scholarly journals Dynamical mass ejection from binary neutron star mergers: Radiation-hydrodynamics study in general relativity

2015 ◽  
Vol 91 (6) ◽  
Author(s):  
Yuichiro Sekiguchi ◽  
Kenta Kiuchi ◽  
Koutarou Kyutoku ◽  
Masaru Shibata
Keyword(s):  
General Relativity ◽  
Neutron Star ◽  
Radiation Hydrodynamics ◽  
Dynamical Mass ◽  
Binary Neutron Star ◽  
Mass Ejection

scholarly journals Dynamical mass ejection from binary neutron star mergers

2016 ◽  
Vol 460 (3) ◽  
pp. 3255-3271 ◽  
Author(s):  
David Radice ◽  
Filippo Galeazzi ◽  
Jonas Lippuner ◽  
Luke F. Roberts ◽  
Christian D. Ott ◽  
...  
Keyword(s):  
Neutron Star ◽  
Dynamical Mass ◽  
Binary Neutron Star ◽  
Mass Ejection

scholarly journals Mass Ejection from the Remnant of a Binary Neutron Star Merger: Viscous-radiation Hydrodynamics Study

2018 ◽  
Vol 860 (1) ◽  
pp. 64 ◽  
Author(s):  
Sho Fujibayashi ◽  
Kenta Kiuchi ◽  
Nobuya Nishimura ◽  
Yuichiro Sekiguchi ◽  
Masaru Shibata
Keyword(s):  
Neutron Star ◽  
Radiation Hydrodynamics ◽  
Binary Neutron Star ◽  
Mass Ejection

scholarly journals Mass ejection from disks surrounding a low-mass black hole: Viscous neutrino-radiation hydrodynamics simulation in full general relativity

2020 ◽  
Vol 101 (8) ◽  
Author(s):  
Sho Fujibayashi ◽  
Masaru Shibata ◽  
Shinya Wanajo ◽  
Kenta Kiuchi ◽  
Koutarou Kyutoku ◽  
...  
Keyword(s):  
General Relativity ◽  
Black Hole ◽  
Radiation Hydrodynamics ◽  
Neutrino Radiation ◽  
Low Mass ◽  
Mass Ejection

Pan Galactic Gargle Blaster

2019 ◽  
pp. 132-137
Author(s):  
Nicholas Mee
Keyword(s):  
General Relativity ◽  
Neutron Star ◽  
Neutron Stars ◽  
Gravitational Waves ◽  
Gamma Ray ◽  
Great Accuracy ◽  
Gamma Ray Bursts ◽  
Tests Of General Relativity ◽  
Binary Neutron Star

The sources of short gamma ray bursts (GRBs) have been identified with neutron star merger events. Hulse and Taylor discovered the first binary neutron star in 1974. By monitoring the pulsar in this system the orbital characteristics of the system have been determined with great accuracy. This has led to tests of general relativity, including the first confirmation of the existence of gravitational waves. The emission of this radiation is gradually bringing the two neutron stars together. They will collide and merge in about 300 million years.

scholarly journals Dynamical mass ejection from black hole-neutron star binaries

2015 ◽  
Vol 92 (4) ◽  
Author(s):  
Koutarou Kyutoku ◽  
Kunihito Ioka ◽  
Hirotada Okawa ◽  
Masaru Shibata ◽  
Keisuke Taniguchi
Keyword(s):  
Black Hole ◽  
Neutron Star ◽  
Dynamical Mass ◽  
Mass Ejection

scholarly journals Properties of Neutrino-driven Ejecta from the Remnant of a Binary Neutron Star Merger: Pure Radiation Hydrodynamics Case

2017 ◽  
Vol 846 (2) ◽  
pp. 114 ◽  
Author(s):  
Sho Fujibayashi ◽  
Yuichiro Sekiguchi ◽  
Kenta Kiuchi ◽  
Masaru Shibata
Keyword(s):  
Neutron Star ◽  
Radiation Hydrodynamics ◽  
Pure Radiation ◽  
Binary Neutron Star

scholarly journals Binary Neutron Star Mergers: Mass Ejection, Electromagnetic Counterparts, and Nucleosynthesis

2018 ◽  
Vol 869 (2) ◽  
pp. 130 ◽  
Author(s):  
David Radice ◽  
Albino Perego ◽  
Kenta Hotokezaka ◽  
Steven A. Fromm ◽  
Sebastiano Bernuzzi ◽  
...  
Keyword(s):  
Neutron Star ◽  
Binary Neutron Star ◽  
Mass Ejection
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