Mach's principle and matter production process in non-steady state cosmological model

Details Mach's principle and matter production process in non-steady state cosmological model Mach's principle and matter production process in non-steady state cosmological model

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pthph..53.1365g&link_type=abstract

Progress of Theoretical Physics, vol. 53, May 1975, p. 1365-1371.

Physics

1

Astronomical Models, Cosmology, Mach Inertia Principle, Matter (Physics), Boundary Value Problems, Einstein Equations, Relativity, Tensor Analysis

Scientific paper

A Hoyle-Pryce tensor can be introduced into the Einstein field equations of general relativity as a possible inference from Mach's principle as formulated in Whitrow's relation. The set of equations obtained can be completely determined for the matter injection field, pressure, density and scaling functions in a closed model universe with asymptotically limited expansion. This model presents a cosmic density higher than the usually accepted value for the smearing out of galactic matter.

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