Generalised Symmetries and Swampland-Type Constraints from Charge Quantisation via Rational Homotopy Theory
Luigi Alfonsi, Hyungrok Kim, William G. A. Luciani
TLDR
This paper refines a charge quantization postulate using rational homotopy theory, deriving new swampland-like constraints on quantum field theories and gravity.
Key contributions
- Refines charge quantization postulate for QFT/string theory, incorporating matter and higher gauge theory.
- Homotopy groups of $\mathcal A$ classify brane charges; homology groups classify invertible higher-form symmetries.
- Derives swampland-like constraints, ruling out noncompact gauge groups and non-nilpotent 1-form field strengths.
- Argues $\mathcal A$ must be contractible for quantum gravity, consistent with swampland conjectures.
Why it matters
This paper offers a novel framework connecting charge quantization to fundamental constraints on quantum field theories and quantum gravity. It provides a concrete mechanism for deriving swampland-like conjectures from first principles, deepening our understanding of consistent theories.
Original Abstract
Sati and Schreiber [arXiv:2402.18473, arXiv:2512.12431] have proposed that charge quantisation in quantum field theory and string theory is governed by a homotopy type $\mathcal A$. We provide a refinement of this postulate, incorporating other currents including matter, connecting it to adjustments in higher gauge theory and providing a prescription for determining $\mathcal A$, and show that, while the homotopy groups of $\mathcal A$ classify the possible brane charges, the homology groups of $\mathcal A$ classify the invertible higher-form symmetries. Furthermore, we show that the charge-quantisation postulate implies a number of non-trivial constraints on quantum field theories similar to those implied by swampland conjectures; in particular, it rules out noncompact gauge groups and one-form field strengths that form a non-nilpotent Lie algebra. Finally, we argue that for theories of quantum gravity the space $\mathcal A$ must be contractible, in accordance with the swampland conjectures on the absence of global generalised symmetries and the completeness of the spectrum of charges, and explain how this explicitly arises in the case of Type I string theory.
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