activity
20152023
most citedExploring the origin of moving groups and diagonal ridges by simulations of stellar orbits and birthplaces

31 citations · 132 across the 17 of their papers we have counts for

collaborators

27 papers

astro-ph.HE2023★ 12 cited

Astrophysical cloaking of a naked singularity

Ronaldo S. S. Vieira, Włodek Kluźniak

A massive naked singularity would be cloaked by accreted matter, and thus may appear to a distant observer as an opaque \mbox{(quasi-)}spherical surface of a fluid, not unlike that…

astro-ph.GA2023★ 2 cited

Envelopes for orbits around axially symmetric sources with spheroidal shape

Javier Ramos-Caro, Ronaldo S. S. Vieira

We introduce a method to obtain the envelopes of eccentric orbits in axially symmetric potentials, , endowed with -symmetry of reflection. By making the transformation $…

gr-qc2022★ 4 cited

Chaotic dynamics of a spinless axisymmetric extended body around a Schwarzschild black hole

Ricardo A. Mosna, Fernanda F. Rodrigues, Ronaldo S. S. Vieira

We investigate the long-term orbital dynamics of spinless extended bodies in Schwarzschild geometry, and show that periodic deviations from spherical symmetry in the shape of a tes…

nlin.CD2022

Homoclinic chaos in the Hamiltonian dynamics of extended test bodies

Ronaldo S. S. Vieira, Ricardo A. Mosna

There is a long tradition of studying chaotic trajectories in systems whose integrability is broken by means of an external perturbation. Here we explore a different route to chaos…

astro-ph.SR2022

Chaotic orbital dynamics of pulsating objects in dark matter halos

Ronaldo S. S. Vieira, Ricardo A. Mosna

Stellar pulsation is nowadays a widely understood subject. However, there has been no research about the effects of pulsations on the star's orbital dynamics throughout the galaxy.…

gr-qc2021★ 1 cited

Levitating atmospheres around naked singularities

Ronaldo S. S. Vieira, Włodek Kluźniak

For a wide class of spherically symmetric naked singularities there is a sphere within which gravity is effectively repulsive. In such spacetimes accreting matter cannot reach the…