First-order formalism for the quintom model of dark energy
arXiv:0805.1117 · doi:10.1007/s10773-008-9757-3
Abstract
The present paper deals to the quintom model of dark energy. We introduce a first-order formalism, which shows how to relate the potential that specifies the scalar field model to Hubble parameter. Reviewing briefly the quintom scenario of dark energy, we present a general procedure to solve the equations of motion for quintom model driven by a couple scalar fields with first-order differential equations.
9 pages, 3 figures. To appear in IJTP (2008)
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