  The paper deals with cosmological solutions describing different phases of
the Universe for the homogeneous and isotropic FLRW model of the Universe with
torsion. Normally, torsion field is not suitable for maximally symmetric space
time model. However, one may use a specific profile of vectorial torsion field,
derived from a scalar function. By proper choices of the torsion scalar
function, it is shown that a continuous cosmic evolution starting from the
emergent scenario to the present late time acceleration is possible. Also
thermodynamics of the system is analyzed and equivalence with Einstein gravity
is discussed.
