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Quantum origin of suppression for vacuum fluctuations of energy

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arxiv 1406.3046 v4 pith:E72O5KW7 submitted 2014-06-10 gr-qc hep-th

classification gr-qchep-th
keywords energydensityfieldaveragecosmologicaldescribeexampleexponentially
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By example of a model with a spatially global scalar field, we show that the energy density of zero-point modes is exponentially suppressed by an average number of field quanta in a finite volume with respect to the energy density in the stationary state of minimal energy. We describe cosmological implications of mechanism.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Cosmological Constant Suppression in Non-Stationary Scalar Covariant State

    hep-th 2024-11 reject novelty 4.0 of 10

    The vacuum energy density is claimed to be ρ = (1/8) m Λ^3 e^{-<n>}, matching the observed cosmological constant when <n> ≈ 250 and m ≈ Λ ≈ 10^16 GeV.

  2. Scalar Field Action under 4D Isotropic Cut-off and its Cosmological Impact

    hep-th 2025-01 reject novelty 3.0 of 10

    A scalar field with a 4D isotropic cutoff reduces to a 1D harmonic oscillator with vacuum energy (1/8)mΛ³, which the authors link to the observed dark energy scale via an exponential suppression factor.

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