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where $\sigma^{z}$ and $\sigma^{x}$ are the Pauli Z and X matrics respectively, and $h$ is the transverse magnetic field strength.
This model is realized in physical experiments related to quantum computing23.
The state that is observed in these physical experiments is the ground state of $H$, defined as the eigenvector of $H$'s smallest eigenvalue $|\psi_{ground}\rangle = \sum_{b}^{2^{N}}c_{b}|\psi_{b}\rangle$, where $|\psi_{b}\rangle$ are basis states $|\uparrow \uparrow \uparrow \cdots \rangle$, $|\downarrow \downarrow \downarrow \cdots \rangle$, $|\uparrow \uparrow \downarrow \cdots \rangle$ and so on.
Note that for a composite system of $N$ spins, there are in total $2^{N}$ basis states.
Magnetization is defined as the average Z spin
$$\left\langle M \right\rangle=\sum_{b}^{2^{N}}p_{b}\frac{\sum_{i}^{N}\sigma_{bi}^{z}}{N}$$
where $p_{b}=\overline{c_{b}}c_{b}$ is the probability at basis state $|\psi_{b}\rangle$.
With magnetization as the order parameter, we get the following graph showing the existence of a phase transition at critical field strength $h_{c}=1$ in the one dimensional case:
This differs from the classical situation where the 1-D Ising model lacks a phase transition.
In the quantum model, the fluctuations required by the phase transition is provided by the transverse field $\sigma^{x}$ which contains off-diagonal matrix elements.
In the two dimensional case, we get $h_{c}\simeq 2.5$ which is close to the theoretical infinite lattice size case of $h_{c}=3$ (Table 3.1 Suzuki4, Fig. 4 Hesselmann5).
This phase transition can also be seen in the band diagram of the ground and excitation states.
We see that as the transverse field approaches $h_{c}$, the ground and 1st excitation energies diverge from being in a shared degenerate state, to two separate states.
Non-symmetric probability distribution in simulation
The basis state probability $p_{b}$ used in our simulations is a non-symmetric one, as opposed to the one belonging to the original hamiltonian $p_{b}^{H}$.
$p_{b}$ is defined as
where $p_{b'}^{H}$ is the probability of the basis state with all the spins in $|\psi_{b}\rangle$ flipped, $b_{\# up}$ and $b_{\#down}$ are the number of spin ups and downs in basis state $|\psi_{b}\rangle$.
In real world experiments, such a non-symmetric distribution is a more realistic description, as it is unlikely to see all $N$ spins flipped down if the initial state is prepared with all up spins, especially when $N$ is very large.
However, due to the finite lattice size of simulations, the characteristic time where the system flips from +M to -M state is much smaller than the observation time as seen in the below graph from Fig 3.10, Section 3.4, Binder et al.6:
Such a non-symmetric distribution in effect measures the average absolute value of magnetization $\left\langle \left| M \right| \right\rangle$ as opposed to the raw average magenetization $\left\langle M \right\rangle$, which in the case of $h\sim 0$ is always 0 for a symmetric hamiltonian like ours.
In the classical 2-D Ising model where $T_{c}=2.269$, we see from the below graphsthat the non-symmetric distribution gives better results (upper graph non-symmetric, lower graph symmetric, from Fig. 14, Fig 15, J. Kotze7):