Cross-correlations between quantum degrees of freedom are required for consistent effective dynamics in Brans-Dicke Bianchi I cosmology, smoothing bounces and keeping energy density finite.
We work in units where 16πG= 1 and setγ= 1 for simplicity
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Quantum Backreaction in Effective Brans-Dicke Bianchi I Cosmology
Cross-correlations between quantum degrees of freedom are required for consistent effective dynamics in Brans-Dicke Bianchi I cosmology, smoothing bounces and keeping energy density finite.