Effects of the interaction between dark energy and dark matter on cosmological parameters
By Jian-hua He, Bin Wang. 2008
224 citations recorded by the source corpus.
We examine the effects of possible phenomenological interactions between dark energy and dark matter on cosmological parameters and their efficiency in solving the coincidence problem. We work with two simple parameterizations of the dynamical dark energy equation of state and the constant dark energy equation of state. Using observational data coming from the new 182 Gold type Ia supernova samples, the shift parameter of the Cosmic Microwave Background given by the three-year Wilkinson Microwave Anisotropy Probe observations and the baryon acoustic oscillation measurement from the Sloan Digital Sky Survey, we perform a statistical joint analysis of different forms of phenomenological interaction between dark energy and dark matter.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/48cf00d844fe076ca642ad62b5949be825cf30c2
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- S. Vagnozzi
- E. di Valentino
- O. Mena
- A. Melchiorri
- Supriya Pan
- Weiqiang Yang
- A. Mukherjee
- R. Maartens
In Nuclear and High Energy Physics
- S. Vagnozzi
- E. di Valentino
- O. Mena
- A. Melchiorri
- Supriya Pan
- Weiqiang Yang
- A. Mukherjee
- R. Maartens
Citations in the corpus
- Observational constraints on an interacting dark energy model (2009, unknown): “…(2004); Chimento et al. (2003); Olivares et al. (2005); Koivisto (2005); Sadjadi & Alimohammadi (2006); Guo et al. (2007); Boehmer et al. (2008); He & Wang (2008); Quartin et al. (2008); Pereira & Jesus (2009); Quercellini et al. (2008); Valiviita et al. (2008); He et al. (2009); Bean et al.…”
- Interacting dark energy with time varying equation of state and the H0 tension (2018, background): “Some recent works on this direction are referred in [11, 33, 34, 35, 36, 37, 38].”
- Interacting scenarios with dynamical dark energy: Observational constraints and alleviation of the H0 tension (2019, unknown): “[14] J.”
- The growth of structure in interacting dark energy models (2009, background): “[7–28]).”
- Interacting dark energy in the early 2020s: A promising solution to the H0 and cosmic shear tensions (2019, background): “[130–239], for a recent comprehensive review see [200]).”
- Nonminimal dark sector physics and cosmological tensions (2019, unknown): “[147–194] and Ref.”