Gauge-covariant flux corrections in loop quantum cosmology produce an asymmetric quantum bounce with a (2/pi)^4 rescaling of Newton's constant in the pre-bounce branch.
Ashtekar, New Hamiltonian formulation of General Relativity, Phys
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New Loop Quantum Cosmology Modifications from Gauge-covariant Fluxes
Gauge-covariant flux corrections in loop quantum cosmology produce an asymmetric quantum bounce with a (2/pi)^4 rescaling of Newton's constant in the pre-bounce branch.