qml.gradients.stoch_pulse_grad¶

stoch_pulse_grad
(tape, argnum=None, num_split_times=1, sampler_seed=None, use_broadcasting=False)¶ Compute the gradient of a quantum circuit composed of pulse sequences by applying the stochastic parameter shift rule.
For a pulsebased cost function \(C(\boldsymbol{v}, T)\) with variational parameters \(\boldsymbol{v}\) and evolution time \(T\), it is given by (c.f. Eqn. (6) in Leng et al. (2022) with altered notation):
\[\frac{\partial C}{\partial v_k} = \int_{0}^{T} \mathrm{d}\tau \sum_{j=1}^m \frac{\partial f_j}{\partial v_k}(\boldsymbol{v}, \tau) \left[C_j^{(+)}(\boldsymbol{v}, \tau)  C_j^{()}(\boldsymbol{v}, \tau)\right]\]Here, \(f_j\) are the pulse envelopes that capture the time dependence of the pulse Hamiltonian:
\[H(\boldsymbol{v}, t) = H_\text{drift} + \sum_j f_j(\boldsymbol{v}, t) H_j,\]and \(C_j^{(\pm)}\) are modified cost functions:
\[\begin{split}C_j^{(\pm)}(\boldsymbol{v}, \tau)&= \bra{\psi^{(\pm)}_{j}(\boldsymbol{v}, \tau)} B \ket{\psi^{(\pm)}_{j}(\boldsymbol{v}, \tau)} \\ \ket{\psi^{(\pm)}_{j}(\boldsymbol{v}, \tau)} &= U_{\boldsymbol{v}}(T, \tau) e^{i (\pm \frac{\pi}{4}) H_j} U_{\boldsymbol{v}}(\tau, 0)\ket{\psi_0}.\end{split}\]That is, the \(j\)th modified time evolution in these circuit interrupts the evolution generated by the pulse Hamiltonian by inserting a rotation gate generated by the corresponding Hamiltonian term \(H_j\) with a rotation angle of \(\pm\frac{\pi}{4}\).
See below for a more detailed description. The integral in the first equation above is estimated numerically in the stochastic parametershift rule. For this, it samples split times \(\tau\) and averages the modified cost functions and the Jacobians of the envelopes \(\partial f_j / \partial v_k\) at the sampled times suitably.
 Parameters
tape (pennylane.QNode or QuantumTape) – quantum tape or QNode to differentiate
argnum (int or list[int] or None) – Trainable tape parameter indices to differentiate with respect to. If not provided, the derivatives with respect to all trainable parameters are returned.
num_split_times (int) – number of time samples to use in the stochastic parametershift rule underlying the differentiation; also see details
sample_seed (int) – randomness seed to be used for the time samples in the stochastic parametershift rule
use_broadcasting (bool) – Whether to use broadcasting across the different sampled splitting times. If
False
(the default), one set of modified tapes per splitting time is created, ifTrue
only a single set of broadcasted, modified tapes is created, increasing performance on simulators.
 Returns
If the input is a QNode, an object representing the Jacobian (function) of the QNode that can be executed to obtain the Jacobian. The type of the Jacobian returned is either a tensor, a tuple or a nested tuple depending on the nesting structure of the original QNode output.
If the input is a tape, a tuple containing a list of generated tapes, together with a postprocessing function to be applied to the results of the evaluated tapes in order to obtain the Jacobian.
 Return type
function or tuple[list[QuantumTape], function]
This transform realizes the stochastic parametershift rule for pulse sequences, as introduced in Banchi and Crooks (2018) and Leng et al. (2022).
Note
This function requires the JAX interface and does not work with other autodiff interfaces commonly encountered with PennyLane. Finally, this transform is not JITcompatible yet.
Note
This function uses a basic sampling approach with a uniform distribution to estimate the integral appearing in the stochastic parametershift rule. In many cases, there are probability distributions that lead to smaller variances of the estimator. In addition, the sampling approach will not reduce trivially to simpler parametershift rules when used with simple pulses (see details and examples below), potentially leading to imprecise results and/or unnecessarily large computational efforts.
