Numerical calculations of minisuperspace cosmological models

Details Numerical calculations of minisuperspace cosmological models Numerical calculations of minisuperspace cosmological models

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985phlb..151...15h&link_type=abstract

Physics Letters B, Volume 151, Issue 1, p. 15-20.

Physics

41

Scientific paper

The wave function of the universe is calculated numerically by solving the zero energy Schrödinger equation for homogeneous isotropic cosmological models with a massive scalar field or with curvature squared corrections to the action. The boundary condition used to integrate the equation is that the wave function should be given by a path integral over compact metrics.

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