3 ms·
Could the math 'shape' of the universe solve the cosmological constant problem?
- k310 6mo agoPaper is free at arxiv. https://arxiv.org/abs/2506.14886 https://arxiv.org/abs/2506.14886 The Cosmological Constant from a Quantum Gravitational θ-Vacua and the Gravitational Hall Effect Stephon Alexander, Heliudson Bernardo, Aaron Hui We provide a new perspective on the cosmological constant by exploring the background-independent Wheeler-DeWitt quantization of general relativity. The Chern-Simons-Kodama state of quantum gravity, a generalization of the Hartle-Hawking and Vilenkin states, has a striking structural similarity to the topological field theory of the quantum Hall effect. As a result, we study the gravitational topological θ-sectors in analogy to Yang-Mills theory. We find that the cosmological constant Λ is intimately linked to the θ-parameter by θ=12π2/(Λℓ2Pl)mod2π due to the fact that Chern-Simons-Kodama state must live in a particular θ-sector. This result is shown in the canonical, non-perturbative formalism. Furthermore, we explain how the physics of the Hamiltonian constraint is analogous to the quantum Hall effect, with the cosmological constant playing the role of a quantum gravitational Hall resistivity. These relations suggest that Λ is topologically protected against perturbative graviton loop corrections, analogous to the robustness of quantized Hall conductance against disorder in a metal.