“…[5,6,8] Our earlier results [19][20][21][22] also suggest that the model with the NNN interaction gives predictions in better agreement with the experimental data. Besides the aforementioned, the choice of the dominant interactions is supported by the fact that these interactions, especially NN, NNN, and DM interaction, but also spin anisotropy to a lesser extent, show a distinctive pressure dependence, [23,24] enabling one to affect the phase transition temperature by applying high pressures on the system. Having this in mind, the purpose of this article will be to study the 2D antiferromagnetic Heisenberg model with the uniaxial XXZ spin anisotropy, DM interaction, and in-plane frustration included.…”