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The computational status of physics

A computable formulation of quantum theory

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Abstract

According to the Church-Turing Thesis (CTT), effective formal behaviours can be simulated by Turing machines; this has naturally led to speculation that physical systems can also be simulated computationally. But is this wider claim true, or do behaviours exist which are strictly hypercomputational? Several idealised computational models are known which suggest the possibility of hypercomputation, some Newtonian, some based on cosmology, some on quantum theory. While these models’ physicality is debatable, they nonetheless throw into question the validity of extending CTT to include all physical systems. We consider the physicality of hypercomputational behaviour from first principles, by showing that quantum theory can be reformulated in a way that explains why physical behaviours can be regarded as ‘computing something’ in the standard computational state-machine sense. While this does not rule out the physicality of hypercomputation, it strongly limits the forms it can take. Our model also has physical consequences; in particular, the continuity of motion and arrow of time become theorems within the basic model.

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Notes

  1. Andréka et al. (2008) argue that the physical variant of CTT was first considered as far back as the 1930s.

  2. There is as yet no empirical evidence that Hawking radiation, the mechanism by which evaporation takes place, exists in Nature. However, the final stages of a primordial micro black hole’s evaporation should theoretically result in a burst of gamma-rays; one of the goals of the GLAST satellite, launched by NASA on 11th June 2008, is to search for such flashes.

  3. Integrating over a union of disjoint rectangles is the same as summing the component integrals: given any integrable function f(x, t) defined on a disjoint union \(R = \bigcup_{\alpha}{R_\alpha},\) we have \(\int_{R}{f} = \sum_{\alpha}{\int_{R_\alpha}{f}}.\)

  4. Strictly, only the internal points of the trajectory are required to lie in R. Either (or both) of the endpoints q I and q F can lie outside R, provided they are on its boundary.

  5. As explained in his 1965 Nobel Prize address, Feynman 1965 subsequently described anti-particles as particles moving ‘backwards in time’. In effect, our own approach adopts this temporal bi-directionality, and places it centre-stage.

  6. For example, suppose we know (from wave-equation methods, say) that P has amplitude η(x) to be at location \(x^\dagger = (x,t^\dagger),\) for each \(x {\in}X.\) A more intuitive solution might then be to take \(\langle{x^\dagger|y^\dagger }\rangle_{h}= {\eta(x^\dagger)}/{\eta(y^\dagger)}.\) This gives \(\langle{x^\dagger|x^\dagger}\rangle_{h}=1\) in agreement with the ‘classical amplitude’, but also provides information about the relative amplitudes of all other spatial locations at time \(t^\dagger.\)

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Acknowledgements

This research was supported in part by the EPSRC HyperNet project (Hypercomputation Research Network, grant number EP/E064183/1).

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Correspondence to Mike Stannett.

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Stannett, M. The computational status of physics. Nat Comput 8, 517–538 (2009). https://doi.org/10.1007/s11047-009-9115-2

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