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+---PAGE_BREAK---
+
+# DIFFERENTIAL MODELS FOR THE ANDERSON DUAL
+TO BORDISM THEORIES AND INVERTIBLE QFT'S
+
+MAYUKO YAMASHITA AND KAZUYA YONEKURA
+
+ABSTRACT. In this paper, we construct new models for the Anderson duals ($I\Omega_G^G$)* to the stable tangential *G*-bordism theories and their differential extensions. The cohomology theory ($I\Omega_G^G$)* is conjectured by Freed and Hopkins [FH21] to classify deformation classes of possibly non-topological invertible quantum field theories (QFT's). Our model is made by abstractizing certain properties of invertible QFT's, thus supporting their conjecture.
+
+## CONTENTS
+
+
| 1. Introduction | 2 |
| 1.1. A sketch of the main results | 3 |
| 1.2. Physical significance | 5 |
| 1.3. Mathematical significance | 10 |
| 1.4. The structure of the paper | 10 |
| 1.5. Notations | 11 |
| 2. Preliminaries | 12 |
| 2.1. Spectra and generalized cohomology theories | 12 |
| 2.2. The Anderson duals | 15 |
| 2.3. Madsen-Tillmann spectra and stable tangential G-bordism theories | 17 |
| 2.4. Singular (co)homology | 21 |
| 2.5. Generalized differential cohomology theories | 25 |
| 2.6. ⟨k⟩-manifolds | 27 |
| 3. Geometric stable tangential G-structures | 30 |
| 3.1. Geometric stable tangential G-structures | 30 |
| 3.2. Geometric Pontryagin-Thom construction | 34 |
| 4. Physically motivated models for the Anderson duals of G-bordisms | 38 |
| 4.1. The models | 39 |
| 4.2. Examples of elements in (IΩdRG)* | 58 |
| 4.3. The proof that (IΩsingG)* is a generalized cohomology theory | 62 |
| 4.4. Self-duality homomorphisms | 74 |
| 5. The proof of the main results | 76 |
| 5.1. The proof of IZsing* ≃ IZ* | 76 |
+
+RESEARCH INSTITUTE FOR MATHEMATICAL SCIENCES, KYOTO UNIVERSITY, 606-8502, KYOTO, JAPAN
+
+DEPARTMENT OF PHYSICS, TOHOKU UNIVERSITY, SENDAI 980-8578, JAPAN
+
+E-mail addresses: mayuko@kurims.kyoto-u.ac.jp, yonekura@tohoku.ac.jp.
+---PAGE_BREAK---
+
+5.2. The proof of $(I\Omega_{\text{sing}}^G)^* \simeq (I\Omega^G)^*$ 82
+
+6. Examples revisited 102
+
+7. Concluding remarks 105
+
+7.1. Normal $G$-structures 105
+
+7.2. Module structures 107
+
+Acknowledgment 107
+
+References 107
+
+# 1. INTRODUCTION
+
+In this paper, we construct new models for the Anderson duals $(I\Omega^G)^*$ to the stable tangential $G$-bordism theories and their differential extensions. Freed and Hopkins [FH21] conjectured that the generalized cohomology theory $(I\Omega^G)^*$ classifies deformation classes of possibly non-topological invertible quantum field theories (QFT's) on stable tangential $G$-manifolds. Our model is physically motivated, in the sense that it is made by abstractizing certain properties of invertible QFT's. Thus the result of this paper supports their conjecture.
+
+Associated to a generalized cohomology theory $E^*$, its *Anderson dual* ([HS05, Appendix B], [FMS07, Appendix B]) is a generalized cohomology theory which we denote by $IE^*$. The crucial property of this theory is that it fits into the following exact sequence for any CW-complex $X$.
