477 citations · 771 across the 9 of their papers we have counts for
14 papers
Long-term evolution of neutron-star merger remnants in general relativistic resistive-magnetohydrodynamics with a mean-field dynamo term
Masaru Shibata, Sho Fujibayashi, Yuichiro Sekiguchi
Long-term neutrino-radiation resistive-magnetohydrodynamics simulations in full general relativity are performed for a system composed of a massive neutron star and a torus formed…
Long-term evolution of a merger-remnant neutron star in general relativistic magnetohydrodynamics I: Effect of magnetic winding
Masaru Shibata, Sho Fujibayashi, Yuichiro Sekiguchi
Long-term ideal and resistive magnetohydrodynamics (MHD) simulations in full general relativity are performed for a massive neutron star formed as a remnant of binary neutron star…
Ultra-delayed neutrino-driven explosion of rotating massive-star collapse
Sho Fujibayashi, Koh Takahashi, Yuichiro Sekiguchi +1
Long-term neutrino-radiation hydrodynamics simulations in full general relativity are performed for the collapse of rotating massive stars that are evolved from He-stars with their…
Alternative possibility of GW190521: Gravitational waves from high-mass black hole-disk systems
Masaru Shibata, Kenta Kiuchi, Sho Fujibayashi +1
We evolve high-mass disks of mass - orbiting a spinning black hole in the framework of numerical relativity. Such high-mass systems could be an outcome d…
Properties of neutrino transfer in a deformed remnant of neutron star merger
Kohsuke Sumiyoshi, Sho Fujibayashi, Yuichiro Sekiguchi +1
We study properties of neutrino transfer in a remnant of neutron star merger, consisting of a massive neutron star and a surrounding torus. We perform numerical simulations of the…
Viscous evolution of a massive disk surrounding stellar-mass black holes in full general relativity
Sho Fujibayashi, Masaru Shibata, Shinya Wanajo +3
Long-term viscous neutrino-radiation hydrodynamics simulations in full general relativity are performed for a massive disk surrounding spinning stellar-mass black holes with mass $…