Conveners
Session 9
- Nobutoshi Yasutake (Chiba Institute of Technology)
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Toshitaka Tatsumi (home)02/05/2026, 13:15
Origin of the strong magnetic field observed in compact stars has been an interesting issue. If nuclear matter favors spin polarization, it gives a possible origin of the magnetic field. However, any realistic calculation has not given positive results. We discuss some microscopic origin of the magnetic field in dense quark matter. We consider here two types of chiral transitions, dual chiral...
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JiaXing Niu (Yangzhou university)02/05/2026, 13:50
Data tables on the equation of state (EOS) and microscopic structures for dense stellar matter under both cold and finite-temperature conditions with proton fractions $Y_p =0.01$-$0.65$ and baryon number densities $n_\text{b}=10^{-8}$-$2 \ \mathrm{fm}^{-3}$ are obtained adopting two classes of relativistic density functionals, namely, those with nonlinear self-couplings and those with...
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Cheng-Jun Xia (Yangzhou University)02/05/2026, 14:10
The properties of magnetized dense stellar matter in white dwarfs and neutron star crusts are investigated in a fully three-dimensional geometry with periodic boundary condition. The Thomas-Fermi approximation is employed to fixed the electron density profiles, while the nonuniform magnetic fields are treated with equivalent magnetic charge method.
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