Tachyon cosmology with non-vanishing minimum potential: a unified model

Abstract

We investigate the tachyon condensation process in the effective theory with non-vanishing minimum potential and its implications to cosmology. It is shown that the tachyon condensation on an unstable three-brane described by this modified tachyon field theory leads to lower-dimensional branes (defects) forming within a stable three-brane. Thus, in the cosmological background, we can get well-behaved tachyon matter after tachyon inflation, (partially) avoiding difficulties encountered in the original tachyon cosmological models. This feature also implies that the tachyon inflated and reheated universe is followed by a Chaplygin gas dark matter and dark energy universe. Hence, such an unstable three-brane behaves quite like our universe, reproducing the key features of the whole evolutionary history of the universe and providing a unified description of inflaton, dark matter and dark energy in a very simple single-scalar field model.

18 pp

References in corpus (8)

• Dynamics of dark energy
• Tachyon Dynamics in Open String Theory
• Gauge-invariant analysis of perturbations in Chaplygin gas unified models of dark matter and dark energy
• Overproduction of cosmic superstrings
• Caustic Formation in Tachyon Effective Field Theories
• Curvaton reheating in tachyonic inflationary models
• Inhomogeneous tachyon condensation
• Cosmological evolution of a D-brane