scholarly journals Gravitational radiation from the coalescence of binary neutron stars: Effects due to the equation of state, spin, and mass ratio

1996 ◽  
Vol 54 (12) ◽  
pp. 7261-7277 ◽  
Author(s):  
Xing Zhuge ◽  
Joan M. Centrella ◽  
Stephen L. W. McMillan
Keyword(s):  
Equation Of State ◽  
Neutron Stars ◽  
Gravitational Radiation ◽  
Mass Ratio ◽  
Binary Neutron Stars ◽  
State Spin

scholarly journals Impact of the nuclear equation of state on the last orbits of binary neutron stars

2005 ◽  
Vol 431 (1) ◽  
pp. 297-306 ◽  
Author(s):  
M. Bejger ◽  
D. Gondek-Rosińska ◽  
E. Gourgoulhon ◽  
P. Haensel ◽  
K. Taniguchi ◽  
...  
Keyword(s):  
Equation Of State ◽  
Neutron Stars ◽  
Nuclear Equation Of State ◽  
Binary Neutron Stars

scholarly journals Constraining the neutron star equation of state with gravitational wave signals from coalescing binary neutron stars

2015 ◽  
Vol 92 (2) ◽  
Author(s):  
M. Agathos ◽  
J. Meidam ◽  
W. Del Pozzo ◽  
T. G. F. Li ◽  
M. Tompitak ◽  
...  
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Neutron Stars ◽  
Gravitational Wave ◽  
Binary Neutron Stars

scholarly journals R-mode constraints from neutron star equation of state

2019 ◽  
Vol 23 ◽  
pp. 100
Author(s):  
Ch. C. Moustakidis ◽  
M. C. Papazoglou
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Neutron Stars ◽  
Gravitational Radiation ◽  
Mode Instability ◽  
X Ray ◽  
Long Time ◽  
Low Mass ◽  
X Ray Binaries

The gravitational radiation has been proposed a long time before, as an explana- tion for the observed relatively low spin frequencies of young neutron stars and of accreting neutron stars in low-mass X-ray binaries as well. In the present work we studied the effects of the neutron star equation of state on the r-mode instability window of rotating neutron stars.

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