scholarly journals The Equation of State of Neutron Star Matter in Strong Magnetic Fields

2000 ◽  
Vol 537 (1) ◽  
pp. 351-367 ◽  
Author(s):  
A. Broderick ◽  
M. Prakash ◽  
J. M. Lattimer
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Magnetic Fields ◽  
Neutron Star Matter ◽  
Strong Magnetic Fields

scholarly journals Delta baryons in neutron-star matter under strong magnetic fields

2021 ◽  
Vol 57 (7) ◽  
Author(s):  
Veronica Dexheimer ◽  
Kauan D. Marquez ◽  
Débora P. Menezes
Keyword(s):  
Neutron Star ◽  
Magnetic Fields ◽  
Neutron Star Matter ◽  
Strong Magnetic Fields

scholarly journals Searching optimum equations of state of neutron star matter in strong magnetic fields with rotation

2020 ◽  
Vol 2020 (10) ◽  
Author(s):  
C Watanabe ◽  
K Yanase ◽  
N Yoshinaga
Keyword(s):  
Neutron Star ◽  
Magnetic Fields ◽  
Equations Of State ◽  
Mean Field ◽  
Maximum Mass ◽  
Neutron Star Matter ◽  
Solar Mass ◽  
Strong Magnetic Fields ◽  
Relativistic Mean Field ◽  
Rho A

Abstract Masses and radii of neutron stars are obtained in the presence of strong magnetic fields together with rotation. Mass-radius relations are calculated using 11 equations of state (EoSs: GM1, TM1-a, TM1-b, TM2$\omega\rho$-a, TM2$\omega\rho$-b, NL3-a, NL3-b, NL3$\omega\rho$-a, NL3$\omega\rho$-b, DDME2-a and DDME2-b) in relativistic mean field (RMF) theory. Obtained masses are over and around twice the solar mass ($M_\odot$) for all EoSs in the presence of strong magnetic fields of $3 \times 10^{18}$ G at the center. For NL3$\omega\rho$-a and NL3$\omega\rho$-b EoSs, masses are more than $M=2.17\,M_\odot$(observed maximum mass: $2.14\,M_\odot$) even without magnetic fields. Rotational effects are found to be insignificant in any case, at least up to the Kepler frequency. Suitable EoSs are also selected concerning the constraint on the radius of a neutron star.

scholarly journals Effect of isovector-scalar meson on neutron-star matter in strong magnetic fields

2005 ◽  
Vol 32 (1) ◽  
pp. 47-61 ◽  
Author(s):  
F X Wei ◽  
G J Mao ◽  
C M Ko ◽  
L S Kisslinger ◽  
H Stöcker ◽  
...  
Keyword(s):  
Neutron Star ◽  
Magnetic Fields ◽  
Scalar Meson ◽  
Neutron Star Matter ◽  
Strong Magnetic Fields

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
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