Scattering Amplitudes and the Conservative Hamiltonian for Binary Systems at Third Post-Minkowskian Order

被引:399
作者
Bern, Zvi [1 ]
Cheung, Clifford [2 ]
Roiban, Radu [3 ]
Shen, Chia-Hsien [1 ]
Solon, Mikhail P. [2 ]
Zeng, Mao [4 ]
机构
[1] Univ Calif Los Angeles, Mani L Bhaumik Inst Theoret Phys, Los Angeles, CA 90095 USA
[2] CALTECH, Walter Burke Inst Theoret Phys, Pasadena, CA 91125 USA
[3] Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
[4] Swiss Fed Inst Technol, Inst Theoret Phys, CH-8093 Zurich, Switzerland
基金
瑞士国家科学基金会;
关键词
GRAVITATIONAL-RADIATION REACTION; MULTIPLE BREMSSTRAHLUNG; DIFFERENTIAL-EQUATIONS; TREE AMPLITUDES; PARTICLES; MOTION; APPROXIMATION; DYNAMICS; OBJECTS; FIELD;
D O I
10.1103/PhysRevLett.122.201603
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We present the amplitude for classical scattering of gravitationally interacting massive scalars at third post-Minkowskian order. Our approach harnesses powerful tools from the modern amplitudes program such as generalized unitarity and the double-copy construction, which relates gravity integrands to simpler gauge-theory expressions. Adapting methods for integration and matching from effective field theory, we extract the conservative Hamiltonian for compact spinless binaries at third post-Minkowskian order. The resulting Hamiltonian is in complete agreement with corresponding terms in state-of-the-art expressions at fourth post-Newtonian order as well as the probe limit at all orders in velocity. We also derive the scattering angle at third post-Minkowskian order and find agreement with known results.
引用
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页数:7
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