© 2017 American Physical Society. It is shown that the standard no-boundary wave function has a natural expression in terms of a Lorentzian path integral with its contour defined by Picard-Lefschetz theory. The wave function is real, satisfies the Wheeler-DeWitt equation and predicts an ensemble of asymptotically classical, inflationary universes with nearly-Gaussian fluctuations and with a smooth semiclassical origin.1 + 10.5 + 2.5 pages, 2 figures. v2: minor changes and added referencesstatus: publishe
In the Hartle-Hawking ``no boundary'' approach to quantum cosmology, a real tunneling geometry is a ...
In this work, we analyze two different aspects of the formulation of Quantum Gravity using the Wave ...
Restricted Access.In quantum cosmology, a wave function ψ for a given theory can be obtained by solv...
It is shown that the standard no-boundary wave function has a natural expression in terms of a Loren...
We argue that the Lorentzian path integral is a better starting point for quantum cosmology than the...
The goal of quantum cosmology is to find a quantum state that describes the entire evolution of our ...
We specify the semiclassical no-boundary wave function of the Universe without relying on a function...
We identify a fundamental obstruction to any theory of the beginning of the universe as a semi-class...
In recent work, we introduced Picard-Lefschetz theory as a tool for defining the Lorentzian path int...
We analyse the impact of various boundary conditions on the (minisuperspace) Lorentzian gravitationa...
The no-boundary wave function (NBWF) specifies a measure for prediction in cosmology that selects in...
We show that the complex saddle points of the no-boundary wave function with a positive cosmological...
We implement the no-boundary proposal for the wave function of the Universe in an exactly solvable B...
We derive a sufficient set of conditions on the Euclidean boundary theory in dS/CFT for it to predic...
Cosmology has, after the formulation of general relativity, been transformed from a branch of philos...
In the Hartle-Hawking ``no boundary'' approach to quantum cosmology, a real tunneling geometry is a ...
In this work, we analyze two different aspects of the formulation of Quantum Gravity using the Wave ...
Restricted Access.In quantum cosmology, a wave function ψ for a given theory can be obtained by solv...
It is shown that the standard no-boundary wave function has a natural expression in terms of a Loren...
We argue that the Lorentzian path integral is a better starting point for quantum cosmology than the...
The goal of quantum cosmology is to find a quantum state that describes the entire evolution of our ...
We specify the semiclassical no-boundary wave function of the Universe without relying on a function...
We identify a fundamental obstruction to any theory of the beginning of the universe as a semi-class...
In recent work, we introduced Picard-Lefschetz theory as a tool for defining the Lorentzian path int...
We analyse the impact of various boundary conditions on the (minisuperspace) Lorentzian gravitationa...
The no-boundary wave function (NBWF) specifies a measure for prediction in cosmology that selects in...
We show that the complex saddle points of the no-boundary wave function with a positive cosmological...
We implement the no-boundary proposal for the wave function of the Universe in an exactly solvable B...
We derive a sufficient set of conditions on the Euclidean boundary theory in dS/CFT for it to predic...
Cosmology has, after the formulation of general relativity, been transformed from a branch of philos...
In the Hartle-Hawking ``no boundary'' approach to quantum cosmology, a real tunneling geometry is a ...
In this work, we analyze two different aspects of the formulation of Quantum Gravity using the Wave ...
Restricted Access.In quantum cosmology, a wave function ψ for a given theory can be obtained by solv...