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Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

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3Does locality fail at intermediate length scales?R. D. SORKINAssuming that “quantum spacetime” is fundamentally discrete, how might this discretenessshow itself? Some of its potential effects are more evident, others less so.The a<strong>to</strong>mic and molecular structure of ordinary matter influences the propagationof both waves and particles in a material medium. Classically, particles can bedeflected by collisions and also retarded in their motion, giving rise in particular<strong>to</strong> viscosity and Brownian motion. In the case of spatio-temporal discreteness,viscosity is excluded by Lorentz symmetry, but fluctuating deviations from rectilinearmotion are still possible. Such “swerves” have been described in [1] and[2]. They depend (for a massive particle) on a single phenomenological parameter,essentially a diffusion constant in velocity space. As far as I know, the correspondinganalysis for a quantal particle with mass has not been carried out yet, but formassless quanta such as pho<strong>to</strong>ns the diffusion equation of [1] can be adapted <strong>to</strong>say something, and it then describes fluctuations of both energy and polarization(but not of direction), as well as a secular “reddening” (or its opposite). A morecomplete quantal s<strong>to</strong>ry, however, would require that particles be treated as wavepackets, raising the general question of how spatiotemporal discreteness affects thepropagation of waves. Here, the analogy with a material medium suggests effectssuch as scattering and extinction, as well as possible nonlinear effects. Further generalization<strong>to</strong> a “second-quantized field” might have more dramatic, if less obvious,consequences. In connection with cosmology, for example, people have wonderedhow discreteness would affect the hypothetical infla<strong>to</strong>n field.So far, I have been assuming that, although the deep structure of spacetime isdiscrete, it continues <strong>to</strong> respect the Lorentz transformations. That this is logicallypossible is demonstrated [3] by the example of causal set (causet) theory [4; 5; 6; 7].With approaches such as loop quantum gravity, on the other hand, the status of localLorentz invariance seems <strong>to</strong> be controversial. Some people have hypothesized thatit would be broken or at least perhaps deformed in such a way that the dispersionrelations for light would cease <strong>to</strong> be those of a massless field. Were this the case,<strong>Approaches</strong> <strong>to</strong> <strong>Quantum</strong> <strong>Gravity</strong>: Toward a New Understanding of Space, Time and Matter, ed. Daniele Oriti.Published by Cambridge University Press. c○ Cambridge University Press 2009.

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