+
+$$
+\begin{equation} \tag{1.1}
+\begin{aligned}
+& \cdots \to \operatorname{Hom}(E_{n-1}(X), \mathbb{R}) \to \operatorname{Hom}(E_{n-1}(X), \mathbb{R}/\mathbb{Z}) \to I\mathrm{E}^n(X) \\
+& \qquad \to \operatorname{Hom}(E_n(X), \mathbb{R}) \to \operatorname{Hom}(E_n(X), \mathbb{R}/\mathbb{Z}) \to \cdots \text{ (exact).}
+\end{aligned}
+\end{equation}
+$$
+
+In this paper we are interested in the Anderson dual to *stable tangential G-bordism theories* $\Omega^G$. Here $G = \{G_d, s_d, \rho_d\}_{d \in \mathbb{Z}_{\ge 0}}$ is a sequence of compact Lie groups equipped with homomorphisms $s_d: G_d \to G_{d+1}$ and $\rho_d: G_d \to O(d, \mathbb{R})$ for each $d$ which are compatible with the inclusion $O(d, \mathbb{R}) \hookrightarrow O(d+1, \mathbb{R})$. The homology theory corresponding to $\Omega^G$ is given by the stable tangential $G$-bordism groups $\Omega^G_*(X)$, and the exact sequence (1.1) becomes
+
+$$
+\begin{equation}
+\begin{split}
+& \cdots \to \operatorname{Hom}(\Omega_{n-1}^G(X), \mathbb{R}) \to \operatorname{Hom}(\Omega_{n-1}^G(X), \mathbb{R}/\mathbb{Z}) \to (I\Omega^G)^n(X) \\
+& \qquad \to \operatorname{Hom}(\Omega_n^G(X), \mathbb{R}) \to \operatorname{Hom}(\Omega_n^G(X), \mathbb{R}/\mathbb{Z}) \to \cdots (\text{exact}).
+\end{split}
+\tag{1.2}
+\end{equation}
+$$
+
+The starting point of this work is the following conjecture by Freed and Hopkins.
+
+**Conjecture 1.3** ([FH21, Conjecture 8.37]). There is a 1 : 1 correspondence¹
+
+$$
+(1.4) \quad \left\{ \text{deformation classes of reflection positive invertible } n\text{-dimensional extended field theories with symmetry type } G \right\} \simeq (I\Omega^G)^{n+1}(\mathrm{pt}).
+$$
+
+¹Here *symmetry types* of QFT’s in [FH21] are certain classes of *G’s* in this paper which satisfy an additional set of conditions.
+---PAGE_BREAK---
+
+Difficult points of Conjecture 1.3 are the following. First, we do not have the axioms for non-topological QFT’s. Thus the left hand side of (1.4) is not a mathematically well-defined object. Second, although the cohomology theory $(I\Omega^G)^*$ is mathematically defined, its definition is abstract. So the right hand side of (1.4) is difficult to treat directly. Actually, those difficulties are overcome if we are interested in topological QFT’s, and Freed and Hopkins proves the version of Conjecture 1.3 for topological QFT’s, where the right hand side of (1.4) is replaced by its torsion part [FH21, Theorem 1.1].
+
+This work is intended to overcome the second difficulty mentioned above, and to give a new approach to Conjecture 1.3. We construct a physically motivated model for the theory $(I\Omega^G)^*$, which is made by abstractizing certain properties of invertible QFT’s. This result supports Conjecture 1.3. On the other hand, our results also turn out to be mathematically interesting, in view of its relations to *differential cohomology theories*.
+
+In the rest of the introduction, we first explain the main result of this paper in Subsection 1.1, and then explain its physical significance in Subsection 1.2, and its mathematical significance in Subsection 1.3.
+
+**1.1. A sketch of the main results.** The main results of this paper is the construction of models for the generalized cohomology theory $(I\Omega^G)^*$ and its differential extension. Actually we construct two models, the *differential model* $(I\Omega_{\mathrm{dR}}^G)^*$ (Definition 4.11) which is defined for manifolds, and the *singular model* $(I\Omega_{\mathrm{sing}}^G)^*$ (Definition 4.56) which is defined for topological spaces. Here we only sketch the construction of the differential model. The precise definition is given in Definition 4.11. The physical meaning of this construction is explained in Subsection 1.2 below. For simplicity, in this subsection we only consider the case where $G$ is oriented, i.e., the image of $\rho_d: G_d \to \mathrm{O}(d, \mathbb{R})$ lies in $\mathrm{SO}(d, \mathbb{R})$ for each $d$.
