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(96) Working out the Poisson bracket between the two constraints we now find: {V2,H2} = Λ ( 1− 3P 4a3Λ ) 6 H2 + ΛP ( 2a3− 3P Λ ) 48a4

Theory 2 in the presence of dust matter Using the results of Appendix II, it can be seen that for Theory 2 in the presence of dust we now have the Hamiltonian H2 =−2N √ a2H2−VV2 (9

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Parity violating Friedmann Universes

gr-qc · 2019-08-14 · conditional · novelty 7.0

In a varying-Lambda Einstein-Cartan theory, homogeneous and isotropic spacetimes can violate parity via torsion, adding a genuine new degree of freedom with Weyl curvature.

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  • Parity violating Friedmann Universes gr-qc · 2019-08-14 · conditional · none · ref 7

    In a varying-Lambda Einstein-Cartan theory, homogeneous and isotropic spacetimes can violate parity via torsion, adding a genuine new degree of freedom with Weyl curvature.