Nonchaotic evolution of triangular configuration due to gravitational radiation reaction in the three-body problem

Understand

Continuing work initiated in an earlier publication [H.

• Asada, Phys.
• Rev.
• D {\bf 80}, 064021 (2009)], the gravitational radiation reaction to Lagrange's equilateral triangular solution of the three-body problem is investigated in an analytic method.