Cosmological aspects of the theory of relativistic bi-Hamiltonian systems. 1. Formation of the space-time continuum of the general theory of relativity

Details Cosmological aspects of the theory of relativistic bi-Hamiltonian systems. 1. Formation of the space-time continuum of the general theory of relativity Cosmological aspects of the theory of relativistic bi-Hamiltonian systems. 1. Formation of the space-time continuum of the general theory of relativity

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ruphj..38..197s&link_type=abstract

Russian Physics Journal, Volume 38, Issue 2, pp.197-204

Physics

Scientific paper

Starting from the fundamental propositions of the nonunitary quantum theory of relativistic bi-Hamiltonian systems, an attempt is made to explain the nature of the big bang by identifying it with a total f→f transition occurring in an ensemble of relativistic bi-Hamiltonian systems. The main principles controlling the formation of the space—time continuum of the general theory of relativity are formulated here.

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