activity
20102021
most citedNext-to-next-to-leading order post-Newtonian linear-in-spin binary Hamiltonians

73 citations · 299 across the 8 of their papers we have counts for

collaborators

8 papers

cs.AI2021

Monte Carlo Tree Search for high precision manufacturing

Dorina Weichert, Felix Horchler, Alexander Kister +3

Monte Carlo Tree Search (MCTS) has shown its strength for a lot of deterministic and stochastic examples, but literature lacks reports of applications to real world industrial proc…

gr-qc2013

Recent progress in spin calculations in the post-Newtonian framework and applications

Johannes Hartung, Jan Steinhoff, Gerhard Schäfer

Recently we derived the next-to-next-to-leading order post-Newtonian Hamiltonians at spin-orbit and spin(1)-spin(2) level for a binary system of compact objects. In this talk the d…

gr-qc2013★ 73 cited

Next-to-next-to-leading order post-Newtonian linear-in-spin binary Hamiltonians

Johannes Hartung, Jan Steinhoff, Gerhard Schäfer

The next-to-next-to-leading order post-Newtonian spin-orbit and spin(1)-spin(2) Hamiltonians for binary compact objects in general relativity are derived. The Arnowitt-Deser-Misner…

gr-qc2012★ 30 cited

Aligned Spins: Orbital Elements, Decaying Orbits, and Last Stable Circular Orbit to high post-Newtonian Orders

Manuel Tessmer, Johannes Hartung, Gerhard Schäfer

In this article the quasi-Keplerian parameterisation for the case that spins and orbital angular momentum in a compact binary system are aligned or anti-aligned with the orbital an…

gr-qc2011★ 63 cited

Next-to-next-to-leading order post-Newtonian spin(1)-spin(2) Hamiltonian for self-gravitating binaries

Johannes Hartung, Jan Steinhoff

We present the next-to-next-to-leading order post-Newtonian (PN) spin(1)-spin(2) Hamiltonian for two self-gravitating spinning compact objects. If both objects are rapidly rotating…

gr-qc2011★ 64 cited

Next-to-next-to-leading order post-Newtonian spin-orbit Hamiltonian for self-gravitating binaries

Johannes Hartung, Jan Steinhoff

We present the next-to-next-to-leading order post-Newtonian (PN) spin-orbit Hamiltonian for two self-gravitating spinning compact objects. If at least one of the objects is rapidly…