+
+Let $X$ be a manifold and let $n$ be a nonnegative integer. The construction starts by defining the larger group $(I\Omega_{\mathrm{dR}}^G)^n(X)$, which is going to be the model for the differential extension. It consists of pairs $(\omega, h)$, where
+
+* $\omega \in \Omega_{\mathrm{clo}}^n(X; \lim_{\leftarrow d} (\mathrm{Sym}^{\bullet/2} g_d^*))$, i.e., $\omega$ is a closed differential form on $X$ with values in invariant polynomials on $g := \lim_{\leftarrow d} g_d$, of total degree $n$, where $g_d$ is the Lie algebra of $G_d$.
+
+* $h$ is a map which assigns an $\mathbb{R}/\mathbb{Z}$-value to a triple $(M, g, f)$, where $M$ is a closed $(n-1)$-dimensional manifold with a stable tangential $G$-structure with connection, which we call a *geometric stable tangential $G$-structure* and symbolically denoted by $g$, and a smooth map $f: M \to X$.
+
+* $\omega$ and $h$ should satisfy the following compatibility condition. Suppose we have a compact $n$-dimensional manifold with boundary $(W, \partial W)$ equipped with a geometric stable tangential $G$-structure $g_W$ and a map $f_W: W \to X$. Assume that all the structures are compatible with a collar structure near $\partial W$, so that it defines a triple $(\partial W, \partial g_W, f_W|_{\partial W})$ as above. The data $g_W$ allows us to define
+---PAGE_BREAK---
+
+a top form on $W$,
+
+$$ (1.5) \qquad \mathrm{cw}_{g_W}(f_W^*\omega) \in \Omega^n(W), $$
+
+by applying the Chern-Weil construction with respect to $g_W$ to the coefficient of $f_W^*\omega$. We require that,
+
+$$ (1.6) \qquad h([\partial W, \partial g_W, f_W | \partial W]) = \int_W \mathrm{cw}_{g_W}(f_W^*\omega) \pmod{\mathbb{Z}}. $$
+
+To define $(I\Omega_{\mathrm{dR}}^G)^n(X)$, we introduce the equivalence relation $\sim$ on $(\widehat{I\Omega_{\mathrm{dR}}^G})^n(X)$. We set $(\omega, h) \sim (\omega', h')$ if there exists $\alpha \in \Omega^{n-1}(X; \lim_{\leftarrow d} (\mathrm{Sym}^{\bullet/2} g_d^*))$ such that
+
+$$ \omega' = \omega + d\alpha, $$
+
+$$ (1.7) \qquad h'([M, g, f]) = h([M, g, f]) + \int_M \mathrm{cw}_g(f^*\alpha). $$
+
+We define
+
+$$ (1.8) \qquad (I\Omega_{\mathrm{dR}}^G)^n(X) := (\widehat{I\Omega_{\mathrm{dR}}^G})^n(X) / \sim. $$
+
+The main result of this paper concerning the differential model is the following.
+
+**Theorem 1.9** (Proposition 4.70, Proposition 4.122 and Theorem 5.21). $(I\Omega_{\mathrm{dR}}^G)^*$ gives a model for the generalized cohomology theory $(I\Omega^G)^*$, restricted to the category of manifolds. Moreover, $(\widehat{I\Omega_{\mathrm{dR}}^G})^*$ is a model for the differential extension of $(I\Omega^G)^*.$
+
+To conclude this subsection, we give an easiest example of elements in $(\widehat{I\Omega_{\mathrm{dR}}^G})^*$. For more examples, see Subsection 4.2.
+
+*Example 1.10* (The holonomy theory (1), Example 4.79). In this example we consider $G = \mathrm{SO} = \{\mathrm{SO}(d, \mathbb{R})\}_d$. Fix a manifold $X$ and a hermitian line bundle with unitary connection $(L, \nabla)$ over $X$. Then we get an element
+
+$$ (c_1(\nabla), \mathrm{Hol}_{\nabla}) \in (\widehat{I\Omega_{\mathrm{dR}}^{\mathrm{SO}}})^2(X). $$
+
+Here,
+
+• $c_1(\nabla) = \frac{\sqrt{-1}}{2\pi} F_\nabla \in \Omega_{\mathrm{clo}}^2(X)$ is the first Chern form of $\nabla$.
