Energy in the very early Universe

Details Energy in the very early Universe Energy in the very early Universe

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007phlb..649..299d&link_type=abstract

Physics Letters B, Volume 649, Issue 4, p. 299-309.

Physics

Lower Dimensional Models, Minisuperspace Models, Quantum Cosmology

Scientific paper

The K=0 Friedmann Robertson Walker metric, which satisfies the Killing spinor equation and approximates a solution to the field equations of the quadratic gravity theory derived from the heterotic string effective action, generates a discontinuity in the derivative of the scale factor. The resulting change in the Hamiltonian is conjectured to be the origin of energy in the very early Universe.

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