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Quantum Noise of Gravitons and Stochastic Force on Geodesic Separation

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arxiv 2112.08174 v2 pith:W5JQTUBQ submitted 2021-12-15 gr-qc astro-ph.COhep-thquant-ph

classification gr-qcastro-ph.COhep-thquant-ph
keywords gravitonsfluctuationsgravitonnoisequantumseparationstochasticforce
verification ladder T0 review T1 audit T2 compute T3 formal
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In this work we consider the effects of gravitons and their fluctuations on the dynamics of two masses using the Feynman-Vernon influence functional formalism, applied to nonequilibrium quantum field theory and semiclassical stochastic gravity earlier by Calzetta, Hu and Verdaguer [1-3], and most recently, to this problem by Parikh, Wilczek and Zahariade [4-6]. The Hadamard function of the gravitons yields the noise kernel acting as a stochastic tensorial force in a Langevin equation governing the motion of the separation of the two masses. The fluctuations of the separation due to the graviton noise are then solved for various quantum states including the Minkowski vacuum, thermal, coherent and squeezed states. The previous considerations of Parikh et al. are only for some selected modes of the graviton, while in this work we have included all graviton modes and polarizations. We comment on the possibility of detecting these fluctuations in primordial gravitons using interferometors with long baselines in deep space experiments.

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Cited by 3 Pith papers

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

  1. Suppressed Quantum Effects of Weakly Coupled Waves

    hep-ph 2026-07 conditional novelty 7.0 of 10

    Nonclassical (quantum) signatures of weakly coupled waves are suppressed by an extra power of the tiny conversion efficiency η (~10^-21 for axions, ~10^-33 for gravitons), so experiments cannot establish the quantizat...

  2. Geometric noise spectrum in interferometers

    hep-th 2026-01 conditional novelty 6.0 of 10

    The noise spectrum an interferometer would see from quantum spacetime jitter is computed for vacuum, thermal, squeezed, and scalar-backreaction states; all are Planck-suppressed.

  3. Geometric noise spectrum in interferometers

    hep-th 2026-01 unverdicted novelty 5.0 of 10

    Computes UV-finite noise spectra in interferometers from graviton fluctuations in vacuum/thermal/squeezed states and from massless scalar vacuum stress-energy, all Planck-suppressed.

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