Late-time tails of wave maps coupled to gravity
We consider the late-time asymptotic behavior for solutions of Einstein's equations with the wave map matter. Using the third-order perturbation expansion about the flat spacetime we show that solutions starting from small compactly supported -equivariant initial data with >= 1 decay as t-(2...
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Veröffentlicht in: | Classical and quantum gravity 2009-11, Vol.26 (22), p.225015-225015 (10) |
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Hauptverfasser: | , , , |
Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | We consider the late-time asymptotic behavior for solutions of Einstein's equations with the wave map matter. Using the third-order perturbation expansion about the flat spacetime we show that solutions starting from small compactly supported -equivariant initial data with >= 1 decay as t-(2+2) at future timelike infinity and as u-(+1) at future null infinity. |
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ISSN: | 0264-9381 1361-6382 |
DOI: | 10.1088/0264-9381/26/22/225015 |