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Investigation of Perturbation Theory with Variational Quantum Algorithm

H.Davoodi Yeganeh [email protected] Faculty of Physics, Theoretical and astrophysics department , University of Tabriz, 51665-163 Tabriz, Iran
Abstract

Variational Quantum Algorithms are among the most promising systems to implement quantum computing under the Noisy-Intermediate Scale Quantum (NISQ) technology. In variational quantum algorithm, wavefunction represented by a parametrized ansatz and variational parameters are updated iteratively with a classical computer based on the measurement outputs from the quantum computer. In this paper, we investigate perturbation theory with these algorithms and prospect the possibility of using the variational quantum algorithm to simulate quantum dynamics in perturbation theory. We illustrate the use of algorithms with detailed examples which are in good agreement with analytical calculations.

Keyword: Variational quantum algorithms, Perturbation Theory, Time-dependent Hamiltonian, Near-term devices, Quantum dynamics

1 Introduction

We know that efficiently simulating quantum systems with high degrees of freedom is hard for classical computers due to the exponential growth of variables for characterizing these systems [1]. Quantum computers were proposed to solve such an exponential explosion problem, ranging from optimization to materials design, and the algorithms used in quantum computers have made great strides in the calculation and efficiency of various issues [2, 3, 4, 5]. Among the different approaches to quantum computing, the near-term quantum devices are mostly center around quantum simulations, which consists of a relatively low-depth quantum circuit by variational quantum algorithms. The variational algorithms were recently attracting a lot of attention, designed to utilize both quantum and classical resources to solve specific optimization tasks not accessible to traditional classical computers [6, 7, 8, 9, 10]. The main idea of this method is to divide the problem into two parts that each of performing a single task and can be implemented efficiently on a classical and a quantum computer. The significant benefit of this method is that it gives rise to a setup that can have much less strict hardware requirements and promising for NISQ [11] and devices typically have on the order of fewer qubits(contain from 1010 to 10310^{3} of qubits) with high gate fidelity and not fault-tolerant error correction. From a practical point of view, most of the current efforts concentrate on analog quantum computing methods such as quantum annealing [12, 13], and quantum adiabatic simulation[14, 15]. Recently, several variational quantum algorithms for specific tasks have been developed, and analog approaches can be approximately solved using gate model NISQ devices. These algorithms and their applications are progressing in various fields such as variations quantum eigensolver (VQE) which is a hybrid algorithm to approximate the ground state eigenvalues for quantum simulations [16, 4], quantum approximate optimization algorithm (QAOA) for finding an approximate solution of an optimization problem[5, 17], dissipative-system Variational Quantum Eigensolver(dVQE) to simulate Non-equilibrium steady states an open system [18], molecular simulations on a quantum computer [19],variational quantum state diagonalization (VQSD) [20] , also to simulate dynamics of open and closed systems[21, 22]. A complete overview of these algorithms is provided in Ref.[23, 24]. In quantum mechanics, few problems have exact solution, whether or not Hamiltonian is time-dependent. Hence, approximate methods have been proposed[25]. The approximate methods play a significant role in the study of different quantum systems. In general, we have three approximate methods; they are Perturbation Theory (PT)[26], Variational theory[27] and WKB approximation[28]. Here we focuse on PT, suppose there is a problem the Hamiltonian of which is represented by HH, for which the exact solution is not known. The Hamiltonian of the system can be described in terms of two terms; the Hamiltonian is written H=H0+λVH=H_{0}+\lambda V, in which H0H_{0} is called as the unperturbed Hamiltonian, and VV is called as the perturbation Hamiltonian, and λ\lambda is a continuous real parameter. It is important to realize that the system actually can be split in terms of these two Hamiltonians, and that should be known. In addition, there are two more conditions; one is that solution of the unperturbed Hamiltonian is completely known. The following condition, which is a stringen condition, that λ\lambda has to be much smaller than 1 (λ<<1)(\lambda<<1), which means the perturbation terms are much smaller compared to the original Hamiltonian H0H_{0}. In general, the PT can be divided into two categories, Time-Independent Perturbation Theory(TIPT) and Tim-Dependent Perturbation Theory(TDPT). In TIPT perturbation Hamiltonian, VV is independent of time, and in TDPT VV is dependent of time. Here, we consider TIPT, and TDPT, and investigate them with the variational quantum algorithm. In fact, in TDPT, we are dealing with a time-dependent Hamiltonian and try to find its spectrum (In the language of mathematics described in detail in Section 2). In this paper, we prospect the possibility of using a variational quantum algorithm to simulate quantum dynamics in TDPT and, TIPT. For this purpose, we employ time-dependent variational quantum algorithm introduced in Ref[21, 22, 29, 30, 31]. In this algorithm, the time-dependent quantum state is approximated by a parametrized quantum state and using McLachlan’s principle, the equation of motion for the variational parameters is obtained(described in detail in Section 3). The paper is organized as follows: In Section 2, we introduce Time-Independent and Time-Dependent Perturbation Theory. The variational quantum algorithm for quantum dynamics is described in Section 3. In Section 4, we present the numerical results. Finally, Section 5, gives the conclusions.

