Dark energy from quantum fluctuations
Bogus{\l}aw Broda, Micha{\l} Szanecki

TL;DR
This paper derives a dynamic quantum vacuum pressure and energy density from quantum fluctuations, which can be incorporated into Einstein's equations to support models of dark energy.
Contribution
It introduces a novel derivation of quantum vacuum pressure and energy density as dynamical entities suitable for cosmological modeling.
Findings
Quantum vacuum pressure P_vac is derived as a primary, dynamical entity.
Quantum vacuum energy density G_vac is secondary but of expected order.
Both P_vac and G_vac can support holographic and thermodynamic dark energy models.
Abstract
We have derived the quantum vacuum pressure P_vac as a primary entity, removing a trivial and a gauge terms from the cosmological constant-like part (the zeroth term) of the effective action for a free matter field. The quantum vacuum energy density G_vac appears a secondary entity, but both are of expected order. Moreover P_vac and G_vac are dynamical, and therefore they can be used in the Einstein equations. In particular, they could dynamically support holographic dark energy model as well as the `thermodynamic' one.
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