Computation of the quadrupolar bremsstrahlung waveform for two-body scattering at 3.5PN order, including frequency-domain evaluation up to O(G^4) and nonlinear memory effects.
Higher-order tail contribu- tions to the energy and angular momentum fluxes in a two-body scattering process
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
fields
gr-qc 2years
2026 2roles
background 1polarities
background 1representative citing papers
First-order self-force analytic result for the total radiated energy of a radial infall from rest in Schwarzschild spacetime, for scalar and gravitational cases.
citing papers explorer
-
Quadrupolar bremsstrahlung waveform at the third-and-a-half post-Newtonian accuracy
Computation of the quadrupolar bremsstrahlung waveform for two-body scattering at 3.5PN order, including frequency-domain evaluation up to O(G^4) and nonlinear memory effects.
-
Analytic self-force effects on radial infalling particles in the Schwarzschild spacetime: the radiated energy
First-order self-force analytic result for the total radiated energy of a radial infall from rest in Schwarzschild spacetime, for scalar and gravitational cases.