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Dynamical system analysis of interacting models

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arxiv 1704.07825 v2 pith:TVMUT2UB submitted 2017-04-25 gr-qc astro-ph.COhep-th

classification gr-qcastro-ph.COhep-th
keywords analysiscreationcriticaldynamicalfuturelimitmatterminkowski
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We perform a dynamical system analysis of a cosmological model with linear dependence between the vacuum density and the Hubble parameter, with constant-rate creation of dark matter. We show that the de Sitter spacetime is an asymptotically stable critical point, future limit of any expanding solution. Our analysis also shows that the Minkowski spacetime is an unstable critical point, which eventually collapses to a singularity. In this way, such a prescription for the vacuum decay not only predicts the correct future de Sitter limit, but also forbids the existence of a stable Minkowski universe. We also study the effect of matter creation on the growth of structures and their peculiar velocities, showing that it is inside the current errors of redshift space distortions observations.

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Cited by 1 Pith paper

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

  1. Quasar cosmology II: joint analyses with Cosmic Microwave Background

    astro-ph.CO 2025-06 conditional novelty 6.0 of 10

    Quasar, supernova, BAO, DES, and CMB data are jointly compatible only in an interacting dark-energy model, not in Lambda-CDM, wCDM, or CPL.

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