Warning
This transform may not be applied directly to QNodes. Use JAX entrypoints (
jax.grad
,jax.jacobian
, …) instead or apply the transform on the tape level. Also see the examples below.Examples
Consider a pulse program with a single twoqubit pulse, generated by a Hamiltonian with three terms: the nontrainable term \(\frac{1}{2}X_0\), the trainable constant (over time) term \(v_1 Z_0 Z_1\) and the trainable sinoidal term \(\sin(v_2 t) (\frac{1}{5} Y_0 + \frac{7}{10} X_1)\).
jax.config.update("jax_enable_x64", True) dev = qml.device("default.qubit.jax", wires=2) def sin(p, t): return jax.numpy.sin(p * t) ZZ = qml.PauliZ(0) @ qml.PauliZ(1) Y_plus_X = qml.dot([1/5, 3/5], [qml.PauliY(0), qml.PauliX(1)]) H = 0.5 * qml.PauliX(0) + qml.pulse.constant * ZZ + sin * Y_plus_X def ansatz(params): qml.evolve(H)(params, (0.2, 0.4)) return qml.expval(qml.PauliY(1)) qnode = qml.QNode(ansatz, dev, interface="jax", diff_method=qml.gradients.stoch_pulse_grad)
The program takes the two parameters \(v_1, v_2\) for the two trainable terms:
>>> params = [jax.numpy.array(0.4), jax.numpy.array(1.3)] >>> qnode(params) Array(0.0905377, dtype=float64)
And as we registered the differentiation method
stoch_pulse_grad()
, we can compute its gradient in a hardware compatible manner:>>> jax.grad(qnode)(params) [Array(0.00109782, dtype=float64, weak_type=True), Array(0.05833371, dtype=float64, weak_type=True)] # results may differ
Note that the derivative is computed using a stochastic parametershift rule, which is based on a sampled approximation of an integral expression (see theoretical background below). This makes the computed derivative an approximate quantity subject to statistical fluctuations with notable variance. The number of samples used to approximate the integral can be chosen with
num_split_times
, the seed for the sampling can be fixed withsampler_seed
:qnode = qml.QNode( ansatz, dev, interface="jax", diff_method=qml.gradients.stoch_pulse_grad, num_split_times=5, # Use 5 samples for the approximation sampler_seed=18, # Fix randomness seed )
>>> jax.grad(qnode)(params) [Array(0.00207256, dtype=float64, weak_type=True), Array(0.05989856, dtype=float64, weak_type=True)]
We may activate the option
use_broadcasting
to improve the performance when running on classical simulators. Internally, it reuses intermediate results of the time evolution. We can compare the performance with a simple test:from time import process_time faster_grad_qnode = qml.QNode( ansatz, dev, interface="jax", diff_method=qml.gradients.stoch_pulse_grad, num_split_times=5, # Use 5 samples for the approximation sampler_seed=18, # Fix randomness seed use_broadcasting=True, # Activate broadcasting ) times = [] for node in [qnode, faster_grad_qnode]: start = process_time() jax.grad(node)(params) times.append(process_time()  start)
>>> print(times) # Show the gradient computation times in seconds. [55.75785480000002, 12.297400500000009]
Warning
As the option
use_broadcasting=True
adds a broadcasting dimension to the modified circuits, it is not compatible with circuits that already are broadcasted.Theoretical background
Consider a pulse generated by a timedependent Hamiltonian
\[H(\boldsymbol{v}, t) = H_\text{drift} + \sum_j f_j(v_j, t) H_j,\]where \(\boldsymbol{v}=\{v_j\}\) are variational parameters and \(t\) is the time. In addition, consider a cost function that is based on using this pulse for a duration \(T\) in a pulse sequence and measuring the expectation value of an observable. For simplicity we absorb the parts of the sequence before and after the considered pulse into the initial state and the observable, respectively:
\[C(\boldsymbol{v}, t) = \bra{\psi_0} U_{\boldsymbol{v}}(T, 0)^\dagger B U_{\boldsymbol{v}}(T, 0)\ket{\psi_0}.\]Here, we denoted the unitary evolution under \(H(\boldsymbol{v}, t)\) from time \(t_1\) to \(t_2\) as \(U_{\boldsymbol{v}(t_2, t_1)}\). Then the derivative of \(C\) with respect to a specific parameter \(v_k\) is given by (see Eqn. (6) of Leng et al. (2022))
\[\frac{\partial C}{\partial v_k} = \int_{0}^{T} \mathrm{d}\tau \sum_{j=1}^m \frac{\partial f_j}{\partial v_k}(\boldsymbol{v}, \tau) \widetilde{C_j}(\boldsymbol{v}, \tau).\]Here, the integral ranges over the duration of the pulse, the partial derivatives of the coefficient functions, \(\partial f_j / \partial v_k\), are computed classically, and \(\widetilde{C_j}\) is a linear combination of the results from modified pulse sequence executions based on generalized parametershift rules (see e.g. Kyriienko and Elfving (2022) or Wierichs et al. (2022) for more details and
param_shift()
for an implementation of the nonstochastic generalized shift rules) Given the parameter shift rule with coefficients \(\{y_\ell\}\) and shifts \(\{x_\ell\}\) for the singleparameter pulse \(\exp(i \theta H_j)\), the linear combination is given by\[\begin{split}\widetilde{C_j}(\boldsymbol{v}, \tau)&=\sum_{\ell=1} y_\ell \bra{\psi_{j}(\boldsymbol{v}, x_\ell, \tau)} B \ket{\psi_{j}(\boldsymbol{v}, x_\ell, \tau)} \\ \ket{\psi_{j}(\boldsymbol{v}, x_\ell, \tau)} &= U_{\boldsymbol{v}}(T, \tau) e^{i x_\ell H_j} U_{\boldsymbol{v}}(\tau, 0)\ket{\psi_0}.\end{split}\]In practice, the time integral over \(\tau\) is computed by sampling values for the time, evaluating the integrand, and averaging appropriately. The probability distribution used for the sampling may have a significant impact on the quality of the obtained estimates, in particular with regards to their variance. In this function, a uniform distribution over the interval \([0, t]\) is used, which often can be improved upon.
