Gravitational Bremsstrahlung and Hidden Supersymmetry of Spinning Bodies - INSPIRE

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Gravitational Bremsstrahlung and Hidden Supersymmetry of Spinning Bodies

Gustav Uhre Jakobsen
(
- Humboldt U., Berlin and
- Potsdam, Max Planck Inst.
)
,
Gustav Mogull
(
- Humboldt U., Berlin and
- Potsdam, Max Planck Inst.
)
,
Jan Plefka
(
- Humboldt U., Berlin
)
,
Jan Steinhoff
(
- Potsdam, Max Planck Inst.
)

Jun 18, 2021

7 pages

Published in:

Phys.Rev.Lett. 128 (2022) 1, 011101

Published: Jan 4, 2022

e-Print:

2106.10256 [hep-th]

DOI:

10.1103/PhysRevLett.128.011101 (publication)

Report number:

HU-EP-21/15-RTG

View in:

reference search149 citations

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Abstract: (APS)

The recently established formalism of a worldline quantum field theory, which describes the classical scattering of massive bodies (black holes, neutron stars, or stars) in Einstein gravity, is generalized up to quadratic order in spin, revealing an alternative

N = 2

supersymmetric description of the symmetries inherent in spinning bodies. The far-field time domain waveform of the gravitational waves produced in such a spinning encounter is computed at leading order in the post-Minkowskian (weak field, but generic velocity) expansion, and exhibits this supersymmetry. From the waveform we extract the leading-order total radiated angular momentum in a generic reference frame, and the total radiated energy in the center-of-mass frame to leading order in a low-velocity approximation.

Note:

7 pages + references, 2 figures

scattering: classical
supersymmetry: hidden symmetry
black hole: Kerr
bremsstrahlung
gravitational radiation
gravitation: weak field
general relativity
black hole: spin
black hole: angular momentum
field theory

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Figures(2)

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