+
+• Note that a triple $(M, g, f)$ in this case consists of a closed oriented 1-dimensional manifold $M$ with a map $f: M \to X$, i.e., a closed oriented curve in $X$, along with other data. The map $\mathrm{Hol}_\nabla$ assigns the holonomy of $(L, \nabla)$ along the curve, using the identification $U(1) \simeq \mathbb{R}/\mathbb{Z}$.
+
+Then, the compatibility condition (1.6) follows from the relation of curvature and holonomy, namely for a compact oriented 2-dimensional manifold $(W, \partial W)$ with a map $f_W: W \to X$, we have
+
+$$ \mathrm{Hol}_{\nabla}(f_W|_{\partial W}) = \int_W f_W^* c_1(\nabla) \pmod{\mathbb{Z}}. $$
+---PAGE_BREAK---
+
+1.2. **Physical significance.** Our results are motivated by the problem of classification of invertible field theories. Let us explain some background in physics. In the following discussion, whenever we say “manifolds”, they are always supposed to be equipped with some geometric structure such as Riemannian metric, bundles and their connections, and so on. What geometric structure we consider should be specified in advance.
+
+Very roughly speaking, a $D$-dimensional QFT is a functor from some geometric bordism category to the (super)vector space category as follows. A QFT assigns a Hilbert space of physical states $\mathcal{H}(N)$ to each $(D-1)$-dimensional closed manifold $N$. In particular, we assume that for the empty manifold $N=\emptyset$, we have a canonical isomorphism $\mathcal{H}(\emptyset) \simeq \mathbb{C}$. It assigns a linear map $Z(M) : \mathcal{H}(N_1) \to \mathcal{H}(N_2)$ to each $D$-dimensional compact manifold $M$ with boundaries $\partial M = \bar{N}_1 \cup N_2$ where $\bar{N}_1$ is a manifold which has the opposite structure to that of $N_1$ (such as orientation reversal), and we have assumed that $M$ has appropriate collar structure near the boundaries, $[0, \epsilon) \times N_1$ and $(-\epsilon, 0] \times N_2$ for some $\epsilon > 0$. We do not try to make these axioms precise, but we remark that they are motivated by (Euclidean) path integrals in physics.
+
+An invertible field theory is a QFT in which the Hilbert space of states $\mathcal{H}(N)$ on any closed manifold $N$ is one-dimensional, $\dim \mathcal{H}(N) = 1$. Invertible field theories play crucial roles in the study of anomalies. (See e.g. [Fre14, Mon19] for overviews.) In fact, the classification of deformation classes of invertible QFT's in $D$-dimensions is believed to be the same as classification of anomalies in $(D-1)$-dimensions.² (We will explain what we mean by “deformation classes” in a little more detail later.) In the context of condensed matter physics, deformation classes of invertible field theories are also called symmetry protected topological (SPT) phases or invertible phases of matter. Anomalous ($D-1$)-dimensional theories appear on the boundaries of these invertible phases and have various applications in physics. Therefore, it is an important problem to classify invertible phases.
+
+In the case of topological QFT (TQFT), the classification of invertible phases has been conjectured to be given by certain cobordism groups [Kap14, KTTW14], and later proved at least for some physically motivated classes of structure types and under some axioms of TQFT [FH21, Yon18]. Let $S$ be the structure type under consideration. For instance, we can consider manifolds equipped with Spin structures, and in that case we denote $S = \text{Spin}$.
