  The restriction of $\sigma^{*}$ and $\phi$ on the protoneutron star (PNS) PSR
J0348+0432 is described by the relativistic mean field theory (RMFT) through
choosing the effective coupling constants. We use an entropy per baryon S=1 to
describe thermal effect on PSR J0348+0432 in this work and compare the
differences between PNS PSR J0348+0432 with $\sigma^{*}$,$\phi$ and without
$\sigma^{*}$,$\phi$. These effects include the particle number distribution,
the mass-radius relation, the moment of inertia and the surface gravitational
redshift. The PNS PSR J0348+0432 with $\sigma^{*}$ and $\phi$ has more nucleons
and will pushed forward the threshold for the appearance of the hyperons. The
mass-radius relations are ($2.010M_{\odot}$,12.6520km) with $\sigma^{*}$ and
$\phi$ and ($2.010M_{\odot}$,12.6170km) without $\sigma^{*}$ and $\phi$
respectively. The moment of inertia corresponding PNS PSR J0348+0432 are
($2.010M_{\odot}$,1.510$\times 10^{45}$g.cm$^{2}$) and
($2.010M_{\odot}$,1.559$\times 10^{45}$g.cm$^{2}$) respectively, the surface
gravitational redshift corresponding PNS PSR J0348+0432 are
($2.010M_{\odot}$,0.3747) and ($2.010M_{\odot}$,0.3701) respectively. With the
help of these calculations, we study the restriction of $\sigma^{*}$ and $\phi$
on the interactions between baryons in PNS core.
