Chaplygin gas with non-adiabatic perturbations
Abstract
Description
Perturbations in a Chaplygin gas, characterized by an equation of state $p = -A/ρ$, may acquire non-adiabatic contributions if spatial variations of the parameter $A$ are admitted. This feature is shown to be related to a specific internal structure of the Chaplygin gas. We investigate how perturbations of this type modify the adiabatic sound speed. A reduction of the effective sound speed compared with the adiabatic value is expected to suppress oscillations in the matter power spectrum. This text is an abridged version of the following reference: W. Zimdahl and J.C. Fabris, Classical and Quantum Gravity, {\bf 22}, 4311(2005).
Latex file, 10 pages. Submitted to the proceedings of the I Brazilian Workshop on Dark Energy/Matter
Latex file, 10 pages. Submitted to the proceedings of the I Brazilian Workshop on Dark Energy/Matter