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“…(4), we show the results from the lookback time-redshift (LT) data, which is very similar to the results obtained from the Sne Ia data [13]. The best-fit values are A s = 0.47 and α = −0.85.…”
Section: For the Gcg Model E(p) In The Friedmann Equation Now Has Thsupporting
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“…(4), we show the results from the lookback time-redshift (LT) data, which is very similar to the results obtained from the Sne Ia data [13]. The best-fit values are A s = 0.47 and α = −0.85.…”
Section: For the Gcg Model E(p) In The Friedmann Equation Now Has Thsupporting
“…Currently, works have been done on the CG and the GCG models [12] and many authors have attempted to constrain them by using various observational data, such as Sne Ia [13,14,15,16,17,18], the CMBR [18,19,20], the gamma-ray bursts [21], the gravitational lensing [15,17,22], the X-ray gas mass fraction of clusters [14,15,16], the large scale structure [18,23], the age of high-redshift objects [24], and the Hubble parameter versus redshift [25].…”
Section: Introductionmentioning
“…This is in agreement with previous, independent fits (e.g. [4] ) including the most recent ones [18]. We can say that our combined analysis constrains the generalized Chaplygin gas scenario to cases effectively equivalent to ΛCDM model.…”
Section: +072supporting
“…Alternatively, one may leave A as a free parameter to be determined by best-fitting models to observations (e.g., Wu & Yu 2007), in which case one obtains 0.6ρ…”
Section: Basic Propertiesmentioning