scholarly journals The Absence of Cyclotron Lines in Neutron-Star Atmospheres with Super-Strong Magnetic Fields

2000 ◽  
Vol 52 (1) ◽  
pp. 167-173 ◽  
Author(s):  
Osamu Nishimura ◽  
Kousuke Sumiyoshi ◽  
Toshikazu Ebisuzaki
Keyword(s):  
Neutron Star ◽  
Magnetic Fields ◽  
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 Neutron Star Composition in Strong Magnetic Fields

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

scholarly journals Neutron Star Crust in Strong Magnetic Fields

2011 ◽  
Vol 312 (4) ◽  
pp. 042016 ◽  
Author(s):  
Rana Nandi ◽  
Debades Bandyopadhyay
Keyword(s):  
Neutron Star ◽  
Magnetic Fields ◽  
Strong Magnetic Fields ◽  
Neutron Star Crust

scholarly journals Thermal luminosities of cooling neutron stars

2020 ◽  
Vol 496 (4) ◽  
pp. 5052-5071 ◽  
Author(s):  
A Y Potekhin ◽  
D A Zyuzin ◽  
D G Yakovlev ◽  
M V Beznogov ◽  
Yu A Shibanov
Keyword(s):  
Spectral Analysis ◽  
Neutron Star ◽  
Magnetic Fields ◽  
Neutron Stars ◽  
Cooling Curves ◽  
Middle Aged ◽  
Superdense Matter ◽  
Strong Magnetic Fields ◽  
Stellar Core ◽  
Neutron Star Cooling

ABSTRACT Ages and thermal luminosities of neutron stars, inferred from observations, can be interpreted with the aid of the neutron star cooling theory to gain information on the properties of superdense matter in neutron-star interiors. We present a survey of estimated ages, surface temperatures, and thermal luminosities of middle-aged neutron stars with relatively weak or moderately strong magnetic fields, which can be useful for these purposes. The catalogue includes results selected from the literature, supplemented with new results of spectral analysis of a few cooling neutron stars. The data are compared with the theory. We show that overall agreement of theoretical cooling curves with observations improves substantially for models where neutron superfluidity in stellar core is weak.

Effects of Strong Magnetic Fields on Neutron Star Structure

2001 ◽  
Vol 554 (1) ◽  
pp. 322-339 ◽  
Author(s):  
Christian Y. Cardall ◽  
Madappa Prakash ◽  
James M. Lattimer
Keyword(s):  
Neutron Star ◽  
Magnetic Fields ◽  
Strong Magnetic Fields ◽  
Star Structure
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