About Lorentz invariance in a discrete quantum setting
arXiv:gr-qc/0405085 · doi:10.1088/1126-6708/2004/06/050
Abstract
A common misconception is that Lorentz invariance is inconsistent with a discrete spacetime structure and a minimal length: under Lorentz contraction, a Planck length ruler would be seen as smaller by a boosted observer. We argue that in the context of quantum gravity, the distance between two points becomes an operator and show through a toy model, inspired by Loop Quantum Gravity, that the notion of a quantum of geometry and of discrete spectra of geometric operators, is not inconsistent with Lorentz invariance. The main feature of the model is that a state of definite length for a given observer turns into a superposition of eigenstates of the length operator when seen by a boosted observer. More generally, we discuss the issue of actually measuring distances taking into account the limitations imposed by quantum gravity considerations and we analyze the notion of distance and the phenomenon of Lorentz contraction in the framework of ``deformed (or doubly) special relativity'' (DSR), which tentatively provides an effective description of quantum gravity around a flat background. In order to do this we study the Hilbert space structure of DSR, and study various quantum geometric operators acting on it and analyze their spectral properties. We also discuss the notion of spacetime point in DSR in terms of coherent states. We show how the way Lorentz invariance is preserved in this context is analogous to that in the toy model.
25 pages, RevTeX
References in corpus (17)
- Relativity in space-times with short-distance structure governed by an observer-independent (Planckian) length scale
- Loop Quantum Gravity
- Spin Foam Models for Quantum Gravity
- QSD V : Quantum Gravity as the Natural Regulator of Matter Quantum Field Theories
- Loop quantum gravity and light propagation
- Quantization of Point Particles in 2+1 Dimensional Gravity and Space-Time Discreteness
- Lectures on Loop Quantum Gravity
- Quantum -Poincare in Any Dimensions
- Quantum symmetry, the cosmological constant and Planck scale phenomenology
- Spacetime geometry from algebra: spin foam models for non-perturbative quantum gravity
- De Sitter space as an arena for Doubly Special Relativity
- Doubly Special Relativity and de Sitter space
- 2+1 gravity and Doubly Special Relativity
- Reconcile Planck-scale discreteness and the Lorentz-Fitzgerald contraction
- Spectra of Length and Area in 2+1 Lorentzian Loop Quantum Gravity
- A Ponzano-Regge model of Lorentzian 3-Dimensional gravity
- The Case for Discrete Energy Levels of a Black Hole
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- Modern tests of Lorentz invariance
- Lorentz violation at high energy: concepts, phenomena and astrophysical constraints
- Interpretation of Quantum Field Theories with a Minimal Length Scale
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- Scalar Field Theory on Non-commutative Snyder Space-Time
- Modification of Heisenberg uncertainty relations in non-commutative Snyder space-time geometry
- The Free Particle in Deformed Special Relativity
- Snyder noncommutative space-time from two-time physics
- Towards Loop Quantum Gravity without the time gauge
- The Thiemann Complexifier and the CVH algebra for Classical and Quantum FLRW Cosmology
- Coupling gauge theory to spinfoam 3d quantum gravity
- Loop Quantum Gravity Phenomenology: Linking Loops to Observational Physics
- The Relativistic Particle: Dirac observables and Feynman propagator
- On the viability of Planck scale cosmology with quartessence
- Coherent States for 3d Deformed Special Relativity: semi-classical points in a quantum flat spacetime
- Non-Relativistic Anti-Snyder Model and Some Applications
- Lifshitz field theories, Snyder noncomutative space-time and momentum dependent metric
- Discrete Lorentz symmetry and discrete spacetime translational symmetry in two- and three-dimensional crystals
- Symmetries of the Dirac quantum walk and emergence of the de Sitter group