Continuous self-similar evaporation of a rotating cosmic string loop
arXiv:0812.2523 · doi:10.1088/0264-9381/26/2/025006
Abstract
A solution of the linearized Einstein and Nambu-Goto equations is constructed which describes the evaporation of a certain type of rotating cosmic string - the Allen-Casper-Ottewill loop - under the action of its own self-gravity. The solution evaporates self-similarly, and radiates away all its mass-energy and momentum in a finite time. Furthermore, the corresponding weak-field metric can be matched to a remnant Minkowski spacetime at all points on the future light cone of the final evaporation point of the loop.
80 pages, 13 figures. Accepted for publication in Classical and Quantum Gravity
References in corpus (13)
- Cosmological evolution of cosmic string loops
- Fractal Properties and Small-scale Structure of Cosmic String Networks
- Scaling of cosmic string loops
- Scaling and Small Scale Structure in Cosmic String Networks
- Cosmic String Structure at the Gravitational Radiation Scale
- Cosmic String Loops, Large and Small
- A Closed-Form Expression for the Gravitational Radiation Rate from Cosmic Strings
- Gravitational Perturbations of Relativistic Membranes and Strings
- Analytic Results for the Gravitational Radiation from a Class of Cosmic String Loops
- Non-divergence of gravitational self-interactions for Goto-Nambu strings
- Cosmic string loops: large and small, but not tiny
- A reformulation of the Barrabes-Israel null-shell formalism
- Self-Similar Evaporation of a Rigidly-Rotating Cosmic String Loop