Effects of isovector scalar meson on neutron star both with and without hyperon
Abstract
We study the effects of isovector-scalar (δ)-meson on neutron and hyperon stars. Influence of δ-meson on both static and rotating stars is discussed. The δ-meson in a neutron star consisting of protons, neutrons and electrons, makes the equations of states (EOS) stiffer at higher density, and consequently increases the maximum mass of the star. But induction of δ-meson in the hyperon star decreases the maximum mass. This is due to the early evolution of hyperons in presence of δ-meson.
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