Interacting models of soft coincidence

Sergio Del Campo, Ramón Herrera, Germán Olivares, Diego Pavón

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77 Citations (Scopus)

Abstract

The coincidence problem of late cosmic acceleration is a serious riddle in connection with our understanding of the evolution of the Universe. In this paper we show that an interaction between the dark energy component (either phantom or quintessence) and dark matter can alleviate it. In this scenario the baryon component is independently conserved. This generalizes a previous study in which neither baryons nor phantom energy were considered. © 2006 The American Physical Society.
Original languageEnglish
Article number023501
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume74
Issue number2
DOIs
Publication statusPublished - 12 Jul 2006

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    Del Campo, S., Herrera, R., Olivares, G., & Pavón, D. (2006). Interacting models of soft coincidence. Physical Review D - Particles, Fields, Gravitation and Cosmology, 74(2), [023501]. https://doi.org/10.1103/PhysRevD.74.023501