Generalized Chaplygin gas and cosmic microwave background radiation constraints
By M. C. Bento, O. Bertolami, A. A. Sen. 2003
201 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/bc0d9c06059d213e75955e53ae6c0ad9cd80d74f
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Citations in the corpus
- Cosmological constraints on f(R) gravity theories within the Palatini approach (2005, result): “…et al. 2005; Freese & Lewis 2002; Meng & Wang 2003; Dolgov & Kawasaki 2003; Shao et al. 2005; Gong et al. 2004; Lima 2004; Ahmed et al. 2004; Bento et al. 2002, 2003) have been proposed, and they can with some degree of success account for the observations (Lue et al. 2004a,b; Lue 2003;…”
- Generalized Chaplygin gas as a unified scenario of dark matter/energy: Observational constraints (2004, methodology): “Using the CMBR power spectrum measurements from BOOMERANG (de Bernardis et al. 2002) and Archeops (Benoit et al. 2003), together with the SNeIa constraints, Bento et al. (2003a) obtained, 0.74 ∼ < As ∼< 0.85, andα ∼< 0.6, which is comparable with our results.”
- Transition redshift: new kinematic constraints from supernovae (2008, background): “…the Chaplygin gas whose equation of state is given by p = −A/ρ where A is a positive constant (Kamenshchik et al. 2001; Bento et al. 2002; Dev et al. 2003; Bento et al. 2003; Cunha et al. 2004; Lima et al. 2006a,b), among others (Lima & Alcaniz 1999; Chimento et al. 2001; Freese & Lewis 2002;…”
- Latest supernova data in the framework of the generalized Chaplygin gas model (2004, methodology): “These results were in agreement with the WMAP data (Bento et al. 2003b).”