2008/07/11 by M. Ibison, Ibison, M. · 1 citation
Physics and Astronomy · #Cosmology and Gravitation Theories #FOS: Physical sciences #General Physics (physics.gen-ph) #General Relativity and Quantum Cosmology (gr-qc) #Relativity and Gravitational Theory #gr-qc #physics.gen-ph
paper · pdf · doi:10.48550/arxiv.0807.1884
References updated, submitted to CQG
openalex publication_date 2008/07/11 · arxiv created 2008/10/04 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The cosmological scale factor a(t) of the flat-space Robertson-Walker geometry is examined from a Hamiltonian perspective wherein a(t) is interpreted as an independent dynamical coordinate and the curvature density √ - g(a) R(a, a, a) is regarded as an action density in Minkowski spacetime. The resulting Hamiltonian for a(t) is just the first Friedmann equation of the traditional approach (i.e. the Robertson-Walker cosmology of General Relativity), as might be expected. The utility of this approach however stems from the fact that each of the terms matter, radiation, and vacuum, and including the kinetic / gravitational field term, are formally energy densities, and the equation as a whole becomes a formal statement of energy conservation. An advantage of this approach is that it facilitates an intuitive understanding of energy balance and exchange on the cosmological scale that is otherwise absent in the traditional presentation. Each coordinate system has its own internally consistent explanation for how energy balance is achieved. For example, in the spacetime with line element ds2 = dt2 - a2(t) d\bfx2, cosmological red-shift emerges as due to a post-recombination interaction between the scalar field a(t) and the EM fields in which the latter loose energy as if propagating through a homogeneous lossy medium, with the energy lost to the scale factor helping drive the cosmological expansion.