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20242026
most citedScalar perturbations in a Top-Star spacetime

2 citations · 9 across the 13 of their papers we have counts for

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gr-qc2026

Radiative losses from unbound orbits at quadratic order in spin from MPM formalism

Donato Bini, Giorgio Di Russo

We study the spinning two-body system in the aligned spin case for hyperboliclike motions computing all radiative losses (at the 2PN absolute accuracy and including spin-squared co…

gr-qc2026

The radial action for massive particles in spherically symmetric geometries: Exact resummation at any PM order

Donato Bini, Giorgio Di Russo

We compute the massive particles radial action along hyperboliclike geodesics in various spherically symmetric spacetimes: the standard Schwarzschild spacetime, its -dimens…

gr-qc2026

5d Schwarzschild-Tangherlini spacetime: MST-like formalism for a Reduced Confluent Heun Equation

Donato Bini, Giorgio Di Russo, Veronica Fantini

We study the five-dimensional Schwarzschild-Tangherlini solution, with particular attention to its geodesic structure and massless scalar perturbations. In the probe limit, we pres…

gr-qc2026

Gravitational waveform from radial infall at the third-and-half Post-Newtonian order

Giorgio Di Russo, Donato Bini

We compute the gravitational waveform associated with a radially infalling particle in a Schwarzschild black hole working in the center-of-mass system and in a post-Newtonian (PN)…

gr-qc2026

Radial fall: the gravitational waveform up to the second-and-half Post-Newtonian order

Donato Bini, Giorgio Di Russo

We consider an application of the Multipolar Post Minkowskian formalism to the case of a two-body system in radial fall. We compute, within the post-Newtonian approximation, the as…

gr-qc2026★ 1 cited

Analytic self-force effects on radial infalling particles in the Schwarzschild spacetime: the radiated energy

Donato Bini, Giorgio Di Russo

We compute, at the first self force accuracy level, the radiated energy from a radially infalling particle released from rest in a Schwarzschild spacetime. We examine both the case…