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arxiv: 1310.0030 · v1 · submitted 2013-09-30 · 🌀 gr-qc · astro-ph.CO· hep-th

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On the Instability of Global de Sitter Space to Particle Creation

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classification 🌀 gr-qc astro-ph.COhep-th
keywords particlesittercreationglobalspacestatefieldphase
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We show that global de Sitter space is unstable to particle creation, even for a massive free field theory with no self-interactions. The O(4,1) de Sitter invariant state is a definite phase coherent superposition of particle and anti-particle solutions in both the asymptotic past and future, and therefore is not a true vacuum state. In the closely related case of particle creation by a constant, uniform electric field, a time symmetric state analogous to the de Sitter invariant one is constructed, which is also not a stable vacuum state. We provide the general framework necessary to describe the particle creation process, the mean particle number, and dynamical quantities such as the energy-momentum tensor and current of the created particles in both the de Sitter and electric field backgrounds in real time, establishing the connection to kinetic theory. We compute the energy-momentum tensor for adiabatic vacuum states in de Sitter space initialized at early times in global S^3 sections, and show that particle creation in the contracting phase results in exponentially large energy densities at later times, necessitating an inclusion of their backreaction effects, and leading to large deviation of the spacetime from global de Sitter space before the expanding phase can begin.

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

  1. The thermal backreaction of a scalar field in de Sitter spacetime. II. Spectrum enhancement and holography

    hep-th 2026-01 unverdicted novelty 5.0

    Thermal backreaction modifies de Sitter geometry so that late-exiting modes produce a blue-tilted spectrum n_S ~ 2 while the boundary theory matches the 3d Sp(N) model flow.