  Axion Like Particles (ALPs) are one promising kind of dark matter candidate
particles that are predicted to couple with photons in the presence of magnetic
fields. The oscillations between photons and ALPs travelling in the magnetic
fields have been used to constrain ALP properties. In this work, we obtain some
new constraints on the ALP mass $m_{\rm a}$ and the photon-ALP coupling
constant $g$ with two different magnetic field models through TeV photons from
PKS 2155-304. One is the discrete-$\varphi$ model that the magnetic field has
the orientation angle $\varphi$ changes discretely and randomly from one
coherent domain to the next, another is the linearly-continuous-$\varphi$ model
that the magnetic field orientation angle $\varphi$ varies continuously across
neighboring coherent domains. For the discrete-$\varphi$ model, we can obtain
the best constraints on the ALP mass $m_{1}=m_{\rm a}/(1\ {\rm neV})=0.1$ and
on the photon-ALP coupling constant $g_{11}=g/(10^{-11}\ {\rm GeV^{-1}})=5$,
the reasonable range of the ALP mass $m_{1}$ is 0.08 $\thicksim$ 0.2 when
$g_{11}$=5, and the only reasonable value of the photon-ALP coupling constant
is $g_{11}$=5 when $m_{1}$=0.1. For the linearly-continuous-$\varphi$ model, we
can obtain the best constraints on the ALP mass $m_{1}=0.1$ and on the
photon-ALP coupling constant $g_{11}=0.7$, the reasonable range of the ALP mass
$m_{1}$ is 0.05 $\thicksim$ 0.4 when $g_{11}$=0.7, and the reasonable range of
the photon-ALP coupling constant $g_{11}$ is 0.5 $\thicksim$ 1 when
$m_{1}$=0.1. All the results are consistent with the upper bound
($g<6.6\times10^{-11}\ {\rm GeV^{-1}}$, i.e. $g_{11}<6.6$) set by the CAST
experiment.
