Remarks on numerical relativity, geodesic motions, binary neutron star evolution
The computations of numerical relativity make use of (3+1)- decompositions of Einstein field equations. We examine the conceptual characteristics of this method; instances of compact-star binaries are considered. The preeminent role of the geodesic motions is emphasized.
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| Format: | Artikel |
| Sprache: | eng |
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| Zusammenfassung: | The computations of numerical relativity make use of (3+1)- decompositions of
Einstein field equations. We examine the conceptual characteristics of this
method; instances of compact-star binaries are considered. The preeminent role
of the geodesic motions is emphasized. |
|---|---|
| DOI: | 10.48550/arxiv.1211.6152 |