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We propose a method for numerical relativity in which the spatial grid is finite and no outer boundary condition is needed. As a "proof of concept" we implement this method… Click to show full abstract
We propose a method for numerical relativity in which the spatial grid is finite and no outer boundary condition is needed. As a "proof of concept" we implement this method for the case of a self-gravitating, spherically symmetric scalar field.
Keywords:
boundary method;
numerical relativity;
method numerical
Journal Title: Classical and Quantum Gravity
Year Published: 2020
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Journal Title: Classical and Quantum Gravity
Year Published: 2020
Link to full text (if available)
Share on Social Media: Sign Up to like & get
recommendations!