Magnetic materials have their
spins aligned over a macroscopic
length scale. Alignment of the spins is typically driven by
exchange interaction between neighboring spins. While at
absolute zero (T = 0) the alignment can always exist, thermal fluctuations misalign magnetic moments at temperatures above the
Curie temperature (T_C), causing a
phase transition to a non-magnetic state. Whether T_C is above the absolute zero depends heavily on the dimensions of the system. For a 3D system, the
Curie temperature is always above zero, while a one-dimensional system can only be in a ferromagnetic state at T = 0 For 2D systems, the transition temperature depends on the spin dimensionality (n). CrI3. behaves like isotropic Heisenberg model. The intrinsic anisotropy in CrI3 and Fe3GeTe2 is caused by strong
spin–orbit coupling, allowing them to remain magnetic down to a
monolayer, while Cr2Ge2Te6 has only exhibit magnetism as a bilayer or thicker. The
XY model describes the case where n = 2. In this system, there is no transition between the ordered and unordered states, but instead the system undergoes a so-called
Kosterlitz–Thouless transition at finite temperature T_{KT}, where at temperatures below T_{KT} the system has quasi-long-range magnetic order. It was reported that the theoretical predictions of the
XY model are consistent with those experimental observations of NiPS3. The Heisenberg model describes the case where n = 3. In this system, there is no transition between the ordered and unordered states because of the
Mermin-Wagner theorem. The experimental realization of the Heisenberg model was reported using MnPS3. The above systems can be described by a generalized Heisenberg spin
Hamiltonian: :H = -\frac{1}{2} \sum_{} (J \mathbf{S}_i \cdot \mathbf{S}_j + \Lambda S_j^z S_i^z) - \sum_{i} A(S_i^z)^2, Where J is the exchange coupling between spins \mathbf{S}_i and \mathbf{S}_j, and A and \Lambda are on-site and inter-site magnetic anisotropies, respectively. Setting A \rightarrow \pm\infty recovered the 2D Ising model and the XY model. (positive sign for n = 1 and negative for n = 2), while A \approx 0 and \Lambda \approx 0 recovers the Heisenberg model (n = 3). Along with the idealized models described above, the spin Hamiltonian can be used for most experimental setups, and it can also model dipole-dipole interactions by renormalization of the parameter A. However, sometimes including further neighbours or using different exchange coupling, such as
antisymmetric exchange, is required. == Measuring two-dimensional magnetism==