2 Perturbation Theory

Perturbation theory is widely used and plays an important role in describing real quantum systems, because it is impossible to find exact solutions to the Schrodinger equation for Hamiltonians even with moderate complexity. In general, the PT can be divided into two categories, TIPT and TDPT. In this section, we describe these two categories in detail.

2.1 Time-Independent Perturbation Theory

Time-independent perturbation theory is a mathematical tool for investigating quantum system which Hamiltonian is independent of time. Consider the time- independent Schrodinger equation

H|ψn=(H0+λV)|ψn=En|ψn,H|\psi_{n}\rangle=(H_{0}+\lambda V)|\psi_{n}\rangle=E_{n}|\psi_{n}\rangle, (1)

where |ψn|\psi_{n}\rangle and EnE_{n} are the nthn^{th} eigenstate and energy respectively. The H0H_{0} is unperturbed Hamiltonian and satisfies the time independent Schrodinger equation.Since, in TIPT, eigenstate and energy will be sought in the form of an expansion in powers of λ\lambda, After som calculation, in the first order approximation eigenstates and energies are expressed as

En=En(0)+n(0)|V|n(0)E_{n}=E_{n}^{(0)}+\langle n^{(0)}|V|n^{(0)}\rangle
|ψn=|n(0)mnVmnEm(0)En(0)|n.|\psi_{n}\rangle=|n^{(0)}\rangle-\sum_{m\neq n}\frac{V_{mn}}{E_{m}^{(0)}-E_{n}^{(0)}}|n\rangle. (2)

For second-order approximation, we have

En=En(0)+mn|Vmn|2Em(0)En(0),E_{n}=E_{n}^{(0)}+\sum_{m\neq n}\frac{|V_{mn}|^{2}}{E_{m}^{(0)}-E_{n}^{(0)}},
|ψn=|n(0)mnVmnEm(0)En(0)|m12mn|Vmn|2Em(0)En(0)|n+mn[lnVmnVln(Em(0)En(0))(El(0)En(0))]|m.|\psi_{n}\rangle=|n^{(0)}\rangle-\sum_{m\neq n}\frac{V_{mn}}{E_{m}^{(0)}-E_{n}^{(0)}}|m\rangle-\frac{1}{2}\sum_{m\neq n}\frac{|V_{mn}|^{2}}{E_{m}^{(0)}-E_{n}^{(0)}}|n\rangle+\sum_{m\neq n}[\sum_{l\neq n}\frac{V_{mn}V_{ln}}{(E_{m}^{(0)}-E_{n}^{(0)})(E_{l}^{(0)}-E_{n}^{(0)})}]|m\rangle. (3)

Denote the VmnV_{mn} and VlnV_{ln} are expectation value of VV as Vm(l)n=m(l)|V|nV_{m(l)n}=\langle m(l)|V|n\rangle.

