Quantum Transitions Between Minkowski and de Sitter Spacetimes

Abstract

Quantum transitions among de Sitter and Minkowski spacetimes through bubble nucleation are revisited using the Hamiltonian formalism. We interpret tunnelling probabilities as relative probabilities: the ratio of the squared wave functionals $\mathcal{P}=\frac{|{\Psi }_{\mathcal{N}}{|}^2}{|{\Psi }_{\mathcal{B}}{|}^2}$, with ${\Psi }_{\mathcal{B},\mathcal{N}}$ solutions of the Wheeler-DeWitt equation corresponding to the spacetimes $\mathcal{N}$ and $\mathcal{B}$, gives the probability of nucleating the state $\mathcal{N}$ relative to the probability of having the state $\mathcal{B}$. We find that the transition amplitude from de Sitter to de Sitter for both up- and down-tunnelling agrees with the original result based on Euclidean instanton methods. Expanding on the work of Fischler, Morgan and Polchinski we find that the Minkowski to de Sitter transition is possible as in the original Euclidean approach of Farhi, Guth and Guven. We further generalise existing calculations by computing the wave function away from the turning points for the classical motion of the wall in de Sitter to de Sitter transitions. We address several challenges for the viability of the Minkowski to de Sitter transition, including consistency with detailed balance and AdS/CFT. This sets this transition on firmer grounds but opens further questions. Our arguments also validate the Coleman-De Luccia formulae in the presence of gravity since it has no issues involving negative eigenmodes and other ambiguities of the Euclidean approach. We briefly discuss the implications of our results for early universe cosmology and the string landscape.

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• Bayesian Reasoning in Eternal Inflation: A Solution to the Measure Problem
• Negative Mode Problem of False Vacuum Decay Revisited
• A Local Wheeler-DeWitt Measure for the String Landscape
• Lorentzian Vacuum Transitions with a Generalized Uncertainty Principle
• A Menagerie of Wormholes and Cosmologies in the Gravitational Path Integral
• Lorentzian Vacuum Transitions for Anisotropic Universes
• Effects of quantum corrections to Lorentzian vacuum transitions in the presence of gravity