+
+Then we may define a bordism group $\Omega_D^S(\text{pt})$ of $D$-dimensional manifolds equipped with structure of the type $S$ roughly as follows. We introduce a monoid structure on the set of (isomorphism classes of) manifolds by disjoint union, $M_1 \sqcup M_2$. The empty manifold $\emptyset$ is the unit of this monoid since $M \sqcup \emptyset \simeq M$. Then we divide this monoid by an equivalence relation. If a closed $D$-manifold $M$ is a boundary of some $(D+1)$-manifold $W$, $M = \partial W$, then it is defined to be equivalent to the empty set, $M \sim \emptyset$. By using the fact that $W = [0,1] \times M$ has the boundary $\partial W = M \sqcup \bar{M}$, one can see that we get a group whose elements are represented in terms of manifolds
+
+²We neglect anomalies which do not fit into the general framework, such as Weyl anomalies. Also, there may be subtleties in reflection non-positive theories [CL20].
+---PAGE_BREAK---
+
+$M$ as $[M]$. In particular, the inverse of $[M]$ is $\overline{[M]}$. This group is denoted as $\Omega_D^S(\text{pt})$.
+
+According to [Kap14, KTTW14, FH21, Yon18], deformation classes of invertible TQFT's are classified by the group $\operatorname{Hom}((\Omega_D^S(\text{pt}))_{\text{tor}}, \mathbb{R}/\mathbb{Z})$, where the subscript tor means to take the torsion part of the group. The reason that we take the torsion part is that we are considering deformation classes. To explain this point, let us first consider the group $\operatorname{Hom}(\Omega_D^S(\text{pt}), \mathbb{R}/\mathbb{Z})$. Then the relation between this group and the above axioms of QFT is the following. If we are given an element $h \in \operatorname{Hom}(\Omega_D^S(\text{pt}), \mathbb{R}/\mathbb{Z})$, it means that we can assign to each closed $D$-dimensional manifold $M$ a number
+
+$$ (1.11) \qquad Z(M) = \exp(2\pi\sqrt{-1}h([M))), $$
+
+where $[M] \in \Omega_D^S(\text{pt})$ is the bordism class represented by $M$. Notice that for a closed manifold $\partial M = \emptyset$, a QFT should assign a linear map $Z(M) : \mathcal{H}(\emptyset) \to \mathcal{H}(\emptyset)$. Since $\mathcal{H}(\emptyset) \simeq \mathbb{C}$, the quantity $Z(M)$ can be regarded just as a number $Z(M) \in \mathbb{C}$. The function which assigns a number $Z(M) \in \mathbb{C}$ to each closed manifold $M$ is called a partition function in physics. From an element $h \in \operatorname{Hom}(\Omega_D^S(\text{pt}), \mathbb{R}/\mathbb{Z})$, we can construct a partition function by (1.11).
+
+A partition function itself does not give full data for the axioms of QFT. However, the theorems proved in [FH21, Yon18] imply that we can construct a TQFT from a given $h \in \operatorname{Hom}(\Omega_D^S(\text{pt}), \mathbb{R}/\mathbb{Z})$ (see Theorem 4.3 of [Yon18] for explicit construction), and also the partition function of any invertible TQFT can be deformed continuously to a partition function given by some $h \in \operatorname{Hom}(\Omega_D^S(\text{pt}), \mathbb{R}/\mathbb{Z})$. Among the elements of $\operatorname{Hom}(\Omega_D^S(\text{pt}), \mathbb{R}/\mathbb{Z})$, the ones which come from $\operatorname{Hom}(\Omega_D^S(\text{pt}), \mathbb{R})$ can be deformed continuously. In this way, we arrive at the classification of deformation classes of invertible TQFT's by $\operatorname{Hom}((\Omega_D^S(\text{pt}))_{\text{tor}}, \mathbb{R}/\mathbb{Z})$.
+
+How about the cases which are not necessarily topological? Freed and Hopkins have conjectured a classification [FH21] in terms of the Anderson dual of bordism groups as stated in Conjecture 1.3. Before going to discuss this conjecture, let us first explain some additional background.