2.2 Time-Dependent Perturbation Theory

In real world, there are many quantum systems of importance with time dependence, therefore, the dynamics of these systems must be examined by considering the time dependence. For a system described by a Hamiltonian H0H_{0}, which is time–independent, the most general state of the system can be described by a wavefunction |ψ(t)|\psi(t)\rangle which can be expanded in the energy eigenbasis {|n}\{|n\rangle\}as follows

|ψ(t)=ncn exp(iEnt/)|n,|\psi(t)\rangle=\sum_{n}c_{n}\text{ exp}(−iE_{n}t/\mathchar 1406\relax)|n\rangle, (4)

where the coefficients,cnc_{n} are time-independent and EnE_{n} is the eigenvalue corresponding to the energy eigenstate |n|n\rangle of H0H_{0}. For time dependent case, we consider a Hamiltonian HH as it can be split into two parts, that’s mean Hamiltonian is of the form

H=H0+V(t),H=H_{0}+V(t), (5)

we can again expand in, |n|n\rangle the time-independent eigenbasis of H0H_{0}

|ψ(t)=ncn(t) exp(iEnt/)|n,|\psi(t)\rangle=\sum_{n}c_{n}(t)\text{ exp}(−iE_{n}t/\mathchar 1406\relax)|n\rangle, (6)

but the coefficients, cnc_{n} will now in general be time-dependent. By using interaction picture and writing En=ωnE_{n}=\mathchar 1406\relax\omega_{n} and given that the wavefunction satisfies the time-dependent Schrödinger equation, we obtain

n(ic˙ncnV) exp(iωnt)|n=0.\sum_{n}(i\mathchar 1406\relax\dot{c}_{n}−c_{n}{V})\text{ exp}(−i\omega_{n}t)|n\rangle=0.

With simple calculations we have

ic˙m exp(iωmt)ncnVmn exp(iωnt)=0,i\mathchar 1406\relax\dot{c}_{m}\text{ exp}(−i\omega_{m}t)−\sum_{n}c_{n}V_{mn}\text{ exp}(−i\omega_{n}t)=0,

giving the following set of coupled, first–order differential equations for the coefficients

ic˙m=ncnVmn exp(iωmnt),i\mathchar 1406\relax\dot{c}_{m}=\sum_{n}c_{n}V_{mn}\text{ exp}(i\omega_{mn}t), (7)

where ωmn=ωnωn\omega_{mn}=\omega_{n}-\omega_{n} and Vmn=m|V|nV_{mn}=\langle m|V|n\rangle It can be seen that, the coefficient cmc_{m} varies with time i.e. the probability that a measurement will show the system to be in the mthm^{th} eigenstate. It is exact, but not terribly useful because we must, in general, solve an infinite set of coupled differential equations. Here, instead of solving differential equations, we obtain the dynamics of the time-dependent Hamiltonian with the variational quantum algorithm directly.

3 Variational Quantum Algorithm

For simulate the time-inpendent Hamiltonian dynamics, we employ variational quantum algorithm introduced in Ref[21, 22, 29, 30, 31]. In this algorithm, state |ψ(t)|\psi(t)\rangle is approximated by a parametrized state |ϕ(λ)|\phi(\vec{\lambda})\rangle, i.e.

|ψ(t)=exp(iHt)|ψ(0)|ϕ(λ),|\psi(t)\rangle=exp(-iHt)|\psi(0)\rangle\approx|\phi(\vec{\lambda})\rangle,

where λ={λ1(t),λ2(t).}\vec{\lambda}=\{\lambda_{1}(t),\lambda_{2}(t)....\} are variational parameters. By using time-dependent variational principle corresponding to the Schrödinger equation we have

