activity
20052012
most citedGravitational waves from neutron stars: Promises and challenges

219 citations · 1k across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.HE2012★ 53 cited

The runaway instability in general relativistic accretion disks

O. Korobkin, E. Abdikamalov, N. Stergioulas +4

When an accretion disk falls prey to the runaway instability, a large portion of its mass is devoured by the black hole within a few dynamical times. Despite decades of effort, it…

astro-ph.SR2012★ 17 cited

Gravitational Waves and Hydromagnetic Instabilities in Rotating Magnetized Neutron Stars

Paul D. Lasky, Burkhard Zink, Kostas D. Kokkotas

We perform nonlinear general relativistic ideal magnetohydrodynamic simulations of poloidal magnetic fields in rotating polytropic neutron stars. We have three primary goals: i) to…

gr-qc2011★ 76 cited

Are gravitational waves from giant magnetar flares observable?

Burkhard Zink, Paul D. Lasky, Kostas D. Kokkotas

Are giant flares in magnetars viable sources of gravitational radiation? Few theoretical studies have been concerned with this problem, with the small number using either highly id…

astro-ph.SR2011★ 47 cited

The f-mode instability in relativistic neutron stars

Erich Gaertig, Kostas Glampedakis, Kostas D. Kokkotas +1

Rapidly spinning neutron stars are known to harbour pulsation modes that may become unstable and grow in amplitude by emitting gravitational radiation. Among the various stellar mo…

astro-ph.SR2011★ 85 cited

Hydromagnetic Instabilities in Neutron Stars

Paul D. Lasky, Burkhard Zink, Kostas D. Kokkotas +1

We model the non-linear ideal magnetohydrodynamics of poloidal magnetic fields in neutron stars in general relativity assuming a polytropic equation of state. We identify familiar…

gr-qc2011★ 10 cited

HORIZON: Accelerated General Relativistic Magnetohydrodynamics

Burkhard Zink

We present Horizon, a new graphics processing unit (GPU)-accelerated code to solve the equations of general relativistic magnetohydrodynamics in a given spacetime. We evaluate the…