Edward Anderson
Universite Paris 7 - Denis Diderot
Project Title
The Problem of Time in Quantum Gravity
Project Summary
Quantum gravity is required when two of 20th century physics' most spectacular successes both apply: quantum theory and Einstein's general relativity. Unfortunately, these individually successful theories fail to be compatible with each other! Some physicists (myself included) expect this to be related to how these theories have different (and incompatible) notions of what time is. Quantum general relativity's equations look frozen: ie featuring no time notion at all! Physicists then try to find a time hidden within, or a time that emerges under certain circumstances (eg when the whole universe is near-classical rather than more bizarre quantum possibilities), or see how much of physics can actually be done in timeless terms (e.g. correlations within a given snapshot). None of these strategies so far work in detail, so I propose combining three that look to reinforce each other: near-classicality, timeless snapshots and consideration of universe-histories. All this being too hard to calculate for full general relativity, I use simpler models that happen to capture most of the features of general relativity essential to these strategies: the triangle and quadrilateral of particles studied without reference to Newtonian background time and space since general relativity pointedly has none of these.
Technical Abstract
Quantum gravity involves quantum theory and general relativity at once. Unfortunately 'time' means something different in each of these theories, and so there is a "problem of time" due to this incompatibility. In particular, the quantum general relativity equations come out as frozen. Some approaches to try to get round this involve time only becoming meaningful in the semiclassical regime, purely timeless considerations and thinking in terms of histories of the universe. None of these approaches are conclusive, but these particular three approaches look to support each other, and as such I wish to produce a more robust problem of time strategy out of their combination (expanding on pioneering work by Halliwell). Relational particle models, i.e. particle mechanics in which only relative times, relative separations and relative angles are meaningful, originally due to Barbour and Bertotti, are particularly suitable toy models for this investigation. I will use in particular the triangle and quadrilateral formed by particles in 2d. These suffice to mirror many of the relevant features of general relativity, whilst I have demonstrated that they have the great advantage of being mathematically straightforward to treat: S^2 and CP^2 mathematics and the cones over these.
Hide Technical Abstract
Quantum gravity involves quantum theory and general relativity at once. Unfortunately 'time' means something different in each of these theories, and so there is a "problem of time" due to this incompatibility. In particular, the quantum general relativity equations come out as frozen. Some approaches to try to get round this involve time only becoming meaningful in the semiclassical regime, purely timeless considerations and thinking in terms of histories of the universe. None of these approaches are conclusive, but these particular three approaches look to support each other, and as such I wish to produce a more robust problem of time strategy out of their combination (expanding on pioneering work by Halliwell). Relational particle models, i.e. particle mechanics in which only relative times, relative separations and relative angles are meaningful, originally due to Barbour and Bertotti, are particularly suitable toy models for this investigation. I will use in particular the triangle and quadrilateral formed by particles in 2d. These suffice to mirror many of the relevant features of general relativity, whilst I have demonstrated that they have the great advantage of being mathematically straightforward to treat: S^2 and CP^2 mathematics and the cones over these.
Hide Technical Abstract
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