Examples
Consider the pulse generated by
\[H(\boldsymbol{v}, t) = \frac{1}{2} X_0 + v_1 Z_0 Z_1 + \sin(v_2 t) X_1\]and the observable \(B=Y_1\). There are two variational parameters, \(v_1\) and \(v_2\), for which we may compute the derivative of the cost function:
\[\begin{split}\frac{\partial C}{\partial v_1} &= \int_{0}^{T} \mathrm{d}\tau \ \widetilde{C_1}((v_1, v_2), \tau)\\ \frac{\partial C}{\partial v_2} &= \int_{0}^{T} \mathrm{d}\tau \cos(v_2 \tau) \tau \ \widetilde{C_2}((v_1, v_2), \tau)\\ \widetilde{C_j}((v_1, v_2), \tau)&= \bra{\psi_{j}((v_1, v_2), \pi/4, \tau)} B \ket{\psi_{j}((v_1, v_2), \pi/4, \tau)}\\ &\bra{\psi_{j}((v_1, v_2), \pi/4, \tau)} B \ket{\psi_{j}((v_1, v_2), \pi/4, \tau)} \\ \ket{\psi_{j}((v_1, v_2), x, \tau)} &= U_{(v_1, v_2)}(T, \tau) e^{i x H_j}U_{(v_1, v_2)}(\tau, 0)\ket{0}.\end{split}\]Here we used the partial derivatives
\[\begin{split}\frac{\partial f_1}{\partial v_1}&= 1\\ \frac{\partial f_2}{\partial v_2}&= \cos(v_2 t) t \\ \frac{\partial f_1}{\partial v_2}= \frac{\partial f_2}{\partial v_1}&= 0\end{split}\]and the fact that both \(H_1=Z_0 Z_1\) and \(H_2=X_1\) have two unique eigenvalues and therefore admit a twoterm parametershift rule (see e.g. Schuld et al. (2018)).
As a second scenario, consider the singlequbit pulse generated by
\[H((v_1, v_2), t) = v_1 \sin(v_2 t) X\]together with the observable \(B=Z\). You may already notice that this pulse can be rewritten as a
RX
rotation, because we have a single Hamiltonian term and the spectrum of \(H\) consequently will be constant up to rescaling. In particular, the unitary time evolution under the Schrödinger equation is given by\[\begin{split}U_{(v_1, v_2)}(t_2, t_1) &= \exp\left(i\int_{t_1}^{t_2} \mathrm{d}\tau v_1 \sin(v_2 \tau) X\right)\\ &=\exp(i\theta(v_1, v_2) X)\\ \theta(v_1, v_2) &= \int_{t_1}^{t_2} \mathrm{d}\tau v_1 \sin(v_2 \tau)\\ &=\frac{v_1}{v_2}(\cos(v_2 t_2)  \cos(v_2 t_1)).\end{split}\]As the
RX
rotation satisfies a (nonstochastic) twoterm parametershift rule, we could compute the derivatives with respect to \(v_1\) and \(v_2\) by implementing \(\exp(i\theta(v_1, v_2) X)\), applying the twoterm shift rule and evaluating the classical Jacobian of the mapping \(\theta(v_1, v_2)\).Using the stochastic parametershift rule instead will lead to approximation errors. This is because the approximated integral not only includes the shifted circuit evaluations, which do not depend on \(\tau\) in this example, but also on the classical Jacobian, which is not constant over \(\tau\). Therefore, it is important to implement pulses in the simplest way possible.