Angular momentum of zero-frequency gravitons

被引:32
作者
Di Vecchia, Paolo [1 ,2 ,3 ]
Heissenberg, Carlo [2 ,3 ,4 ]
Russo, Rodolfo [5 ]
机构
[1] Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark
[2] KTH Royal Inst Technol, NORDITA, Hannes Alfvens Vag 12, SE-11419 Stockholm, Sweden
[3] Stockholm Univ, Hannes Alfvens Vag 12, SE-11419 Stockholm, Sweden
[4] Uppsala Univ, Dept Phys & Astron, Box 516, SE-75120 Uppsala, Sweden
[5] Queen Mary Univ London, Ctr Theoret Phys, Dept Phys & Astron, Mile End Rd, London E1 4NS, England
基金
英国科学技术设施理事会;
关键词
Black Holes; Classical Theories of Gravity; Scattering Amplitudes; Supergravity Models; GRAVITATIONAL-WAVES; BREMSSTRAHLUNG; GENERATION; DERIVATION; PHOTONS;
D O I
10.1007/JHEP08(2022)172
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
By following closely Weinberg's soft theorem, which captures the 1/omega pole contribution to the amplitude for soft graviton emissions (omega < Lambda on top of an arbitrary background hard process, we calculate the expectation value of the graviton's angular momentum operator for arbitrary collisions dressed with soft radiation. We find that the result becomes independent of the cutoff Lambda on the graviton's frequency, effectively localizing at omega = 0. In this way, our result captures the contribution to the angular momentum that comes from the zero-frequency modes. Like the soft theorem, our formula has an exact dependence on the kinematics of the hard particles and is only a function of their momenta. As an example, we discuss in some detail the case of the 2 -> 2 scattering of spinless particles in General Relativity and N = 8 supergravity.
引用
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页数:25
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