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A First-Quantized Formalism for Cosmological Particle Production

2003/11/30 by Alex Hamilton, Alex J. Hamilton, Daniel Kabat +2 · 1 citation
Physics and Astronomy · #Cosmology and Gravitation Theories #Noncommutative and Quantum Gravity Theories #Quantum Electrodynamics and Casimir Effect #astro-ph #gr-qc #hep-th

paper · pdf · doi:10.1088/1126-6708/2004/07/024

published as JHEP0407:024,2004 · 18 pages, LaTeX; v2: significantly revised for clarity; conclusions unchanged

arxiv created 2004/05/12 · openalex publication_date 2004/07/14 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/01

Abstract

We show that the amount of particle production in an arbitrary cosmological background can be determined using only the late-time positive-frequency modes. We don't refer to modes at early times, so there is no need for a Bogolubov transformation. We also show that particle production can be extracted from the Feynman propagator in an auxiliary spacetime. This provides a first-quantized formalism for computing particle production which, unlike conventional Bogolubov transformations, may be amenable to a string-theoretic generalization.

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