arXiv · 2409.03723
Quantum Energy Density of Cosmic Strings with Nonzero Radius
Abstract
Zero-point fluctuations in the background of a cosmic string provide an opportunity to study the effects of topology in quantum field theory. We use a scattering theory approach to compute quantum corrections to the energy density of a cosmic string, using the "ballpoint pen" and "flowerpot" models to allow for a nonzero string radius. For computational efficiency, we consider a massless field in $2+1$ dimensions. We show how to implement precise and unambiguous renormalization conditions in the presence of a deficit angle, and make use of Kontorovich-Lebedev techniques to rewrite the sum over angular momentum channels as an integral on the imaginary axis.
Explore related subjects
Keep this discovery
M. Koike, X. Laquidain, N. Graham. 2024-09-05. Quantum Energy Density of Cosmic Strings with Nonzero Radius. https://doi.org/10.1103/physrevd.110.105009
Cite the original work for its findings. Save a collection to share your selection of sources.