activity
19962008
most citedGravitational waves from relativistic neutron star mergers with nonzero-temperature equations of state

133 citations · 258 across the 7 of their papers we have counts for

collaborators
Showing astro-phShow all

16 papers · 1 filter

astro-ph2008107 cited

Influence of light nuclei on neutrino-driven supernova outflows

A. Arcones, G. Martinez-Pinedo, E. O'Connor +4

We study the composition of the outer layers of a protoneutron star and show that light nuclei are present in substantial amounts. The composition is dominated by nucleons, deutero…

astro-ph200711 cited

Neutrino-driven explosions twenty years after SN1987A

H. -Th. Janka, A. Marek, F. -S. Kitaura

The neutrino-heating mechanism remains a viable possibility for the cause of the explosion in a wide mass range of supernova progenitors. This is demonstrated by recent two-dimensi…

astro-ph2007133 cited

Gravitational waves from relativistic neutron star mergers with nonzero-temperature equations of state

R. Oechslin, H. -T. Janka

We analyze the gravitational wave (GW) emission from our recently published set of relativistic neutron star (NS) merger simulations and determine characteristic signal features th…

astro-ph2006

Theory of Core-Collapse Supernovae

H. -Th. Janka, K. Langanke, A. Marek +2

Advances in our understanding and the modeling of stellar core-collapse and supernova explosions over the past 15 years are reviewed, concentrating on the evolution of hydrodynamic…

astro-ph20042 cited

Supernova Asymmetries and Pulsar Kicks -- Views on Controversial Issues

H. -Th. Janka, L. Scheck, K. Kifonidis +2

Two- and three-dimensional simulations demonstrate that hydrodynamic instabilities can lead to low-mode (l=1,2) asymmetries of the fluid flow in the neutrino-heated layer behind th…

astro-ph2004

Global Anisotropies in Supernova Explosions and Pulsar Recoil

L. Scheck, T. Plewa, K. Kifonidis +2

We show by two-dimensional and first three-dimensional simulations of neutrino-driven supernova explosions that low (l=1,2) modes can dominate the flow pattern in the convective po…