Abstract
We describe the computation of post-Minkowskian Hamiltonians in general relativity from scattering amplitudes. Using a relativistic Lippmann-Schwinger equation, we relate perturbative amplitudes of massive scalars coupled to gravity to the post-Minkowskian Hamiltonians of classical general relativity to any order in Newton's constant. We illustrate this by deriving a Hamiltonian for binary black holes without spin up to second order in the post-Minkowskian expansion and explicitly demonstrate the equivalence with the recently proposed method based on an effective field theory matching.
Originalsprog | Engelsk |
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Artikelnummer | 084040 |
Tidsskrift | Physical Review D |
Vol/bind | 100 |
Udgave nummer | 8 |
Antal sider | 8 |
ISSN | 2470-0010 |
DOI | |
Status | Udgivet - 18 okt. 2019 |