Relativistic closed-form Hamiltonian for many-body gravitating systems in the post-Minkowskian approximation.
The Hamiltonian for a system of relativistic bodies interacting by their gravitational field is found in the post-Minkowskian approximation, including all terms linear in the gravitational constant. It is given in a surprisingly simple closed form as a function of canonical variables describing the bodies only. The field is eliminated by solving inhomogeneous wave equations, applying transverse-traceless projections, and using the Routh functional. By including all special relativistic effects our Hamiltonian extends the results described in classical textbooks of theoretical physics. As an application, the scattering of relativistic objects is considered.
Ledvinka
Tomás
T
Institute of Theoretical Physics, Faculty of Mathematics and Physics, Charles University, Prague, Czech Republic.
Schäfer
Gerhard
G
Bicák
Jirí
J