Randall-Sundrum brane cosmology: modification of late-time cosmic dynamics by exotic matter. (English) Zbl 1217.83055
Summary: We show, through the study of concrete examples, that depending on the cosmic dynamics of the energy density of matter degrees of freedom living in the brane, Randall-Sundrum (RS) brane effects can be important not only at short distances (UV regime), but also at large cosmological scales (IR regime). Our first example relies on the study, by means of the dynamical system tools, of a toy model based in a nonlinear electrodynamics (NLED) Lagrangian. Then we show that other, less elaborated models, such as the inclusion of a scalar phantom field, and of a tachyon phantom field-trapped in the brane-produce similar results. The form of the RS correction seems to convert what would have been future attractors in general relativity into saddle points. The above ‘mixing of scales’ effect is distinctive only of theories that modify the right-hand side (matter part) of the Friedmann equation, so that, for instance, Dvali-Gabadadze-Porrati-brane models do not show this feature.
MSC:
83F05 | Relativistic cosmology |
83E30 | String and superstring theories in gravitational theory |
81T30 | String and superstring theories; other extended objects (e.g., branes) in quantum field theory |
83D05 | Relativistic gravitational theories other than Einstein’s, including asymmetric field theories |
83C55 | Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) |
85A40 | Astrophysical cosmology |
83C75 | Space-time singularities, cosmic censorship, etc. |