+
+Suppose we are given a manifold $X$. Then we can consider a new structure given as follows. In addition to the geometric structure already present in a manifold $M$, we consider an additional datum $f: M \to X$ which is a map from $M$ to $X$. In the context of invertible phases and anomalies in physics, we can consider various types of $X$. If the manifold $X$ is taken to be the target space of a sigma model, it is relevant to sigma model anomalies [MN84, MN85, Tho17]. On the other hand, if $X$ is taken to be the space of coupling constants, it is relevant to more subtle anomalies discussed in e.g. [TY17, STY18, ST19, LMSN18, CFLS19a, CFLS19b, HKT20]. Let us denote the new structure type as $(S, X)$, where $S$ is the original one already considered on $M$. Then we denote $\Omega_D^S(X) := \Omega_D^{(S,X)}(\text{pt})$. For appropriate structure types $S$, it is known that $\Omega_*^S$ gives a generalized homology theory, and $\Omega_*^S(X)$ are the generalized homology groups of $X$.
+
+Given a generalized homology theory $E_*$, we have the Anderson dual cohomology theory $IE^*$ satisfying the exact sequence (1.1). This exact sequence
+---PAGE_BREAK---
+
+is analogous to the one in the ordinary cohomology theory associated to the short exact sequence of coefficient groups $0 \to \mathbb{Z} \to \mathbb{R} \to \mathbb{R}/\mathbb{Z} \to 0$.
+
+The conjecture of Freed-Hopkins, with a generalization including sigma models and more general types of $\mathcal{S}$, is that deformation classes of invertible field theories with the structure type $(\mathcal{S}, X)$ is given by $(I\Omega^S)^{D+1}(X)$, where $(I\Omega^S)^*$ is the Anderson dual of $\Omega_*^S$. It fits into the exact sequence
+
+$$
+\begin{align*}
+& \dots \to \operatorname{Hom}(\Omega_D^S(X), \mathbb{R}) \to \operatorname{Hom}(\Omega_D^S(X), \mathbb{R}/\mathbb{Z}) \to (I\Omega^S)^{D+1}(X) \\
+& \qquad \to \operatorname{Hom}(\Omega_{D+1}^S(X), \mathbb{R}) \to \operatorname{Hom}(\Omega_{D+1}^S(X), \mathbb{R}/\mathbb{Z}) \to \dots
+\end{align*}
+$$
+
+Let us explain physical reasons to believe that this conjecture is reasonable, following [LOT20]. (See also [DL20] for some applications.)
+
+First, let us consider elements of $(I\Omega^S)^{D+1}(X)$ which are in the kernel of the map $(I\Omega^S)^{D+1}(X) \to \operatorname{Hom}(\Omega_{D+1}^S(X), \mathbb{R})$. We denote the homomorphism $\operatorname{Hom}(\Omega_D^S(X), \mathbb{R}) \to \operatorname{Hom}(\Omega_D^S(X), \mathbb{R}/\mathbb{Z})$ as $p$. By the exact sequence, the kernel is isomorphic to
+
+$$
+(1.12) \quad \operatorname{Hom}(\Omega_D^S(X), \mathbb{R}/\mathbb{Z}) / \operatorname{Im}(p) \simeq \operatorname{Hom}((\Omega_D^S(pt))_{\operatorname{tor}}, \mathbb{R}/\mathbb{Z}).
+$$
+
+This is what we have discussed before in the case of TQFT. Any element of $\operatorname{Hom}(\Omega_D^S(X), \mathbb{R}/\mathbb{Z})$ gives a TQFT. The division by the image of the map $p: \operatorname{Hom}(\Omega_D^S(X), \mathbb{R}) \to \operatorname{Hom}(\Omega_D^S(X), \mathbb{R}/\mathbb{Z})$ is due to the fact that we are considering deformation classes. The group $\operatorname{Hom}(\Omega_D^S(X), \mathbb{R})$ is a vector space over $\mathbb{R}$, and any two elements of this group can be continuously deformed into one another. Therefore, we should divide $\operatorname{Hom}(\Omega_D^S(X), \mathbb{R}/\mathbb{Z})$ by $\operatorname{Im}(p)$ when we consider deformation classes of TQFT's.
