English

Quantum Indeterminacy of Emergent Spacetime

General Relativity and Quantum Cosmology 2007-10-28 v2 Astrophysics High Energy Physics - Theory

Abstract

It is shown that nearly-flat 3+1D spacetime emerging from a dual quantum field theory in 2+1D displays quantum fluctuations from classical Euclidean geometry on macroscopic scales. A covariant holographic mapping is assumed, where plane wave states with wavevector k on a 2D surface map onto classical null trajectories in the emergent third dimension at an angle \theta=l_P k relative to the surface element normal, where l_P denotes the Planck length. Null trajectories in the 3+1D world then display quantum uncertainty of angular orientation, with standard deviation \Delta\theta=\sqrt{l_P/z} for longitudinal propagation distance z in a given frame. The quantum complementarity of transverse position at macroscopically separated events along null trajectories corresponds to a geometry that is not completely classical, but displays observable holographic quantum noise. A statistical estimator of the fluctuations from Euclidean behavior is given for a simple thought experiment based on measured sides of triangles. The effect can be viewed as sampling noise due to the limited degrees of freedom of such a theory, consistent with covariant bounds on entropy.

Keywords

Cite

@article{arxiv.0710.4153,
  title  = {Quantum Indeterminacy of Emergent Spacetime},
  author = {Craig J. Hogan},
  journal= {arXiv preprint arXiv:0710.4153},
  year   = {2007}
}
R2 v1 2026-06-21T09:34:52.756Z