2022
DOI: 10.48550/arxiv.2205.07701
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A Discrete Analog of General Covariance -- Part 2: Despite what you've heard, a perfectly Lorentzian lattice theory

Abstract: A crucial step in the history of General Relativity was Einstein's adoption of the principle of general covariance which demands a coordinate independent formulation for our spacetime theories. General covariance helps us to disentangle a theory's substantive content from its merely representational artifacts. It is an indispensable tool for a modern understanding of spacetime theories, especially regarding their background structures and symmetry. Motivated by quantum gravity, one may wish to extend these not… Show more

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Cited by 2 publications
(3 citation statements)
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“…We only expect detectors to be physically able to probe a finite number of modes within a given spatial region, and therefore, they can be used to define an operationally motivated cutoff to the field theory. This suggests that, from the point of view of detectors, even a continuous field theory with infinitely many degrees of freedom may behave as an effectively discretized chain of oscillators, up to the resolution allowed by the detectors [44,45,64].…”
Section: Discussionmentioning
confidence: 99%
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“…We only expect detectors to be physically able to probe a finite number of modes within a given spatial region, and therefore, they can be used to define an operationally motivated cutoff to the field theory. This suggests that, from the point of view of detectors, even a continuous field theory with infinitely many degrees of freedom may behave as an effectively discretized chain of oscillators, up to the resolution allowed by the detectors [44,45,64].…”
Section: Discussionmentioning
confidence: 99%
“…( 51) leads to couplings between the amplitudes at different sites, and therefore we see explicitly that the price we pay for imposing a UV cutoff is to have a non-local Hamiltonian, i.e., we need to give up locality. However, if we additionally perform an approximation of the derivative to nearest neighbors (see, for instance, [45]), we get that the field Hamiltonian reduces to…”
Section: The Continuum Limitmentioning
confidence: 99%
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