=ψ(t)|itH|ψ(t)\mathcal{L}=\langle\psi(t)|\frac{i\partial}{\partial t}-H|\psi(t)\rangle (8)

where, \mathcal{L} is Lagrangian. By considering |ψ(t)|ϕ(λ)|\psi(t)\rangle\approx|\phi(\vec{\lambda})\rangle and using the Euler-Lagrange equation we have

qMpqλq˙=Vp,\sum_{q}M_{pq}\dot{\lambda_{q}}=V_{p}, (9)

where

Mp,q=iϕ(λ)|λk|ϕ(λ)λq+H.CM_{p,q}=i\frac{\partial\langle\phi(\vec{\lambda})|}{\partial\lambda_{k}}\frac{\partial|\phi(\vec{\lambda})\rangle}{\partial\lambda_{q}}+H.C (10)
Vp=ϕ|λpH|ϕ(λ)+H.CV_{p}=\frac{\partial\langle\phi|}{\partial\lambda_{p}}H|\phi(\vec{\lambda})\rangle+H.C (11)

For simulate the time-dependent Hamiltonian dynamics, we employ variational quantum algorithm introduced in Ref[21, 22, 29, 30, 31]. In this algorithm, state |ψ(t)|\psi(t)\rangle is approximated by a parametrized state |ϕ(λ)|\phi(\vec{\lambda})\rangle, i.e.

|ψ(t)=Texp(i0tH(t)𝑑t)|ψ(0)|ϕ(λ),|\psi(t)\rangle=Texp(-i\int^{t}_{0}H(t^{\prime})dt^{\prime})|\psi(0)\rangle\approx|\phi(\vec{\lambda})\rangle,

where λ={λ1(t),λ2(t).}\vec{\lambda}=\{\lambda_{1}(t),\lambda_{2}(t)....\} are variational parameters and TT is the time-ordering operator. By using McLachlan’s principle,( or Dirac and Frenkel variational principle) the equation of motion for the variational parameters is obtained by minimizing the quantity (itH)|ϕ(λ)||(i\frac{\partial}{\partial t}-H)|\phi(\vec{\lambda})\rangle||, so we have

λ(tn+1)=λ(tn)+λ˙δt\lambda(t_{n+1})=\lambda(t_{n})+\dot{\lambda}\delta t
iMkiλi˙=Vk.\sum_{i}M_{ki}\dot{\lambda_{i}}=V_{k}. (12)

where

Mki=Reϕ(λ)λk|ϕ(λ)λiVk=Imϕ(λ)|H|ϕ(λ)λk.\begin{split}M_{ki}=Re\langle\frac{\partial\phi(\vec{\lambda})}{\partial\lambda_{k}}|\frac{\partial\phi(\vec{\lambda})}{\partial\lambda_{i}}\rangle\\ V_{k}=Im\langle\phi(\vec{\lambda})|H|\frac{\partial\phi(\vec{\lambda})}{\partial\lambda_{k}}\rangle.\end{split} (13)

The coefficients of the differential Eq.( 13) are determined using a quantum computer, while each propagation step is carried out by classically solving the differential equation. To obtain high accuracy of algorithm, we must be sensitive in choosing the wavefunction ansatz. Here we consider an ansatz of the form

|ϕ(λ)=U(λ)|ϕ0=U(λ1)U(λ2)U(λi)U(λN)|ϕ0|\phi(\vec{\lambda})\rangle=U(\vec{\lambda})|\phi_{0}\rangle=U(\lambda_{1})U(\lambda_{2})...U(\lambda_{i})...U(\lambda_{N})|\phi_{0}\rangle

The evolution operator is unitary, so it is equivalent to a certain rotation in the Hilbert space of states .i.e.

