Non-commutative and commutative vacua effects in a scalar torsion scenario
arXiv:1506.08416 · doi:10.1016/j.physletb.2015.07.075
Abstract
In this work, the effects of non-commutative and commutative vacua on the phase space generated by a scalar field in a scalar torsion scenario are investigated. For both classical and quantum regimes, the commutative and non-commutative cases are compared. To take account the effects of non-commutativity, two well known non-commutative parameters, and are introduced. It should be emphasized, the effects of which is related to momentum sector has more key role in comparison to which is related to space sector. Also the different boundary conditions and mathematical interpretations of non-commutativity are explored.
10 pages, Accepted for publication in Physics Letters B (July/30/2015)
References in corpus (11)
- Dark torsion as the cosmic speed-up
- Modified teleparallel gravity: inflation without inflaton
- Einstein's Other Gravity and the Acceleration of the Universe
- Modified f(R) gravity consistent with realistic cosmology: from matter dominated epoch to dark energy universe
- "Teleparallel" Dark Energy
- Observational Constraints on Teleparallel Dark Energy
- Self-Gravitating Spherically Symmetric Solutions in Scalar-Torsion Theories
- Cosmology of F(T) gravity and k-essence
- Parameter and Solar System constraint in Chameleon Brans Dick Theory
- Ghost dark energy in model of gravity
- Late time acceleration in a non-commutative model of modified cosmology