Abstract (EN):
We study the dependence of the location of the cosmic microwave background radiation peaks on the parameters of the generalized Chaplygin gas model, whose equation of state is given by p=-A/rho(alpha), where A is a positive constant and 0<alphaless than or equal to1. We find, in particular, that observational data arising from Archeops, BOOMERANG, supernova and high-redshift observations allow constraining significantly the parameter space of the model. Our analysis indicates that the emerging model is clearly distinguishable from the alpha=1 Chaplygin case and the LambdaCDM model.
Language:
English
Type (Professor's evaluation):
Scientific
No. of pages:
5