activity
20072015
most citedHigh resolution numerical-relativity simulations for the merger of binary magnetized neutron stars

221 citations · 479 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2015★ 190 cited

High-resolution magnetohydrodynamics simulation of black hole-neutron star merger: Mass ejection and short gamma-ray burst

Kenta Kiuchi, Yuichiro Sekiguchi, Koutarou Kyutoku +3

We report results of a high-resolution numerical-relativity simulation for the merger of black hole-magnetized neutron star binaries on Japanese supercomputer "K". We focus on a bi…

astro-ph.HE2014★ 221 cited

High resolution numerical-relativity simulations for the merger of binary magnetized neutron stars

Kenta Kiuchi, Koutarou Kyutoku, Yuichiro Sekiguchi +2

We perform high-resolution magnetohydrodynamics simulations of binary neutron star mergers in numerical relativity on the Japanese supercomputer K. The neutron stars and merger rem…

astro-ph.SR2013★ 32 cited

Kinetic aspects of the ion current layer in a reconnection outflow exhaust

Seiji Zenitani, Iku Shinohara, Tsugunobu Nagai +1

Kinetic aspects of the ion current layer at the center of a reconnection outflow exhaust near the X-type region are investigated by a two-dimensional particle-in-cell (PIC) simulat…

astro-ph.HE2011★ 18 cited

A Particle Simulation for the Axisymmetric Pulsar Magnetosphere: II. the case of dipole field

Tomohide Wada, Shinpei Shibata

The main issue of the pulsar magnetosphere is how the rotation power is converted into both particle beams which causes pulsed emissions, and a highly relativistic wind of electron…

astro-ph2007★ 18 cited

A Particle Simulation for the Global Pulsar Magnetosphere: the Pulsar Wind linked to the Outer Gaps

Tomohide Wada, Shinpei Shibata

Soon after the discovery of radio pulsars in 1967, the pulsars are identified as strongly magnetic (typically G) rapidly rotating ( Hz) neutron stars. How…