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Note thatF andf(defined in Eq

Simplified effective modev k dynamics Writing (46) in cosmic time gives ¨vk − ˙F F ˙vk +F 2ω2vk = 0 (49) where the rescaled functionFis F:=− r 2 3 ip ∆J ,(50), the scalar mode e

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Quantum corrections to cosmic perturbations for a bouncing background

gr-qc · 2026-05-15 · unverdicted · novelty 6.0

In an LQC bouncing cosmology, second-order quantum moments yield a Planck-suppressed scale-dependent correction δP_R ∝ (k ℓ_Pl)^6 to the curvature power spectrum together with post-bounce damping from gravitational moments.

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  • Quantum corrections to cosmic perturbations for a bouncing background gr-qc · 2026-05-15 · unverdicted · none · ref 1

    In an LQC bouncing cosmology, second-order quantum moments yield a Planck-suppressed scale-dependent correction δP_R ∝ (k ℓ_Pl)^6 to the curvature power spectrum together with post-bounce damping from gravitational moments.