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Cited by 530

The DOI matches its Crossref record; 4 of the 4 references it cites were found in a registry or an index.

Interacting quintessence solution to the coincidence problem

Open access
Chimento, Luis P., Jakubi, Alejandro S., Pavón, Diego, Zimdahl, Winfried·2003·Physical Review D

Abstract

We show that a suitable interaction between a scalar field and a matter fluid in a spatially homogeneous and isotropic spacetime can drive the transition from a matter dominated era to an accelerated expansion phase and simultaneously solve the coincidence problem of our present Universe. For this purpose we study the evolution of the energy density ratio of these two components. We demonstrate that a stationary attractor solution is compatible with an accelerated expansion of the Universe. We extend this study to account for dissipation effects due to interactions in the dark matter fluid. Finally, type Ia supernovae and primordial nucleosynthesis data are used to constrain the parameters of the model.

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Crossref · 10.1103/physrevd.67.083513

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Metadata

Authors
Chimento, L. P., Jakubi, A. S., Pavón, D., & Zimdahl, W.
Venue
Physical Review D
Published
2003-04-24
Volume
67
Issue
8
ISSN
  • 0556-2821 (ISSN-L)
  • 1089-4918
OpenAlex
W2153527788
Cited by
530
References
4
FWCI
11.21
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Interacting quintessence solution to the coincidence problem. https://app.cochat.ai/papers/10.1103/physrevd.67.083513
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Chimento, L. P., Jakubi, A. S., Pavón, D., & Zimdahl, W. (2003). Interacting quintessence solution to the coincidence problem. Physical Review D. https://doi.org/10.1103/physrevd.67.083513

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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.