Stationary dark energy: The Present universe as a global attractor
By Luca Amendola, D. Tocchini-Valentini. 2000
247 citations recorded by the source corpus.
We propose a cosmological model that makes a significant step toward solving the coincidence problem of the near similarity at the present of the dark energy and dark matter components. Our cosmology has the following properties: (a) among flat and homogeneous spaces, the present universe is a global attractor; all the possible initial conditions lead to the observed proportion of dark energy and dark matter; once reached, it remains fixed forever; (b) the expansion is accelerated at the present; (c) the model is consistent with the large-scale structure and microwave background data; (d) the dark energy and the dark matter densities scale similarly after equivalence and are close to within one order of magnitude.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/06499283fdbf6d8dcd2ed8b0f5bf48c0a08bda96
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In Astronomy and Astrophysics
- Yi Wang
- Shuang Wang
- Miao Li
- Emmanuel N. Saridakis
- Xin Zhang
- M. Setare
- Fotios Anagnostopoulos
- Ratbay Myrzakulov
In Nuclear and High Energy Physics
- Yi Wang
- Shuang Wang
- Miao Li
- Emmanuel N. Saridakis
- Xin Zhang
- M. Setare
- Fotios Anagnostopoulos
- Ratbay Myrzakulov
Citations in the corpus
- Holographic dark energy (2016, methodology): “Theoretical Studies for The IHDE Model The DE/DM interactions were first introduced to justify the currently small value of the cosmological constant [278, 279]; afterwards they were found to be very useful to alleviate the coincidence problem [280, 281, 282, 283].”