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
2020 ◽  
Vol 2020 (10) ◽  
Author(s):  
C Watanabe ◽  
K Yanase ◽  
N Yoshinaga

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.


2005 ◽  
Vol 32 (1) ◽  
pp. 47-61 ◽  
Author(s):  
F X Wei ◽  
G J Mao ◽  
C M Ko ◽  
L S Kisslinger ◽  
H Stöcker ◽  
...  

2000 ◽  
Vol 537 (1) ◽  
pp. 351-367 ◽  
Author(s):  
A. Broderick ◽  
M. Prakash ◽  
J. M. Lattimer

2003 ◽  
Vol 20 (8) ◽  
pp. 1238-1241 ◽  
Author(s):  
Mao Guang-Jun ◽  
V. N Kondratyev ◽  
A Iwamoto ◽  
Li Zhu-Xia ◽  
Wu Xi-Zhen ◽  
...  

2000 ◽  
Vol 52 (1) ◽  
pp. 167-173 ◽  
Author(s):  
Osamu Nishimura ◽  
Kousuke Sumiyoshi ◽  
Toshikazu Ebisuzaki

2011 ◽  
Vol 312 (4) ◽  
pp. 042016 ◽  
Author(s):  
Rana Nandi ◽  
Debades Bandyopadhyay

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