U(λi)=exp(iλiΛi)=exp(ijλisi,jσ^i,j),U(\lambda_{i})=exp(-i\lambda_{i}\Lambda_{i})=exp(-i\sum_{j}\lambda_{i}s_{i,j}\hat{\sigma}_{i,j}), (14)

where Λi=jsi,jσ^i,j\Lambda_{i}=\sum_{j}s_{i,j}\hat{\sigma}_{i,j} where σ^i,j\hat{\sigma}_{i,j} are Pauli operators. So, we have,

U(λ)λi=U(λ1)U(λ2)ijsi,jσ^i,jU(λi).U(λN)U(λ)λi=U(λN).ijsi,jσ^i,jU(λi)U(λ2)U(λ1),\begin{split}\frac{\partial U(\vec{\lambda})}{\partial\lambda_{i}}=U(\lambda_{1})U(\lambda_{2})...-i\sum_{j}s_{i,j}\hat{\sigma}_{i,j}U(\lambda_{i})....U(\lambda_{N})\\ \frac{\partial U^{\dagger}(\vec{\lambda})}{\partial\lambda_{i}}=U^{\dagger}(\lambda_{N})....i\sum_{j}s^{*}_{i,j}\hat{\sigma}_{i,j}U^{\dagger}(\lambda_{i})...U^{\dagger}(\lambda_{2})U^{\dagger}(\lambda_{1}),\end{split} (15)

therefore the matrix elements of MM and VV are

Mki=Re(ϕ0|U(λ1)U(λN)ΛkU(λl)ΛiU(λi).U(λ1)|ϕ0)Vk=Im(ijcjϕ0|U(λ1)U(λN)hjU(λN)ΛkU(λk)U(λ1)|ϕ0),\begin{split}M_{ki}=Re(\langle\phi_{0}|U(\lambda_{1})^{\dagger}...U(\lambda_{N})^{\dagger}\Lambda_{k}^{\dagger}...U(\lambda_{l})^{\dagger}\Lambda_{i}U(\lambda_{i})....U(\lambda_{1})|\phi_{0}\rangle)\\ V_{k}=Im(i\sum_{j}c_{j}\langle\phi_{0}|U(\lambda_{1})^{\dagger}...U(\lambda_{N})^{\dagger}h_{j}U(\lambda_{N})...\Lambda_{k}U(\lambda_{k})...U(\lambda_{1})|\phi_{0}\rangle),\end{split} (16)

where the Hamiltonian expressed H=jcjhjH=\sum_{j}c_{j}h_{j}. The MkiM_{ki} and VkV_{k} are obtained in a quantum circuit via the Hadamard or Swap test. Note that the matrix elements in the first and second-order approximations i.e. Eq(2), Eq(3) and Eq(7) can be obtained by variational quantum algorithm.

4 Numerical Example

In this section, we numerically test the performance of the previously described variational quantum algorithm on some of the systems. In the first example, consider H2H_{2} molecule and find ground state energy H2H_{2}. We used a standard molecular basis set, the minimal STO-3G basis. Via JordanWigner or Bravyi-Kitaev transformation, the qubit-Hamiltonians of this molecule can be obtained. So,

H=g0I+g1Z0+g2Z1+g3Z0Z1+g4Y0Y1+g5X0X1,H=g_{0}I+g_{1}Z_{0}+g_{2}Z_{1}+g_{3}Z_{0}Z_{1}+g_{4}Y_{0}Y_{1}+g_{5}X_{0}X_{1}, (17)

where the coefficients gig_{i} were all derived in this classical preprocessing step and {Xi,Yi,Zi}\{X_{i},Y_{i},Z_{i}\} are Puali matrixs. Whit using TIPT we can divid this Hamiltinain in two trem,

H0=g0I+g1Z0+g2Z1+g3Z0Z1H_{0}=g_{0}I+g_{1}Z_{0}+g_{2}Z_{1}+g_{3}Z_{0}Z_{1}
H=g4Y0Y1+g5X0X1H^{\prime}=g_{4}Y_{0}Y_{1}+g_{5}X_{0}X_{1}

H0H_{0} is the unperturbed Hamiltonian and HH^{\prime} is the perturbation Hamiltonain. H0H_{0} is diagonal matrix and we can obtain eigenstate and energy HH by using TIPT. For variational quantum algorithm, we consider an anstaz of the form

|ψ(λ)=eiλ1X0Y1eiλ2Z0I1|01|\psi(\vec{\lambda})\rangle=e^{i\lambda_{1}X_{0}Y_{1}}e^{i\lambda_{2}Z_{0}I_{1}}|01\rangle

