Large scale structure and the generalised Chaplygin gas as dark energy

Details Large scale structure and the generalised Chaplygin gas as dark energy Large scale structure and the generalised Chaplygin gas as dark energy

2003-07-30

arxiv.org/abs/astro-ph/0307533v2

Phys.Rev.D69:023004,2004

Astronomy and Astrophysics

Astrophysics

6 pages, matches version accepted for publication in Phys.Rev.D (in press)

Scientific paper

10.1103/PhysRevD.69.023004

The growth of large scale structure is studied in a universe containing both cold dark matter (CDM) and generalized Chaplygin gas (GCg). GCg is assumed to contribute only to the background evolution of the universe while the CDM component collapses and forms structures. We present some new analytical as well as numerical results for linear and non-linear growth in such model. The model passes the standard cosmological distance test without the need of a cosmological constant (LCDM). But we find that the scenario is severely constrained by current observations of large scale structure. Any small deviations of the GCg parameters away from the standard Lambda dominated cosmology (LCDM) produces substantial suppression for the growth of structures.

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