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- W3105194922 abstract "We study how the magnetic field and non-standard vector channels affect hadronic, quark and hybrid stars. In the hadronic phase, we use the QHD model, with its standard $$sigma omega rho $$ mesons, and compare the results with the ones obtained with the inclusion of the strangeness hidden $$phi $$ meson. In the quark phase, we use the standard SU(3) NJL and compare the results with the version that takes into account the vector channel $$G_v({bar{psi }}gamma ^mu psi )$$. Magnetic fields are taken into account via chaotic magnetic field approximation." @default.
- W3105194922 created "2020-11-23" @default.
- W3105194922 creator A5011700408 @default.
- W3105194922 creator A5021808603 @default.
- W3105194922 date "2020-04-01" @default.
- W3105194922 modified "2023-09-24" @default.
- W3105194922 title "Role of vector channel in different classes of (non) magnetized neutron stars" @default.
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