  The range of the U bosonic coupling constants in neutron star matter is a
very interesting but still unsolved problem which has multifaceted influences
in nuclear physics, particle physics, astrophysics and cosmology. The
combination of the theoretical numerical simulation and the recent observations
provides a very good opportunity to solve this problem. In the present work,
the range of the U bosonic coupling constants is inferred based on the three
relations of the mass-radius, mass-frequency and mass-tidal deformability in
neutron star containing hyperons using the GM1, TM1 and NL3 parameter sets
under the two flavor symmetries of the SU(6) and SU(3) in the framework of the
relativistic mean field theory. Combined with observations from PSRs
J1614-2230, J0348+0432, J2215-5135, J0952-0607, J0740+6620, J0030-0451,
J1748-2446ad, XTE J1739-285, GW170817 and GW190814 events, our numerical
results show that the U bosonic coupling constants may tend to be within the
range from 0 to 20 GeV$^{-2}$ in neutron star containing hyperons. Moreover,
the numerical results of the three relations obtained by the SU(3) symmetry are
better in accordance with observation data than those obtained by the SU(6)
symmetry. The results will help us to improve the strict constraints of the
equation of state for neutron stars containing hyperons.
