Unitary and Vilenkin's wave functions
arXiv:2304.00666 · doi:10.1103/PhysRevD.108.023526
Abstract
It is remarkably difficult to reconcile unitary and Vilenkin's wave function. For example, the natural conserved inner product found in quantum unimodular gravity applies to the Hartle-Hawking wave function, but fails for its Vilenkin counterpart. We diagnose this failure from different angles (Laplace transform instead of Fourier transform, non-Hermiticity of the Hamiltonian, etc) to conclude that ultimately it stems from allowing the connection to become imaginary in a section of its contour. In turn this is the unavoidable consequence of representing the Euclidean theory as an imaginary image within a fundamentally Lorentzian theory. It is nonetheless possible to change the underlying theory and replace the connection's foray into the imaginary axis by an actual signature change (with the connection, action and Hamiltonian remaining real). The structural obstacles to unitarity are then removed, but special care must still be taken, because the Euclidean theory {\it a priori} has boundaries, so that appropriate boundary conditions are required for unitarity. Reflecting boundary conditions would reinstate a Hartle-Hawking-like solution in the Lorentzian regime. To exclude an incoming wave in the Lorentzian domain one must allow a semi-infinite tower of spheres in the Euclidean region, wave packets travelling through successive spheres for half an eternity in unimodular time. Such "Sisyphus" boundary condition no longer even vaguely resembles Vilenkin's original proposal.
arXiv comment13 pages, 7 figures
References in corpus (19)
- Forks in the Road, on the Way to Quantum Gravity
- Approaches to Quantum Cosmology
- The quantization of unimodular gravity and the cosmological constant problem
- No smooth beginning for spacetime
- Tunneling wave function of the universe
- Singularity resolution depends on the clock
- Unimodular loop quantum gravity and the problems of time
- Tunneling wave function of the universe II: the backreaction problem
- Cosmological time and the constants of nature
- Instantons and unitarity in quantum cosmology with fixed four-volume
- Uses of Complex Metrics in Cosmology
- Equivalence of the Chern-Simons state and the Hartle-Hawking and Vilenkin wave-functions
- Unstable no-boundary fluctuations from sums over regular metrics
- Cosmological signature change in Cartan Gravity with dynamical symmetry breaking
- Quantum resolution of the cosmological singularity without new physics
- Unimodular Hartle-Hawking wave packets and their probability interpretation
- Lower bound on the cosmological constant from the classicality of the Early Universe
- Torsion and the Probability of Inflation
- Canonical analysis of covariant unimodular gravity and an extension of the Kodama state