+
+Next, let us consider the physical meaning of the map $(I\Omega^S)^{D+1}(X) \to \operatorname{Hom}(\Omega_{D+1}^S(X), \mathbb{R})$. In physics, we may expect the following property of invertible QFT. Suppose that a closed $D$-manifold $M$ is the boundary of a ($D+1$)-manifold $W$ with a collar structure $(-\epsilon, 0] \times M \subset W$ near the boundary, including geometric data such that $(-\epsilon, 0]$ has the trivial geometric structure. We expect to have a closed differential ($D+1$)-form $I_{D+1}$ on $W$ (which is sometimes called an anomaly polynomial in the context of anomalies). It is constructed from geometric data on $W$. For example, $W$ may have connections of some bundles from which we can construct characteristic forms. Also, $W$ is equipped with a map $f_W: W \to X$ and hence we can pullback differential forms from $X$ to $W$ by using $f_W$. The closed form $I_{D+1}$ is constructed by using such differential forms, and it is given by $cw_{g_W}(f_W^*\omega)$ which appeared in (1.5) in the case of $\mathcal{S}=G$. Then, physicists may expect that the partition function of an invertible QFT evaluated on $M=\partial W$ is given (after some continuous deformation of the theory$^3$) by
+
+$$
+(1.13) \qquad Z(\partial W) = \exp \left( 2\pi \sqrt{-1} \int_W I_{D+1} \right).
+$$
+
+³In generic theories, there can be nonuniversal terms such as the cosmological constant of the background Riemannian metric and the Euler number term. We need to eliminate them by continuous deformation of the theory for the following claim to be valid. This deformation can be done by a procedure similar to (1.15) below.
+---PAGE_BREAK---
+
+When $I_{D+1} = 0$, this equation is precisely the cobordism invariance of the partition function as implied by (1.11), since $[\partial W] = [\emptyset]$ by the definition of bordism groups.
+
+Now, by using $I_{D+1}$, we can define an element of $\operatorname{Hom}(\Omega_{D+1}^S(X), \mathbb{R})$ by
+
+$$ (1.14) \qquad \Omega_{D+1}^S(X) \ni [W] \mapsto \int_W I_{D+1} \in \mathbb{R} $$
+
+for any closed $(D+1)$-manifold $W$. Its well-definedness (i.e. it only depends on the equivalence class $[W]$ rather than a representative $W$) is immediate from the Stokes theorem and $dI_{D+1} = 0$. Moreover, for the partition function (1.13) to be well-defined, the integral $\int_W I_{D+1}$ on any closed $W$ must be an integer since $\partial W = \emptyset$ implies $Z(\partial W) = 1$. Therefore, (1.14) is actually an element of $\operatorname{Hom}(\Omega_{D+1}^S(X), \mathbb{Z})$, and, equivalently, it is in the kernel of the map $\operatorname{Hom}(\Omega_{D+1}^S(X), \mathbb{R}) \to \operatorname{Hom}(\Omega_{D+1}^S(X), \mathbb{R}/\mathbb{Z})$. For appropriate (but not all)$^4 S$, the fact that any element of $\operatorname{Hom}(\Omega_{D+1}^S(X), \mathbb{Z})$ can be realized in this way by some $I_{D+1}$ will follow from the Chern-Weil theory and the Hurewicz theorem as we will see later in the paper. This gives the exactness at $\operatorname{Hom}(\Omega_{D+1}^S(X), \mathbb{R})$. Also, if $I_{D+1} = dJ_D$ for some $J_D$ which is constructed by geometric data, we get $Z(\partial W) = \exp(2\pi\sqrt{-1}\int_{\partial W} J_D)$. This kind of contribution can be continuously deformed to zero by considering a one parameter family of QFT's parametrized by $t \in [0, 1]$ as
+
+$$ (1.15) \qquad Z_t(M) = \exp \left( 2\pi\sqrt{-1} \int_M t J_D \right), $$
+
+so it does not contribute to the deformation classes of QFT's. This corresponds to taking the equivalence classes as in (1.8). The $\mathbb{R}/\mathbb{Z}$-valued functions $h$ which appeared in the definition of elements of $(I\Omega_{\mathrm{DR}}^G)^n(X)$ correspond to partition functions as $Z = \exp(2\pi\sqrt{-1}h)$, and $cw_g(f^*\alpha)$ in (1.7) corresponds to $J_D$.
