Meson effect in the proto neutron star PSR J0348+0432
Xian-Feng Zhao

TL;DR
This paper investigates how specific mesons affect the physical properties of the proto neutron star PSR J0348+0432, revealing their impact on energy density, pressure, radius, and moment of inertia within a relativistic mean field framework.
Contribution
It provides a detailed analysis of the individual and combined effects of mesons $f_{0}(975)$, $ ext{ }\phi(1020)$, and $ ext{ }\delta$ on neutron star properties, which is a novel application in this context.
Findings
Mesons $f$, $ ext{ }\phi$, and $ ext{ }\delta$ alter energy density and pressure.
Considering all mesons decreases radius and moment of inertia.
Mesons $f$ and $ ext{ }\phi$ have a larger impact on moment of inertia than $ ext{ }\delta$.
Abstract
The effect of mesons (named as ), (named as ) and 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 and pressure will increase considering the mesons whereas will decrease as the mesons and being considered. When the mesons and are considered, the energy density and pressure will all decrease. It is also found that the contribution of mesons , and to the central energy density is only the central energy density's 0.060.6\% whereas the contribution of mesons , and to the central pressure is the central pressure's 47\%. For the radius, it will decrease when the contributions of mesons , and …
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