Dynamical Quantum Phase Transitions

Author: Xu-Dong Liu | Date: April 20, 2026


1. Total Phase

1.1 Loschmidt Amplitude

The Loschmidt amplitude is defined as the overlap between the initial state and the time-evolved state:

 g_k(t) = \langle\Psi(0)|e^{-iH_k t}|\Psi(0)\rangle

In polar form, g_k(t) = r_k e^{i\varphi_R}, where r_k = |g_k(t)|. The total phase \varphi_R is extracted as:

 \varphi_R = -i \ln \left( \frac{g_k(t)}{|g_k(t)|} \right)

1.2 Density Matrix and Statistical Analogy

Using the analogy P_n = e^{-\beta E_n} / Z, we construct the density matrix in momentum space. For H_k = \omega_k \hat{n}_k \cdot \vec{\sigma}, we have:

 \begin{aligned} \rho_k(0) &= \frac{e^{-\beta H_k}}{\text{Tr } (e^{-\beta H_k})} \\ &= \frac{\cosh(\beta \omega_k) \sigma_0 - (\hat{n}_k \cdot \vec{\sigma}) \sinh(\beta \omega_k)}{\text{Tr} [ \cosh(\beta \omega_k) \sigma_0 - (\hat{n}_k \cdot \vec{\sigma}) \sinh(\beta \omega_k) ]} \\ &= \frac{\cosh(\beta \omega_k) \sigma_0 - (\hat{n}_k \cdot \vec{\sigma}) \sinh(\beta \omega_k)}{2 \cosh(\beta \omega_k)} \\ &= \frac{1}{2} \left( \sigma_0 - \tanh(\beta \omega_k) (\hat{n}_k \cdot \vec{\sigma}) \right) = \frac{1}{2} \left( \sigma_0 - m (\hat{n}_k \cdot \vec{\sigma}) \right) \end{aligned}

Here, m = \tanh(\beta \omega_k) acts as the effective magnetization.


2. DYNAMICAL PHASE

In non-Hermitian systems ($[H, H^\dagger] \neq 0$), we use biorthogonal quantum mechanics. The right and left eigenvectors satisfy H|s^r\rangle = s\omega|s^r\rangle and H^\dagger|s^l\rangle = s\omega^*|s^l\rangle with \langle s^l | s'^r \rangle = \delta_{s,s'}.

[Image of biorthogonal basis vectors in non-Hermitian systems]

The time-evolution operators are expanded as:

 \begin{aligned} U^r &= \sum_{s=\pm} e^{-is\text{Re}[\omega]t + s\text{Im}[\omega]t} |s^r\rangle\langle s^l| \\ U^{l\dagger} &= \sum_{s=\pm} e^{is\text{Re}[\omega]t + s\text{Im}[\omega]t} |s^r\rangle\langle s^l| \end{aligned}

Evaluating the traces for U^{l\dagger}U^r using the biorthogonality condition:

 \begin{aligned} \text{Tr}(U^{l\dagger}U^r) &= \sum_{s=\pm} \langle s^l| U^{l\dagger}U^r |s^r\rangle = e^{2\text{Im}[\omega]t} + e^{-2\text{Im}[\omega]t} = 2 \cosh[2\text{Im}(\omega)t] \\ \text{Tr}(U^{l\dagger}HU^r) &= \sum_{s=\pm} \langle s^l| H U^{l\dagger}U^r |s^r\rangle = \omega e^{2\text{Im}[\omega]t} - \omega e^{-2\text{Im}[\omega]t} = 2\omega \sinh[2\text{Im}(\omega)t] \\ \text{Tr}(U^{l\dagger}HU^r H) &= \sum_{s=\pm} \langle s^l| H^2 U^{l\dagger}U^r |s^r\rangle = \omega^2 e^{2\text{Im}[\omega]t} + \omega^2 e^{-2\text{Im}[\omega]t} = 2\omega^2 \cosh[2\text{Im}(\omega)t] \end{aligned}

For the initial state \rho(0) = \frac{1}{2}(\sigma_0 - \frac{m}{\omega}H), the integrated dynamical phase \varphi_D is:

 \begin{aligned} \varphi_D &= -\frac{1}{\hbar} \int_{0}^{\tau} \frac{\text{Tr}[U^{l\dagger} \frac{1}{2}(\sigma_0 - \frac{m}{\omega}H) U^r H]}{\text{Tr}[U^{l\dagger} \frac{1}{2}(\sigma_0 - \frac{m}{\omega}H) U^r]} dt \\ &= -\frac{1}{\hbar} \int_{0}^{\tau} \omega \frac{\sinh[2\text{Im}(\omega)t] - m \cosh[2\text{Im}(\omega)t]}{\cosh[2\text{Im}(\omega)t] - m \sinh[2\text{Im}(\omega)t]} dt \\ &= -\frac{1}{\hbar} \int_{0}^{\tau} \omega \frac{\tanh[2\text{Im}(\omega)t] - m}{1 - m \tanh[2\text{Im}(\omega)t]} dt \end{aligned}

3. HERMITIAN SYSTEMS

In the Hermitian limit (H = H^\dagger, \text{Im}[\omega] = 0), the left and right eigenvectors become identical ($|s^l\rangle = |s^r\rangle = |s\rangle$). As \tanh[2\text{Im}(\omega)t] \to 0, the phase accumulation becomes strictly linear:

 \varphi_D = -\frac{1}{\hbar} \int_{0}^{\tau} \omega (-m) dt = \frac{m\omega\tau}{\hbar}

4. SPECIAL CASE: EXACT REAL SPECTRUM IN QUANTUM WALKS

For certain non-Hermitian quantum walks, the energy spectrum is E_\pm = \pm \omega(k,\theta) + i\ln \eta(k,\theta), where \omega is real. The non-Hermiticity acts as a global scalar e^{2\ln \eta \cdot t}, which cancels out in the density matrix:

 \rho(t) = \frac{e^{2\ln \eta \cdot t} \rho(0)}{e^{2\ln \eta \cdot t} \text{Tr}[\rho(0)]} = \rho(0)

The observable dynamical phase (real part) accumulates linearly, identical to Hermitian systems:

 \varphi_d(k,\tau) = \text{Re}\{\varphi_D\} = \frac{m \omega(k,\theta) \tau}{\hbar}

5. GEOMETRIC PHASE AND WINDING NUMBER

The geometric phase is \varphi_G(k,t) = \varphi_R(k,t) - \varphi_d(k,t). The winding number \nu(t) acts as a dynamical topological order parameter:

 \nu(t) = \oint_{\text{BZ}} dk \frac{\partial \varphi_G(k,t)}{\partial k}
[Image of winding number jumps at critical times]

Note: Quantized jumps in \nu(t) occur exactly at critical times t_c where the Loschmidt amplitude vanishes ($g_k(t_c) = 0$), signaling a Dynamical Quantum Phase Transition.

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