The small-scale structure of quantum spacetime
Planck-scale quantum spacetime undergoes probabilistic local curvature fluctuations whose distributions cannot explicitly depend on position otherwise vacuum's small-scale quantum structure would fail to be statistically homogeneous. Since the collection of fluctuations is a many-body system, t...
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Zusammenfassung: | Planck-scale quantum spacetime undergoes probabilistic local curvature
fluctuations whose distributions cannot explicitly depend on position otherwise
vacuum's small-scale quantum structure would fail to be statistically
homogeneous. Since the collection of fluctuations is a many-body system, the
natural explanation for their position-independent statistics is that they are
in equilibrium with each other and distributed at maximum entropy.
Consequently, their probability distributions obey the laws of statistical
physics which enforces small-scale smoothness, prevents the
homogeneity-violating diffusion found in any free quantum system, and maintains
decoherence. Their entropy, calculated using the explicitly-constructed phase
space of the Riemann whose statistics are derived using a
background-independent graviton exchange ensemble, is proportional to the
Einstein-Hilbert action evaluated on the macroscopic expected geometry and
includes a small, positive cosmological constant. Entropy maximization yields
quantum spacetime's Ehrenfest equations of motion which are identical to
Einstein's expectation-valued field equations. This background-independent
dynamical formulation reveals curvature fluctuation entropy as a source of
expansion and raises the possibility that matter's zero-point energy problem,
which is action-based and not energy shift invariant, may not be a problem
after all. |
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DOI: | 10.48550/arxiv.1203.5238 |