Unified dark energy and dark matter from a scalar field different from quintessence
Changjun Gao, M. Kunz, Andrew R. Liddle, David Parkinson
Abstract
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Changjun Gao, M. Kunz, Andrew R. Liddle, David Parkinson
Abstract
Open-access reader
We explore unification of dark matter and dark energy in a theory containing a scalar field of non-Lagrangian type, obtained by direct insertion of a kinetic term into the energy-momentum tensor. This scalar is different from quintessence, having an equation of state between $\ensuremath{-}1$ and 0 and a zero sound speed in its rest frame. We solve the equations of motion for an exponential potential via a rewriting as an autonomous system, and demonstrate the observational viability of the scenario, for sufficiently small exponential potential parameter $\ensuremath{\lambda}$, by comparison to a compilation of kinematical cosmological data.
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We explore unification of dark matter and dark energy in a theory containing a scalar field of non-Lagrangian type, obtained by direct insertion of a kinetic term into the energy-momentum tensor. This scalar is different from quintessence, having an equation of state between $\ensuremath{-}1$ and 0 and a zero sound speed in its rest frame. We solve the equations of motion for an exponential potential via a rewriting as an autonomous system, and demonstrate the observational viability of the scenario, for sufficiently small exponential potential parameter $\ensuremath{\lambda}$, by comparison to a compilation of kinematical cosmological data.
Key concepts: Quintessence, Dark energy, Physics, Scalar field, Dark fluid, Scalar field dark matter, Kinetic term, Scalar (mathematics)