activity
20152020
most citedA spine-sheath model for strong-line blazars

38 citations · 76 across the 7 of their papers we have counts for

collaborators

7 papers

gr-qc2020★ 6 cited

The problem of ultracompact rotating gravastars

Mieszko Rutkowski, Andrzej Rostworowski

A number of authors provided arguments that a rotating gravastar is a good candidate for a source of the Kerr metric. These arguments were based on the second order perturbation an…

hep-th2019★ 22 cited

Master equations and stability of Einstein-Maxwell-scalar black holes

Aron Jansen, Andrzej Rostworowski, Mieszko Rutkowski

We derive master equations for linear perturbations in Einstein-Maxwell-scalar theory, for any spacetime dimension D and any background with a maximally symmetric n = (D - 2)-dimen…

gr-qc2019★ 2 cited

Nonlinear perturbations of Reissner-Nordström black holes

Mieszko Rutkowski

We develop a nonlinear perturbation theory of Reissner-Nordström black holes. We show that, at each perturbation level, Einstein-Maxwell equations can be reduced to four inhomogene…

gr-qc2018★ 5 cited

Einstein clusters as models of inhomogeneous spacetimes

Sebastian J. Szybka, Mieszko Rutkowski

We study the effect of small-scale inhomogeneities for Einstein clusters. We construct a spherically symmetric stationary spacetime with small-scale radial inhomogeneities and prop…

gr-qc2016★ 3 cited

Collisions near Kerr black holes: lower limit of energy between orbiting and incoming particles

Mieszko Rutkowski

In our paper we investigate the lower limit of collisional energy of test particles near the Kerr black hole. In particular we examine the minimal Lorentz factor between the freely…

astro-ph.HE2015★ 38 cited

A spine-sheath model for strong-line blazars

Marek Sikora, Mieszko Rutkowski, Mitchell C. Begelman

We have developed a quasi-analytical model for the production of radiation in strong-line blazars, assuming a spine-sheath jet structure. The model allows us to study how the spine…

astro-ph.HE2015

Evolutionary tracks of millisecond pulsars with low-mass companions

Filip Ficek, Mieszko Rutkowski, Włodek Kluźniak

We consider the evolution of millisecond radio pulsars in binary systems with a main-sequence or evolved stellar companion. Evolution of non-accreting binary systems with "eclipsin…