vix.ing · top · new · best · stats · spec

New Solutions To The Bianchi IX Wheeler DeWitt Equation And Leading Order Solutions For Λ ≠ 0 And A Primordial Magnetic Field

2019/10/26 by Daniel Berkowitz, Berkowitz, Daniel
Physics and Astronomy · #Experimental and Theoretical Physics Studies #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Mathematical Physics (math-ph) #Quantum Physics (quant-ph) #Solar and Space Plasma Dynamics

paper · pdf · doi:10.48550/arxiv.1910.11970

openalex publication_date 2019/10/26 · openalex created_date 2024/04/11 · openalex updated_date 2026/07/28

Abstract

New closed form solutions to the Lorentzian signature symmetry reduced Bianchi IX Wheeler DeWitt equation are obtained using a Euclidean-signature semi classical method for Hartle Hawking ordering parameters ± 2√(33) for the wormhole Hamilton-Jacobi solution. Moving past the wormhole case we also compute first order quantum corrections to Bianchi IX wave functions restricted to the β+ axis for the 'no boundary' solution and one of the 'arm' solutions. Furthermore, six solutions to the Bianchi IX Euclidean-signature Hamiltonian Jacobi equation for the case when a cosmological constant is present have been found and are used to construct a semi-classical which respects the symmetry of the Bianchi IX potential. Also two additional solutions were found when both a cosmological constant and an aligned primordial magnetic field are present, which are also used to construct a leading order wave function. Furthermore we construct leading order 'excited' states which are restricted to the β+ axis for the cases when a cosmological constant and a primordial magnetic field are present. To conclude, we discuss the interesting features of our solutions, and point out how the cosmological constant appears to act as a driver of anisotropy in our Bianchi IX models. The Euclidean-signature semi-classical method used here is applicable to certain field theories as well. Because this semi classical method was able to find new solutions to a heavily studied problem the results in this paper represent significant progress in the Wheeler-DeWitt approach to quantum cosmology and in the application of Euclidean-signature semi classical methods to Lorentzian signature problems in general.

Related