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On leading order gravitational backreactions in de Sitter spacetime

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arxiv gr-qc/0604122 v2 pith:KG5AVEOD submitted 2006-04-28 gr-qc

classification gr-qc
keywords invariancesitterstatesfluctuationsgravitationalleadingorderquantum
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Backreactions are considered in a de Sitter spacetime whose cosmological constant is generated by the potential of scalar field. The leading order gravitational effect of nonlinear matter fluctuations is analyzed and it is found that the initial value problem for the perturbed Einstein equations possesses linearization instabilities. We show that these linearization instabilities can be avoided by assuming strict de Sitter invariance of the quantum states of the linearized fluctuations. We furthermore show that quantum anomalies do not block the invariance requirement. This invariance constraint applies to the entire spectrum of states, from the vacuum to the excited states (should they exist), and is in that sense much stronger than the usual Poincare invariance requirement of the Minkowski vacuum alone. Thus to leading order in their effect on the gravitational field, the quantum states of the matter and metric fluctuations must be de Sitter invariant.

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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. Crossed products and quantum reference frames: on the observer-dependence of gravitational entropy

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    Gravitational subregion entropy is observer-dependent: different quantum clocks produce different von Neumann algebras and different entropy functionals for the same global state.

  2. Linearization (in)stabilities and crossed products

    hep-th 2024-11 conditional novelty 6.0 of 10

    Second-order Taub charge constraints are justified as linearization stability conditions in spatially closed spacetimes, while in boundary or no-isometry cases the justification is weaker and depends on interest in se...

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