Meson effect in the proto neutron star PSR J0348+0432

Abstract

The effect of mesons $f_0(975)$ (named as $f$), $\varphi (1020)$ (named as $\varphi$) and $\delta$ on the moment of inertia of the PNS PSR J0348+0432 is examined in the framework of the relativistic mean field theory considering the baryon octet. It is found that the energy density $\epsilon$ and pressure $p$ will increase considering the mesons $\delta$ whereas will decrease as the mesons $f$ and $\varphi$ being considered. When the mesons $f,\varphi$ and $\delta$ are considered, the energy density and pressure will all decrease. It is also found that the contribution of mesons $f$, $\varphi$ and $\delta$ to the central energy density is only the central energy density's 0.06$\sim$0.6\% whereas the contribution of mesons $f$, $\varphi$ and $\delta$ to the central pressure is the central pressure's 4$\sim$7\%. For the radius, it will decrease when the contributions of mesons $f$, $\varphi$ and $\delta$ are considered. The moment of inertia $I$ will increase considering the mesons $\delta$ whereas will decrease as the mesons $f$ and $\varphi$ being considered. When the mesons $f$, $\varphi$ and $\delta$ are all considered, the moment of inertia will decrease. It is found that the contribution of mesons $f$ and $\varphi$ to moment of inertia is 4$\sim$9 times larger than that of mesons $\delta$. Our results show that the mesons $f$, $\varphi$ and $\delta$ contribute to the moment of inertia's 2$\sim$5\%.

arXiv comment13 pages, 7 figures

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