scholarly journals Maximum mass cutoff in the neutron star mass distribution and the prospect of forming supramassive objects in the double neutron star mergers

2020 ◽  
Vol 102 (6) ◽  
Author(s):  
Dong-Sheng Shao ◽  
Shao-Peng Tang ◽  
Jin-Liang Jiang ◽  
Yi-Zhong Fan
Keyword(s):  
Neutron Star ◽  
Mass Distribution ◽  
Maximum Mass ◽  
Star Mass ◽  
Neutron Star Mass

scholarly journals Neutron star masses

2012 ◽  
Vol 8 (S291) ◽  
pp. 146-146
Author(s):  
David Nice
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Nuclear Matter ◽  
Observational Data ◽  
Mass Distribution ◽  
Binary Star ◽  
Star Mass ◽  
Star Evolution ◽  
Neutron Star Mass ◽  
Present Understanding

AbstractNeutron star masses can be inferred from observations of binary pulsar systems, particularly by the measurement of relativistic phenomena within these orbits. The observed distribution of masses can be used to infer or constrain the equation of state for nuclear matter and to study astrophysical processes such as supernovae and binary star evolution. In this talk, I will review our present understanding of the neutron star mass distribution with an emphasis on the observational data.

scholarly journals Neutron Star Mass Distribution in Binaries

2016 ◽  
Vol 716 ◽  
pp. 012021
Author(s):  
Chang-Hwan Lee ◽  
Young-Min Kim
Keyword(s):  
Neutron Star ◽  
Mass Distribution ◽  
Star Mass ◽  
Neutron Star Mass

scholarly journals THE NEUTRON STAR MASS DISTRIBUTION

2013 ◽  
Vol 778 (1) ◽  
pp. 66 ◽  
Author(s):  
Bülent Kiziltan ◽  
Athanasios Kottas ◽  
Maria De Yoreo ◽  
Stephen E. Thorsett
Keyword(s):  
Neutron Star ◽  
Mass Distribution ◽  
Star Mass ◽  
Neutron Star Mass

scholarly journals Nucleosynthesis and Kilonovae from Strange Star Mergers

Universe ◽  
2019 ◽  
Vol 5 (6) ◽  
pp. 144
Author(s):  
J. E. Horvath ◽  
O. G. Benvenuto ◽  
E. Bauer ◽  
L. Paulucci ◽  
A. Bernardo ◽  
...  
Keyword(s):  
Neutron Star ◽  
Binary System ◽  
Mass Distribution ◽  
A Priori ◽  
Strange Star ◽  
Star Mass ◽  
Full Characterization ◽  
Neutron Star Mass ◽  
A Priori Probability

In this talk, we summarize the work in progress toward a full characterization of strange star–strange star (SS–SS) mergers related to the GW/GRB/kilonova events. In addition, we show that the a priori probability constructed from the observed neutron star mass distribution points toward an asymmetric binary system as the progenitor of the GW170817 event.

scholarly journals Measuring neutron star mass and radius with three mass-radius relations

2007 ◽  
Vol 374 (1) ◽  
pp. 232-236 ◽  
Author(s):  
C. M. Zhang ◽  
H. X. Yin ◽  
Y. Kojima ◽  
H. K. Chang ◽  
R. X. Xu ◽  
...  
Keyword(s):  
Neutron Star ◽  
Star Mass ◽  
Neutron Star Mass
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