| | Structure formation with a self-tuning scalar field (Site not responding. Last check: 2007-10-21) |
 | | A scalar field with an exponential potential has the particular property that it is attracted into a solution in which its energy scales as the dominant component (radiation or matter) of the Universe, contributing a fixed fraction of the total energy density. |
 | | We study the growth of perturbations in a flat CDM dominated universe with this extra field, with an initial flat spectrum of adiabatic fluctuations. |
 | | The observational constraints from structure formation are satisfied as well, or better, than in other models, with approximately 10% of the energy density in the scalar field, which is small enough to be consistent with entry into the attractor prior to nucleosynthesis. |
| www.maths.tcd.ie /report_series/abstracts/tcdm9710.html (108 words) |