MG13 - Talk detail |
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Participant |
Yamada, Kei | |||||||
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Institution |
Hirosaki University - Bunkyou - Hirosaki - Aomori - Japan | |||||||
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Session |
AN1 |
Accepted |
Yes |
Order |
4 |
Time |
15:15 - 15:40 | |
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Talk |
Oral abstract |
Title |
Triangular solution to the general relativistic three-body problem | |||||
| Co-authors | Hideki Asada | |||||||
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Abstract |
We reexamine the post-Newtonian effects on Lagrange's equilateral triangular solution for three-body problem. For three finite masses, it is found that a general triangular configuration satisfies the post-Newtonian equation of motion in general relativity, if and only if it has the relativistic corrections to each side length. We mention also about a collinear solution to the general relativistic three-body problem. reference:[1] K. Yamada & H. Asada, PRD 82, 104019 (2010) [2] K. Yamada & H. Asada, PRD 83, 024040 (2011) [3] T. Ichita, K. Yamada, & H. Asada, PRD 83, 084026 (2011) |
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