A snapping cosmic string in a de Sitter or anti-de Sitter universe
J. Podolsky, J. B. Griffiths

TL;DR
This paper presents an exact solution to Einstein's equations depicting a snapping cosmic string in a universe with a cosmological constant, generating impulsive gravitational waves and connecting to known wave families.
Contribution
It introduces a new exact solution modeling a snapping cosmic string in de Sitter or anti-de Sitter space, linking it to Robinson-Trautman waves and the C-metric.
Findings
Solution describes impulsive spherical gravitational waves from a snapping string
Connects the solution to Robinson-Trautman and C-metric families
Provides geometric interpretation and various metric forms
Abstract
We present and describe an exact solution of Einstein's equations which represents a snapping cosmic string in a vacuum background with a cosmological constant . The snapping of the string generates an impulsive spherical gravitational wave which is a particular member of a known family of such waves. The global solution for all values of is presented in various metric forms and interpreted geometrically. It is shown to represent the limit of a family of sandwich type N Robinson-Trautman waves. It is also derived as a limit of the C-metric with , in which the acceleration of the pair of black holes becomes unbounded while their masses are scaled to zero.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