+
+The authors are not aware of completely general proof of the expectation that the partition function can be expressed as (1.13). However, there are various evidence supporting this claim. First, (1.13) is exactly what is used in the construction of Wess-Zumino-Witten terms [WZ71] with the target space $X$ by extending a manifold $M$ to $W$ [Wit83]. In physics literature, Chern-Simons invariants are also described by (1.13). (See Example 4.81 for more precise discussions.) Second, invertible field theories constructed from massive fermions in the large mass limit satisfy (1.13). (See e.g. [WY19] for a systematic discussion). Third, other nontrivial examples of invertible QFT's also satisfy (1.13), such as the one relevant for the anomalies of chiral $p$-form fields [HTY20]. Finally, it is possible to give a physically reasonable derivation of a weaker version of the claim as follows. The functional derivative of the log of the partition function $\log Z(M)$ in terms of a background
+
+⁴The following statement fails when the Chern-Weil construction does not give an isomorphism. It happens in some noncompact groups, such as SL(2, R). Thus we have assumed that the groups $G_d$ in this paper are compact. However, there are also groups which are noncompact but the Chern-Weil isomorphism holds. An example is SL(2, Z) which has a trivial real cohomology $H^*(BSL(2, Z), R)$. This group can also have anomalies which are physically relevant [STY18, HTY19, HTY20].
+---PAGE_BREAK---
+
+field $\phi$ (i.e. geometric data such as Riemann metric, connections, etc.) is
+given by a one-point function of some local operator $O$,
+
+$$
+(1.16) \qquad \frac{\partial \log Z(M)}{\partial \phi(x)} = \langle O(x) \rangle, \quad (x \in M)
+$$
+
+In theories whose low energy limits are invertible QFT's, there is no light
+degrees of freedom and all Feynman propagators are short range. Thus we
+expect that the one-point function $\langle O(x) \rangle$ is given by local geometric data at
+the point $x \in M$. Therefore, if two manifolds equipped geometric structure,
+$M$ and $M'$, are homotopy equivalent, the ratio of their partition functions
+is given by an integral of some local quantity.⁵
+
+So far, we have argued that the exact sequence satisfied by $(I\Omega^S)^{D+1}(X)$
+is physically reasonable. However, the above physical arguments do not tell
+us anything about the group $(I\Omega^S)^{D+1}(X)$ itself beyond the exact sequence.
+The Anderson dual is defined in a very abstract way, and it is hard to find
+a direct physical interpretation of the Anderson dual. One of our main
+results stated in Theorem 1.9 is a natural isomorphism of the cohomology
+theory $I\Omega^G$ to the theory $I\Omega_{\text{DR}}^G$. Here the structure type $\mathcal{S}$ is taken to be a
+specific kind specified by $G$. The cohomology theory $I\Omega_{\text{DR}}^G$ is constructed in
+a way which closely follows the above physical discussions. Therefore, our
+results give a very strong support of the Freed-Hopkins conjecture 1.3 and
+its further generalization to include target spaces $X$.
+
+Although $(I\Omega_{\mathrm{DR}}^{G})^{n}(X)$ is the group which is believed to classify the deformation classes of invertible field theories, the group $(\widetilde{I\Omega}_{\mathrm{DR}}^{G})^{n}(X)$ before taking the deformation classes is also physically very relevant. When we make background fields to dynamical fields, invertible field theories give topologically interesting terms in the action of the dynamical fields. Examples of this kind include topological $\theta$-terms in gauge theories and Wess-Zumino-Witten terms in sigma models.
+
+Finally, let us comment on reflection positivity. In the context of parti-
+tion functions, reflection positivity is the following requirement. Consider a
+*D*-manifold *M* with a boundary. We glue *M* and its opposite $\overline{M}$ along their
+boundaries to get a closed manifold *M* ∪ *M* which is called a double. Reflec-
+tion positivity is a requirement that *Z*(*M* ∪ *M*) is a nonnegative real number.
+In the case of TQFT, reflection positivity is an important ingredient in the
+classification of [FH21, Yon18]. Indeed, there are counterexamples to the
+classification if we do not impose reflection positivity. See [FH21, HTY20]
+for these examples. The partition function on a sphere *S*