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Cited by 169

The DOI matches its Crossref record; 5 of the 5 references it cites were found in a registry or an index.

Primordial perturbations in a nonsingular bouncing universe model

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Peter, Patrick, Pinto-Neto, Nelson·2002·Physical Review D

Abstract

We construct a simple nonsingular cosmological model in which the currently observed expansion phase was preceded by a contraction. This is achieved, in the framework of pure general relativity, by means of a radiation fluid and a free scalar field having negative energy. We calculate the power spectrum of the scalar perturbations that are produced in such a bouncing model under the assumption of initial vacuum state for the quantum field associated with the hydrodynamical perturbation. The matching conditions applying to this bouncing model are derived and shown to be different from those in the case of a sharp transition. We show that if our bounce transition is smoothly connected to a slowly contracting phase, this provides a new way to generate a scale invariant power spectrum.

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Metadata

Authors
Peter, P., & Pinto-Neto, N.
Venue
Physical Review D
Published
2002-09-25
Volume
66
Issue
6
ISSN
  • 0556-2821 (ISSN-L)
  • 1089-4918
OpenAlex
W2156815396
Cited by
169
References
5
FWCI
8.25
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Primordial perturbations in a nonsingular bouncing universe model. https://app.cochat.ai/papers/10.1103/physrevd.66.063509
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Peter, P., & Pinto-Neto, N. (2002). Primordial perturbations in a nonsingular bouncing universe model. Physical Review D. https://doi.org/10.1103/physrevd.66.063509

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.