We study the effect of symmetry-breaking perturbations in the one-dimension
al SU(4) spin-orbital model. We allow the exchange in spin (J(1)) and orbit
al (J(2)) channel to be different and thus reduce the symmetry to SU(2) x S
U(2). A magnetic field h along the S-z direction is also applied. Using the
formalism developed by Azaria er al. [Phys. Rev. Lett. 83, 624 (1999)] we
extend their analysis of the isotropic J(1)=J(2), h=0 case and obtain the l
ow-energy effective theory near the SU(4) point in the generic case J(1)not
equal J(2), h not equal 0. In zero magnetic field, we retrieve the same qu
alitative low-energy;physics as in the isotropic case. In particular, the i
sotropic massless behavior found on the line J(1)=J(2)<K/4 extends in a lar
ge anisotropic region. We discover, however, that the anisotropy plays its
trick in allowing nontrivial scaling behaviors of the physical quantities.
For example, the mass gap M has two different scaling behaviors depending o
n the anisotropy. In addition, we show that in some regions, the anisotropy
is responsible for anomalous finite-size effects and may change qualitativ
ely the shape of the computed critical line in a finite system. When a magn
etic field is present the effect of the anisotropy is striking. In addition
to the usual commensurate-incommensurate phase transition that occurs in t
he spin sector of the theory, we find that the field may induce a second tr
ansition of the KT type in the remaining degrees of freedom to which it doe
s nor couple directly. In this sector, we find that the effective theory is
that of an SO(4) Gross-Neveu model with an h-dependent coupling that may c
hange its sign as h varies.