Conserved energy for Robertson-Walker spacetimes with scalar fields

Details Conserved energy for Robertson-Walker spacetimes with scalar fields Conserved energy for Robertson-Walker spacetimes with scalar fields

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phrvd..38.3815h&link_type=abstract

Physical Review D (Particles and Fields), Volume 38, Issue 12, 15 December 1988, pp.3815-3818

Physics

1

Fundamental Problems And General Formalism, Lagrangian And Hamiltonian Approach

Scientific paper

Energy for Robertson-Walker spacetimes is defined using the static Einstein spacetime as a reference space. The energy is shown to be equivalent to the dilatation operator. This leads to a useful formulation for the dynamics and for a quantum field theory on a classical Roberston-Walker spacetime; it also provides the basis for a microcanonical entropy.

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