duality rules.

Conclusions
We have made a proposal based on C-spaces and the Hitchin-Chatterjee description of a gerbe where both the local (bundle) O(d, d) symmetry and the T-dual spaces of a spacetime can be described in a globally consistent way. In particular, we have demonstrated that the doubled space of a DFT as described in [3] can be included into a C-space and the O(d, d) symmetry arises as part of the generalised geometry structure on C-spaces. Furthermore, we have demonstrated that the T-dual spaces of a spacetime that are constructed using Buscher rules can be identified as subspaces of the gerbe which is included in C-spaces but not in the doubled spaces. In this identification, the T-dual angular coordinate of a spacetime which is a circle fibration with T-duality operation taken along the fibre circle is identified with the gerbe angular coordinate which is the fibre coordinate of a principal U(1) bundle defined on an intersection of two open sets of the spacetime.
Our analysis has indicated that it is not possible to formulate a theory which exhibits both local O(d, d) symmetry and at the same time has a description of all the T-dual spaces of a spacetime based only on doubled spaces. Using the available globally consistent definitions of doubled spaces, we have demonstrated that these cannot provide an explanation for the property of the T-dual circles to topologically twist over the spacetime. This topological twisting has been established in several examples and it is a consequence of the Buscher rules. In other words, the T-dual spaces cannot arise in DFT as different solutions to the (strong) section condition on doubled spaces.
The inclusion of gerbes in a consistent definition of a theory which exhibits local O(d, d) symmetry and which describes the T-dual spaces of a spacetime requires the presence of additional angular coordinates, the gerbe coordinates. Such spaces are not manifolds and in particular they do not have a fixed dimension. Nevertheless they contain all the necessary ingredients for the definition of the theory including the ability to perform differential geometry computations related to O(d, d) symmetry and the topological properties required for the descrption of the T-dual spaces.
The gerbe description of T-dual spaces of a spacetime has some additional consequences. First notice that the Buscher rules are not covariant. Their formulation involves several gauge choices and their construction is essentially local on the spacetime. Moreover, they depend on the spacetime admitting an isometry. On the other hand gerbes can be defined on any smooth manifold with a closed 3-form flux H without further additional assumptions. Therefore the gerbe description can be seen as a covariantisation of the Tduality rules. Furthermore the gerbe description opens the possibility that it might be possible to investigate the T-duals of a spacetime that does not admit isometries. In this case, however, it may not be possible to identify the subspaces of the gerbe which can be characterised as T-dual spaces as we have done in the case of spacetimes with isometries. Even if the T-dual spaces can be identified, it is likely that they will not be manifolds.