scholarly journals R-PROCESS NUCLEOSYNTHESIS IN NEUTRON STAR MERGER WITH NEW FISSION MODEL

2015 ◽  
Author(s):  
Shota Shibagaki
Keyword(s):  
Neutron Star ◽  
R Process

scholarly journals Fission fragment distributions and their impact on the r -process nucleosynthesis in neutron star mergers

2021 ◽  
Vol 103 (2) ◽  
Author(s):  
J.-F. Lemaître ◽  
S. Goriely ◽  
A. Bauswein ◽  
H.-T. Janka
Keyword(s):  
Neutron Star ◽  
Fission Fragment ◽  
R Process

scholarly journals The role of fission on neutron star mergers and its impact on the r-process peaks

2016 ◽  
Author(s):  
M. Eichler ◽  
A. Arcones ◽  
A. Kelic ◽  
O. Korobkin ◽  
K. Langanke ◽  
...  
Keyword(s):  
Neutron Star ◽  
R Process

scholarly journals Fission and the r -process nucleosynthesis of translead nuclei in neutron star mergers

2020 ◽  
Vol 102 (4) ◽  
Author(s):  
Samuel A. Giuliani ◽  
Gabriel Martínez-Pinedo ◽  
Meng-Ru Wu ◽  
Luis M. Robledo
Keyword(s):  
Neutron Star ◽  
R Process

The r-process nucleosynthesis during the decompression of neutron star crust material

2014 ◽  
Author(s):  
S. Goriely ◽  
A. Bauswein ◽  
H.-T. Janka ◽  
J.-L. Sida ◽  
J.-F. Lemaı̂tre ◽  
...  
Keyword(s):  
Neutron Star ◽  
Neutron Star Crust ◽  
R Process

scholarly journals Merger and Mass Ejection of Neutron Star Binaries

2019 ◽  
Vol 69 (1) ◽  
pp. 41-64 ◽  
Author(s):  
Masaru Shibata ◽  
Kenta Hotokezaka
Keyword(s):  
Numerical Simulation ◽  
Black Hole ◽  
Neutron Star ◽  
Numerical Relativity ◽  
High Energy ◽  
Ejection Process ◽  
Merger Process ◽  
Unique Approach ◽  
R Process ◽  
Mass Ejection

Mergers of binary neutron stars and black hole–neutron star binaries are among the most promising sources for ground-based gravitational-wave (GW) detectors and are also high-energy astrophysical phenomena, as illustrated by the observations of GWs and electromagnetic (EM) waves in the event of GW170817. Mergers of these neutron star binaries are also the most promising sites for r-process nucleosynthesis. Numerical simulation in full general relativity (numerical relativity) is a unique approach to the theoretical prediction of the merger process, GWs emitted, mass ejection process, and resulting EM emission. We summarize the current understanding of the processes of neutron star mergers and subsequent mass ejection based on the results of the latest numerical-relativity simulations. We emphasize that the predictions of the numerical-relativity simulations agree broadly with the optical and IR observations of GW170817.

scholarly journals r -process nucleosynthesis from matter ejected in binary neutron star mergers

2017 ◽  
Vol 96 (12) ◽  
Author(s):  
Luke Bovard ◽  
Dirk Martin ◽  
Federico Guercilena ◽  
Almudena Arcones ◽  
Luciano Rezzolla ◽  
...  
Keyword(s):  
Neutron Star ◽  
Binary Neutron Star ◽  
R Process
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