Phantom energy from graded algebras
arXiv:hep-th/0603160 · doi:10.1142/S0217732307022372
Abstract
We construct a model of phantom energy using the graded Lie algebra SU(2/1). The negative kinetic energy of the phantom field emerges naturally from the graded Lie algebra, resulting in an equation of state with w<-1. The model also contains ordinary scalar fields and anti-commuting (Grassmann) vector fields which can be taken as two component dark matter. A potential term is generated for both the phantom fields and the ordinary scalar fields via a postulated condensate of the Grassmann vector fields. Since the phantom energy and dark matter arise from the same Lagrangian the phantom energy and dark matter of this model are coupled via the Grassman vector fields. In the model presented here phantom energy and dark matter come from a gauge principle rather than being introduced in an ad hoc manner.
8 pages no figures; references added and discussion on condensate of vector grassman fields added. To be published MPLA
References in corpus (38)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Cosmological parameters from SDSS and WMAP
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- Quintessence, Cosmic Coincidence, and the Cosmological Constant
- An alternative to quintessence
- New Constraints on , , and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
- Dark Energy Constraints from the Cosmic Age and Supernova
- Accelerated Universe from Gravity Leaking to Extra Dimensions
- Inhomogeneous Equation of State of the Universe: Phantom Era, Future Singularity and Crossing the Phantom Barrier
- The phantom menaced: constraints on low-energy effective ghosts
- Can dark energy evolve to the Phantom?
- Phantom energy traversable wormholes
- Dark Matter and Dark Energy
- Wormholes supported by a phantom energy
- The State of the Dark Energy Equation of State
- Oscillating Quintom and the Recurrent Universe
- Observational constraints on low redshift evolution of dark energy: How consistent are different observations?
- Perturbations of the Quintom Models of Dark Energy and the Effects on Observations
- K-Essential Phantom Energy: Doomsday around the corner?
- On the Significance of the Quantity "A Squared"
- Vacuum condensate of mass dimension 2 as the origin of mass gap and quark confinement
- On a class of stable, traversable Lorentzian wormholes in classical general relativity
- Probing the dark side: Constraints on the dark energy equation of state from CMB, large scale structure and Type Ia supernovae
- Dark matter: A spin one half fermion field with mass dimension one?
- Supernovae, CMB, and Gravitational Leakage into Extra Dimensions
- On the Emerging Phenomenology of <(A_μ)^2>
- Testing Landau gauge OPE on the Lattice with a Condensate
- The Case for an Accelerating Universe from Supernovae
- Constraints on Oscillating Quintom from Supernova, Microwave Background and Galaxy Clustering
- Consistent OPE Description of Gluon Two- and Three-point Green Function?
- Axion Phantom Energy
- Smooth dynamical (de)-phantomization of a scalar field in simple cosmological models
- A determination of <A^2> and the non-perturbative vacuum energy of Yang-Mills theory in the Landau gauge
- Description of Gluon Propagation in the Presence of an A^2 Condensate
- Ginzburg - Landau equation from SU(2) gauge field theory
- Effective 't Hooft-Polyakov monopoles from pure SU(3) gauge theory