# Spin qubits

Semiconductor quantum dots are small devices in which charge carriers are confined in all three dimensions: this can be achieved by electrical gating and/or etching techniques applied e. g. to a two-dimensional electron gas.

In the quantum-dot scenario either the electron spin or the charge (orbital) degrees of freedom can be chosen as the qubit. Here we will describe the spin dot which has two immediate advantages:

1. the qubit represented by a real spin-1/2 is always well-defined as the two-dimensional Hilbert space is the entire space available and therefore there are no extra dimensions into which the qubit state could "leak";
2. real spins have quite long dephasing times (order of microseconds in GaAs).

In order to be able to perform quantum computation, in addition to a well-defined qubit, we also need a controllable source of entanglement, i. e. a mechanism by which two specific qubits at a time can be entangled so as to produce the fundamental CNOT gate operation. This can be achieved by temporarily coupling two spins via the Heisenberg Hamiltonian

Hs(t) = J(t)1 ⋅ 2,  where  J(t) = 4t02(t)/U is the time dependent exchange constant produced by turning on and off the tunneling matrix element  t0(t),  U is the charging energy of a single dot, and  i is the spin-1/2 operator for the i-th dot. The Heisenberg Hamiltonian  Hs(t) provides a good description of the quantum-dot system if the following conditions are met:

1.  ΔE ≫ kT (where  ΔE is the level spacing and  T is the temperature) so that higher-lying single-particle states of the dots can be ignored;
2. τs ≫ ℏ/ΔE (where  τs is the time scale for pulsing the gate potential "low") in order to prevent transitions to higher orbital levels;
3.  U > t0(t) ∀t, in order for the Heisenberg-exchange approximation to be accurate;
4.  Γ − 1 ≫ τs, where  Γ − 1 is the decoherence time.

In general the decoherence times of the electron spins are longer than those of the charge degrees of freedom, since the former are insensitive to environmental fluctuations of the electric potential.

Condition 1. above ensures that we can focus on the two lowest orbital eigenstates which are the spin singlet and the spin triplet. The general Hamiltonian  Horb can thus be effectively replaced by the Heisenberg spin Hamiltonian  Hs where the exchange constant  J0 = εt − εs is the difference between the triplet and singlet energy.

In this setting, quantum computing can be achieved by applying the unitary time evolution operator  Us(t) = Texp{ − i∫0tHs(tʹ)dtʹ} to the initial state of the two spins:  ∣Ψ(t)⟩ = Us∣Ψ(0)⟩. For a specific duration  τs of the spin-spin coupling such that  ∫J(t)dt = J0τs = π(mod 2π), the pulsed Heisenberg Hamiltonian  Hs(t) leads to the swap operatorUswap ≡ Us(J0τs = π). This operation conserves the total angular momentum of the system and therefore is not sufficient by itself to perform useful quantum computing. However, we can pulse the interaction for just half the duration and thus obtain the square root of swap which is a fundamental quantum gate in the implementation, for instance, of the CNOT:

$$\; U_{CNOT} = e^{i\frac{\pi}{2}S_1^z}e^{-i\frac{\pi}{2}S_1^z}U_{swap}^{1/2} e^{i \pi S_1^z}U_{swap}^{1/2} ,$$ where  eiπS1z etc. are single-qubit operations and  Uswap1/2 is the square root of swap.

#### One-qubit gates

We have seen how to obtain the two-qubit operations swap gate and root of swap gate but we still have to see how to implement one-qubit gates. Single-qubit rotations such as  eiπS1z can be achieved by pulsing a magnetic field  i exclusively onto the i-th spin. This could be done with:

1. a scanning-probe tip;
2. an auxiliary dot.

In the latter case the auxiliary dot (FM) is made of an insulating, ferromagnetically-ordered material that can be connected to the i-ht dot of interest , (i = 1, 2), by the same kind of electrical gating which connects the two spins in the Heisenberg Hamiltonian  Hs. If we want a magnetic field  i to be pulsed exclusively onto the i-th spin, we just have to lower the barrier between the FM dot and the i-th dot so that the electron's wavefunction overlaps with the magnetized region for a fixed time  τs. Thus, during this time, the Hamiltonian for the qubit on the i-th dot will contain a Zeeman term which leads to the single-qubit rotation. Therefore the i-th spin is rotated and the corresponding Hamiltonian is

∫0τsHsBdt = ∑i = 12ωiτsSiz,  with  ωi = gμBBiz, where  g is the effective g-factor,  μB the Bohr magneton and  Biz the magnetic field acting on the i-th spin in the z direction.

• D. Loss, D. P. DiVincenzo, Phys. Rev. A 57, 120 (1998)
• G. Burkard, D. Loss, D. P. DiVincenzo, Phys. Rev. B 59, 2070 (1999)