The refined de Sitter conjecture

Let Φ=(ϕ1,,ϕN)\Phi=(\phi^1,\dots,\phi^N) be scalar fields with potential V(Φ)V(\Phi) in a low-energy effective field theory coupled to dynamical DD-dimensional spacetime. Let i\nabla_i denote the covariant derivative for the field-space metric, and let ijV\nabla_i\nabla_jV be evaluated in an orthonormal frame. Refined de Sitter conjecture. At least one of the inequalities

iVc1MPV|\nabla_iV|\geq\frac{c_1}{M_{\mathrm{P}}}V

and

min(ijV)c2MP2V\min(\nabla_i\nabla_jV)\leq-\frac{c_2}{M_{\mathrm{P}}^2}V

must hold, where c1c_1 and c2c_2 are positive constants of order one.

This conjecture is a proposed obstruction to stable de Sitter vacua in quantum gravity and refines the original de Sitter conjecture by allowing a sufficiently tachyonic direction. Its status is not resolved here.

Sources & referencesView supporting material

Primary source

Davide De Biasio, “Geometric flows and the Swampland”, arXiv:2307.08320 (2023).

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