  In the present work authors derive exact solutions for the relativistic
compact stars in the presence of two fields axion (Dante's Inferno model) and
with/without the complex scalar field (with the quartic self-interaction)
coupled to gravity. The matter source is assumed as the perfect fluid one, and
we also use barotropic/MIT bag EoS to derive energy density and
anisotropic/isotropic pressures from Einstein Field Equations (EFE's). For
simplicity, as the metric potentials we use Tolman-Kuchowicz metric potentials,
which are non-singular and physically acceptable. Unknown variables for the T-K
metric potentials were derived from the junction conditions. To examine the
redshift function, adiabatic index and energy, causality conditions we used
such compact stars as PSR J1416-223, PSR J1903+32, 4U 1820-30, Cen X-3, EXO
1785-248, SAX J1808.4365.
