Uniformly accelerating observer in -deformed space-time
arXiv:1206.6179 · doi:10.1103/PhysRevD.86.045022
Abstract
In this paper, we study the effect of -deformation of the space-time on the response function of a uniformly accelerating detector coupled to a scalar field. Starting with -deformed Klein-Gordon theory, which is invariant under a -Poincaré algebra and written in commutative space-time, we derive -deformed Wightman functions, valid up to second order in the deformation parameter . Using this, we show that the first non-vanishing correction to the Unruh thermal distribution is only in the second order in . We also discuss various other possible sources of -dependent corrections to this thermal distribution.
12 pages, minor changes, to appear in Phys. Rev. D
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- Hawking radiation in the kappa-spacetime
- Uniformly accelerated detector in the -deformed Dirac vacuum
- Influence of the dispersion relation on the Unruh effect according to the relativistic Doppler shift method
- Quantisation of Klein-Gordon field in space-time: deformed oscillators and Unruh effect
- Time-space noncommutativity and Casimir effect
- Accelerated horizons and Planck-scale kinematics
- Effect of Non-commutativity of space-time on Thermodynamics of Photon gas
- Twisted Fermionic Oscillator Algebra in -Minkowski space-time
- Particle Dynamics and Lie-algebraic type of Non-commutativity of space-time
- Effect of Noncommutativity of Space-time on Zitterbewegung