activity
20122016
most citedRadial accretion flows on static spherically symmetric black holes

55 citations · 158 across the 6 of their papers we have counts for

collaborators

6 papers

gr-qc2016★ 28 cited

Black holes in nonlinear electrodynamics: quasi-normal spectra and parity splitting

Eliana Chaverra, Juan Carlos Degollado, Claudia Moreno +1

We discuss the quasi-normal oscillations of black holes which are sourced by a nonlinear electrodynamic field. While previous studies have focused on the computation of quasi-norma…

gr-qc2015★ 24 cited

Michel accretion of a polytropic fluid with adiabatic index gamma > 5/3: Global flows versus homoclinic orbits

Eliana Chaverra, Patryk Mach, Olivier Sarbach

We analyze the properties of a polytropic fluid which is radially accreted into a Schwarzschild black hole. The case where the adiabatic index gamma lies in the range 1 < gamma <=…

gr-qc2015★ 3 cited

Quasi-normal acoustic oscillations in the transonic Bondi flow

Eliana Chaverra, Olivier Sarbach

In recent work, we analyzed the dynamics of spherical and nonspherical acoustic perturbations of the Michel flow, describing the steady radial accretion of a relativistic perfect f…

gr-qc2015★ 55 cited

Radial accretion flows on static spherically symmetric black holes

Eliana Chaverra, Olivier Sarbach

We analyze the steady radial accretion of matter into a nonrotating black hole. Neglecting the self-gravity of the accreting matter, we consider a rather general class of static, s…

gr-qc2015★ 20 cited

Quasi-normal acoustic oscillations in the Michel flow

Eliana Chaverra, Manuel D. Morales, Olivier Sarbach

We study spherical and nonspherical linear acoustic perturbations of the Michel flow, which describes the steady radial accretion of a perfect fluid into a nonrotating black hole.…

gr-qc2012★ 28 cited

Linear perturbations of self-gravitating spherically symmetric configurations

Eliana Chaverra, Néstor Ortiz, Olivier Sarbach

We present a new covariant, gauge-invariant formalism describing linear metric perturbation fields on any spherically symmetric background in general relativity. The advantage of t…