Scalar fields in numerical general relativity : inhomogeneous inflation and bubble collapse
Einstein’s field equation of General Relativity (GR) has been known for over 100 years, yet it remains challenging to solve analytically in strongly relativistic regimes, particularly where there is a lack of a priori symmetry. Numerical Relativity (NR) - the evolution of the Einstein Equations usin...
| Main Author: | |
|---|---|
| Other Authors: | |
| Published: |
King's College London (University of London)
2017
|
| Subjects: | |
| Online Access: | https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.718546 |