Cold Ideal Equation of State for Strongly Magnetized Neutron Star Matter: Effects on Muon Production and Pion Condensation

2001 ◽  
Vol 546 (2) ◽  
pp. 1126-1136 ◽  
Author(s):  
In‐Saeng Suh ◽  
G. J. Mathews
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Neutron Star Matter ◽  
Pion Condensation ◽  
Matter Effects ◽  
Muon Production

scholarly journals Gravitational-Wave Constraints on the Neutron-Star-Matter Equation of State

2018 ◽  
Vol 120 (17) ◽  
Author(s):  
Eemeli Annala ◽  
Tyler Gorda ◽  
Aleksi Kurkela ◽  
Aleksi Vuorinen
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Gravitational Wave ◽  
Neutron Star Matter

Equation of State of Neutron-Star Matter at Subnuclear Densities

1972 ◽  
Vol 176 ◽  
pp. 723 ◽  
Author(s):  
Zalman Barkat ◽  
Jean-Robert Buchler ◽  
Lester Ingber
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Neutron Star Matter

scholarly journals Parametrized equation of state for neutron star matter with continuous sound speed

2020 ◽  
Vol 102 (8) ◽  
Author(s):  
Michael F. O’Boyle ◽  
Charalampos Markakis ◽  
Nikolaos Stergioulas ◽  
Jocelyn S. Read
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Sound Speed ◽  
Neutron Star Matter

scholarly journals COMPUTATION OF NEUTRON STAR STRUCTURE USING MODERN EQUATION OF STATE

2006 ◽  
Vol 21 (07) ◽  
pp. 1555-1565 ◽  
Author(s):  
G. H. BORDBAR ◽  
M. HAYATI
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Equations Of State ◽  
Maximum Mass ◽  
Neutron Star Matter ◽  
Radio Pulsars ◽  
Good Consistency ◽  
The Given ◽  
Neutron Star Radius ◽  
Star Structure

Using the modern equations of state derived from microscopic calculations, we have calculated the neutron star structure. For the neutron star, we have obtained a minimum mass about 0.1 M⊙ which is nearly independent of the equation of state, and a maximum mass between 1.47 M⊙ and 1.98 M⊙ which is strongly dependent on the equation of state. It is shown that among the equations of state of neutron star matter which we have used, the stiffest one leads to higher maximum mass and radius and lower central density. It is seen that the given maximum mass for the Reid-93 equation of state shows a good consistency with the accurate observations of radio pulsars. We have indicated that the thickness of neutron star crust is very small compared to the predicted neutron star radius.

scholarly journals Instability of Neutron Star Matter for Pion Condensation

1975 ◽  
Vol 54 (5) ◽  
pp. 1429-1439 ◽  
Author(s):  
A. Suzuki ◽  
Y. Futami ◽  
Y. Takahashi
Keyword(s):  
Neutron Star ◽  
Neutron Star Matter ◽  
Pion Condensation
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