. Output of variational algorithm compared it to TIPT solution ground state energy as shown in figure 1. Also we implement a quantum circuitfor evaluating coefficients on quantum processor in figure 2

Refer to caption
Figure 1: Energy curves of the molecular hydrogen ground state in the two cases TIPT and Variational method
Refer to caption
Figure 2: Quantum circuit used in the finding ground state energy H2H_{2} molecule. This circuit employed to evaluate coefficients. The ancilla qubit on the top line undergoes Hadamard gates HH and unitary operations nd controls operations apply on initial state |01|01\rangle

In second example let us consider a two-state system with

H0=E1|00|+E2|11|H_{0}=E_{1}|0\rangle\langle 0|+E_{2}|1\rangle\langle 1|
V(t)=δeiωt|01|+δeiωt|10|.V(t)=\delta e^{i\omega t}|0\rangle\langle 1|+\delta e^{-i\omega t}|1\rangle\langle 0|.

Whit TDPT, we can obtain

ic˙=δ(ei(ωω21)t|01|+ei(ωω21)t|10|)c,i\mathchar 1406\relax\vec{\dot{c}}=\delta(e^{i(\omega-\omega_{21})t}|0\rangle\langle 1|+e^{-i(\omega-\omega_{21})t}|1\rangle\langle 0|)\vec{{c}},

where c\vec{{c}} is the two-component vector c=(c1(t),c2(t))\vec{{c}}=(c_{1}(t),\ c_{2}(t))and ω21=(E2E1)/\omega_{21}=(E_{2}-E_{1})/\mathchar 1406\relax. With the initial condition c1(0)=1c_{1}(0)=1, and c2(0)=0c_{2}(0)=0 this equation has the solution

|c2(t)|2=4δ2δ2+2(ωω21)2sin2Ωt|c1(t)|2=1|c2(t)|2|c_{2}(t)|^{2}=\frac{4\delta^{2}}{\delta^{2}+\mathchar 1406\relax^{2}(\omega-\omega_{21})^{2}}sin^{2}\Omega t\qquad|c_{1}(t)|^{2}=1-|c_{2}(t)|^{2} (18)

where Ω=((δ/)2+(ωω21)2/4)1/2\Omega=((\delta/\mathchar 1406\relax)^{2}+(\omega-\omega_{21})^{2}/4)^{1/2} is known as the Rabi frequency. The solution, which varies periodically in time, describes the transfer of probability from state 0 to state 1 and back. For variational quantum algorithm, we consider an anstaz of the form

|ψ(λ)=eiλ1Zeiλ2X|0|\psi(\vec{\lambda})\rangle=e^{i\lambda_{1}Z}e^{i\lambda_{2}X}|0\rangle

Output of variational algorithm compared it to TDPT solution the transfer of probability from states as shown in figure 3. Also We propose a quantum circuit for evaluating coefficients on quantum processor in figure 4

Refer to caption
Figure 3: Probability of transition in the two cases TDPT and Variational method for t=1t=1. The orange and blue lines corresponds to the probability |c1(t)|2|c_{1}(t)|^{2} and |c2(t)|2|c_{2}(t)|^{2} respectively.
Refer to caption
Figure 4: Quantum circuit used in the second example to evaluate coefficients. The ancilla qubit on the top line undergoes Hadamard gates HH and unitary operations nd controls operations apply on initial state |0|0\rangle

5 Conclusion

We have considered a variational quantum algorithm for investigation of perturbation theory. We considered perturbation theory as two categories, time-independent perturbation theory and time-dependent perturbation theory. We have used a variational quantum algorithm which, exact state is approximated by a parametrized state and variational principle. In the case TIPT and, TDPT using the time-dependent variational principle and McLachlan’s principle corresponding to the Schrödinger equation, respectively, we obtained the differential equations for simulating dynamics. We compare the analytical and numerical results obtained from the exact solution with the variational quantum algorithm which, are in good agreement with each other.

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