The cosmological constant is related to the topological theta angle by theta = 12 pi^2 / (Lambda l_Pl^2), suggesting Lambda is topologically protected.
Quantum gravity as a Fermi liquid
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abstract
We present a reformulation of loop quantum gravity with a cosmological constant and no matter as a Fermi-liquid theory. When the topological sector is deformed and large gauge symmetry is broken, we show that the Chern-Simons state reduces to Jacobson's degenerate sector describing 1+1 dimensional propagating fermions with nonlocal interactions. The Hamiltonian admits a dual description which we realize in the simple BCS model of superconductivity. On one hand, Cooper pairs are interpreted as wormhole correlations at the de Sitter horizon; their number yields the de Sitter entropy. On the other hand, BCS is mapped into a deformed conformal field theory reproducing the structure of quantum spin networks. When area measurements are performed, Cooper-pair insertions are activated on those edges of the spin network intersecting the given area, thus providing a description of quantum measurements in terms of excitations of a Fermi sea to superconducting levels. The cosmological constant problem is naturally addressed as a nonperturbative mass-gap effect of the true Fermi-liquid vacuum.
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The Cosmological Constant from a Quantum Gravitational $\theta$-Vacua and the Gravitational Hall Effect
The cosmological constant is related to the topological theta angle by theta = 12 pi^2 / (Lambda l_Pl^2), suggesting Lambda is topologically protected.