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20022026
most citedSecond Order Scalar Invariants of the Riemann Tensor: Applications to Black Hole Spacetimes

112 citations · 1.2k across the 49 of their papers we have counts for

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Showing 2004Show all

8 papers · 1 filter

gr-qc2004★ 9 cited

Spinning particles in the vacuum C metric

Donato Bini, Christian Cherubini, Andrea Geralico +1

The motion of a spinning test particle given by the Mathisson-Papapetrou equations is studied on an exterior vacuum C metric background spacetime describing the accelerated motion…

gr-qc2004★ 2 cited

Inertial effects of an accelerating black hole

D. Bini, C. Cherubini, B. Mashhoon

We consider the static vacuum C metric that represents the gravitational field of a black hole of mass undergoing uniform translational acceleration such that $mA<1/(3\sqrt…

gr-qc2004★ 11 cited

The Speciality Index as invariant indicator in the BKL Mixmaster Dynamics

Christian Cherubini, Donato Bini, Marco Bruni +1

The speciality index, which has been mainly used in Numerical Relativity for studying gravitational waves phenomena as an indicator of the special or non-special Petrov type charac…

gr-qc2004★ 5 cited

Geometric transport along circular orbits in stationary axisymmetric spacetimes

Donato Bini, Christian Cherubini, Gianluca Cruciani +1

Parallel transport along circular orbits in orthogonally transitive stationary axisymmetric spacetimes is described explicitly relative to Lie transport in terms of the electric an…

gr-qc2004★ 32 cited

Spin, Acceleration and Gravity

Donato Bini, Christian Cherubini, Bahram Mashhoon

The massless field perturbations of the accelerating Minkowski and Schwarzschild spacetimes are studied. The results are extended to the propagation of the Proca field in Rindler s…

gr-qc2004★ 18 cited

Petrov classification of perturbed spacetimes: the Kasner example

Christian Cherubini, Donato Bini, Marco Bruni +1

In this paper we consider vacuum Kasner spacetimes, focusing on those that can be parametrized as linear perturbations of the special Petrov type D case. For these quasi-D Kasner m…