Structure Formation in the Quintessential Universe

Details Structure Formation in the Quintessential Universe Structure Formation in the Quintessential Universe

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001acppb..32.3643l&link_type=abstract

Acta Physica Polonica B, 32, 3643-3654

Physics

13

Scientific paper

I review the main characteristics of structure formation in the quintessential Universe. Assuming equation of state w=const I provide a brief description of the background cosmology and discuss the linear growth of density perturbations, the strongly nonlinear evolution, the power spectra and r.m.s. fluctuations as well as mass functions focusing on the three values w=-1, -2/3 and -1/3. Finally I describe the presently available and future constraints on w.

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