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Bosonisation Cohomology: Spin Structure Summation in Every Dimension

Philip Boyle Smith, Joe Davighi

Abstract

Gauging fermion parity and summing over spin structures are subtly distinct operations. We introduce 'bosonisation cohomology' groups $H_B^{d+2}(X)$ to capture this difference, for theories in spacetime dimension $d$ equipped with maps to some $X$. Non-trivial classes in $H_B^{d+2}(X)$ contain theories for which $(-1)^F$ is anomaly-free, but spin structure summation is anomalous. We formulate a sequence of cobordism groups whose failure to be exact is measured by $H_B^{d+2}(X)$, and from here we compute it for $X=\text{pt}$. The result is non-trivial only in dimensions $d\in 4\mathbb{Z}+2$, being due to the presence of gravitational anomalies. The first few are $H_B^4=\mathbb{Z}_2$, probed by a theory of 8 Majorana-Weyl fermions in $d=2$, then $H_B^8=\mathbb{Z}_8$, $H_B^{12}=\mathbb{Z}_{16}\times \mathbb{Z}_2$. We rigorously derive a general formula extending this to every spacetime dimension. Along the way, we compile many general facts about (fermionic and bosonic) anomaly polynomials, and about spin and pin$^-$ (co)bordism generators, that we hope might serve as a useful reference for physicists working with these objects. We briefly discuss some physics applications, including how the $H_B^{12}$ class is trivialised in supergravity. Despite the name, and notation, we make no claim that $H_B^\bullet(X)$ actually defines a cohomology theory (in the Eilenberg-Steenrod sense).

Bosonisation Cohomology: Spin Structure Summation in Every Dimension

Abstract

Gauging fermion parity and summing over spin structures are subtly distinct operations. We introduce 'bosonisation cohomology' groups to capture this difference, for theories in spacetime dimension equipped with maps to some . Non-trivial classes in contain theories for which is anomaly-free, but spin structure summation is anomalous. We formulate a sequence of cobordism groups whose failure to be exact is measured by , and from here we compute it for . The result is non-trivial only in dimensions , being due to the presence of gravitational anomalies. The first few are , probed by a theory of 8 Majorana-Weyl fermions in , then , . We rigorously derive a general formula extending this to every spacetime dimension. Along the way, we compile many general facts about (fermionic and bosonic) anomaly polynomials, and about spin and pin (co)bordism generators, that we hope might serve as a useful reference for physicists working with these objects. We briefly discuss some physics applications, including how the class is trivialised in supergravity. Despite the name, and notation, we make no claim that actually defines a cohomology theory (in the Eilenberg-Steenrod sense).

Paper Structure

This paper contains 33 sections, 137 equations, 4 figures.

Figures (4)

  • Figure 1: The cobordism sequence \ref{['eq:int:seq']} in low degrees $n \leq 13$.
  • Figure 2: An illustration of the suspension $\Sigma X$ for some space $X$ indicated by the blue disc. One can think of 'hanging' $X$ between two endpoints. For reduced suspension, all the basepoints, indicated by the red line, are also identified.
  • Figure 3: Illustration of how to go left and right through the Smith isomorphism.
  • Figure 4: The construction of the manifold $Y$ from $(M, \rho, A)$.