Quintom scenario
The Quintom scenario was proposed in 2004 by Xin-Min Zhang et al., and is a hypothetical model of dark energy. The name of 'quintom' was derived from 'quintessence' from quintessence field and 'phantom' from phantom dark energy. The Quintom scenario was to fit the evolution of dark energy with the cosmological data.
Equation of state
In this scenario, the equation of state of the dark energy, relating its pressure and energy density, can cross the boundary associated with the cosmological constant. The boundary separates the phantom-energy-like behavior with from the quintessence-like behavior with.According to a no-go theorem, a single-field, single-fluid scalar model cannot cross. Achieving such a crossing requires at least two degrees of freedom in dark energy models built from ideal fluids or scalar fields. To allow the effective equation of state to cross, possible approaches include:
- Multiple fields & extra degrees of freedom, e.g. additional scalar fields or fermion fields;
- Higher-order derivative terms, e.g. Galileon theory;
- Modified gravities, e.g.,, gravity, metric-affine theory, or Horndeski gravity;
- Matter-dark energy interactions, e.g. interacting dark sector;
- Extra dimension effects, e.g. DGP gravity.