English

Plane wave holonomies in loop quantum gravity II: sine wave solution

General Relativity and Quantum Cosmology 2014-11-12 v2

Abstract

This paper constructs an approximate sinusoidal wave packet solution to the equations of loop quantum gravity (LQG). There is an SU(2) holonomy on each edge of the LQG simplex, and the goal is to study the behavior of these holonomies under the influence of a passing gravitational wave. The equations are solved in a small sine approximation: holonomies are expanded in powers of sines, and terms beyond sin2\sin^2 are dropped; also, fields vary slowly from vertex to vertex. The wave is unidirectional and linearly polarized. The Hilbert space is spanned by a set of coherent states tailored to the symmetry of the plane wave case. Fixing the spatial diffeomorphisms is equivalent to fixing the spatial interval between vertices of the loop quantum gravity lattice. This spacing can be chosen such that the eigenvalues of the triad operators are large, as required in the small sine limit, even though the holonomies are not large. Appendices compute the energy of the wave, estimate the lifetime of the coherent state packet, discuss coarse-graining, and determine the behavior of the spinors used in the U(N) SHO realization of LQG.

Keywords

Cite

@article{arxiv.1305.2599,
  title  = {Plane wave holonomies in loop quantum gravity II: sine wave solution},
  author = {Donald E. Neville},
  journal= {arXiv preprint arXiv:1305.2599},
  year   = {2014}
}

Comments

56 pages, LaTeX Much improved presentation. Material on coarse-graining and U(N) SHO formalism added

R2 v1 2026-06-22T00:15:06.218Z