Recent advances in hole-spin qubits Yinan Fang1 Pericles Philippopoulos2 Dimitrie Culcer34 W. A. Coish5 and Stefano Chesi67

2025-04-29 0 0 1.79MB 46 页 10玖币
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Recent advances in hole-spin qubits
Yinan Fang1, Pericles Philippopoulos2, Dimitrie Culcer3,4, W.
A. Coish5, and Stefano Chesi6,7
1School of Physics and Astronomy, Yunnan University, Kunming 650091, China
2Nanoacademic Technologies Inc., Montréal QC, Canada
3School of Physics, University of New South Wales, Sydney NSW 2052, Australia
4Australian Research Council Centre of Excellence in Future Low-Energy Electronics
Technologies, The University of New South Wales, Sydney NSW 2052, Australia
5Department of Physics, McGill University, Montréal QC, Canada
6Beijing Computational Science Research Center, Beijing 100193, China
7Department of Physics, Beijing Normal University, Beijing 100875, China
E-mail: stefano.chesi@csrc.ac.cn
Abstract. In recent years, hole-spin qubits based on semiconductor quantum dots
have advanced at a rapid pace. We first review the main potential advantages of these
hole-spin qubits with respect to their electron-spin counterparts, and give a general
theoretical framework describing them. The basic features of spin-orbit coupling and
hyperfine interaction in the valence band are discussed, together with consequences on
coherence and spin manipulation. In the second part of the article we provide a survey
of experimental realizations, which spans a relatively broad spectrum of devices based
on GaAs, Si, or Si/Ge heterostructures. We conclude with a brief outlook.
Nearly 25 years have passed since the idea of implementing quantum information
processing with semiconductor quantum dots was put forward [1]. The spin of confined
electrons (or holes) is a natural two-level system, relatively well shielded from charge
fluctuations and which, as it has been now established, can be coherently manipulated
with high accuracy and speed. Research in the field has been constantly progressing over
the years, exploring at the same time the rich physics of these semiconductor devices,
but is still restricted to the few-qubits regime. At the moment it is not yet obvious
which platform offers better prospects to realize intermediate- or large-scale devices,
and recently hole-spin devices have gained prominence.
Recent rapid progress in controlling hole spins has brought breath of fresh air to
the field. However, the potential advantages (and disadvantages) of these qubits over
their electron-spin counterparts should be carefully weighted. To get some perspective,
it is interesting to discuss how this family of spin qubits fits the main line of progress,
dominated by electron-spin devices. Within about 10 years from the 1998 theoretical
proposal, all the main ingredients required to realize quantum information processing,
such as spin readout, single-spin manipulation, and controllable spin-spin exchange
interactions, were firmly established. An account of early progress can be found in
the 2007 review Ref. [2]. In this initial phase, the most successful qubits were planar
arXiv:2210.13725v2 [cond-mat.mes-hall] 6 Feb 2023
Recent advances in hole-spin qubits 2
(lateral) quantum dots in AlGaAs/GaAs heterostructures. However, these systems are
susceptible to strong dephasing caused by nuclear spins. This dephasing is unavoidable
in III-V semiconductors since every isotope of Ga and As has a finite nuclear spins.
To remedy this situation, Si electron-spin devices have gradually emerged as a better
alternative. Coherent singlet-triplet oscillations in a Si/SiGe double quantum dot were
demonstrated in 2012 [3] and a number of landmark results have been obtained so
far, such as high-fidelity (>99.9%) single-qubit manipulation [4, 5], strong coupling
of spin qubits to a superconducting resonator [6–9] and, very recently, two-qubit
quantum processors with gate fidelities surpassing the fault-tolerance threshold [10–12]
and universal operation of a six-qubit array [13].
Hole-spin qubits fit naturally into the historical path, as they can overcome the
influence of nuclear spins in the same way as electron-spin devices based on Si: For
hole-spin qubits in Si and Ge, the low natural abundance of spinful nuclei can be further
reduced by isotopic purification. Furthermore, even in III-V semiconductors, holes are
much less affected by nuclear spins than conduction-band electrons. The Fermi contact
interaction vanishes, leading to an anisotropic hyperfine interaction caused by dipolar
and orbital terms, weaker by about an order of magnitude. In addition to having
a weaker influence of nuclear spins, two attractive features of holes should facilitate
scalability. The first is the absence of a valley degree of freedom. The valley splitting
of electrons in Si quantum dots depends on atomistic features of the device, which are
difficult to control uniformly over large quantum-dot arrays. The second and most
important feature is the strong spin-orbit interaction of holes, allowing in-situ electric
control of spin couplings and effective spin manipulation through a local electric drive.
In contrast, the spin-orbit coupling of conduction electrons in Si is weak, and single-spin
manipulation (as well as coupling of the spin to superconducting resonators) requires
large auxiliary elements, such as micromagnets [14,15].
Strong spin-orbit coupling is, of course, a double-edged sword, as it enhances the
influence of charge noise on the spin degrees of freedom. Despite this general difficulty,
and the late start of hole devices in terms of fabrication, in recent years hole-spin qubits
have achieved remarkable results. In many aspects concerning single-spin manipulation
[16–19], scalability [20,21], as well as coupling to superconducting circuits [22], hole-spin
qubits can approach and sometimes already surpass the performance of electron-spin
qubits.
To describe recent progress in hole-spin qubits, we have structured the article in two
main parts. Section 1 gives a theoretical perspective, introducing the general framework
for hole-spin qubits and the main interactions affecting them. Section 2 is a survey of
various experimental platforms, highlighting some of the most interesting achievements.
While the present review does not aim to be complete, it should offer an informative
and sufficiently broad view of hole-spin qubits. Recently, two more specialized reviews
have appeared: Ref. [23], focusing on hole spins in GaAs lateral quantum dots, and
Ref. [24], reviewing hole-based Ge devices. For a more complete perspective on spin
qubits (including electron-spin systems), one could consult Ref. [25].
Recent advances in hole-spin qubits 3
1. General description of hole-spin qubits
Quantum dots for use in information processing are typically based on either III-V
compound semiconductors such as GaAs, which have zincblende lattices, or on group-
IV semiconductors such as Si and Ge, with diamond lattices. While the conduction band
is formed by s-like atomic wave functions, resulting in spin-1/2quasiparticles, valence-
band states in diamond and zincblende semiconductors are predominantly formed by
atomic p-orbitals. In the atomic limit, combining the L= 1 orbital angular momentum
with the electron spin-1/2we obtain two possibilities for the total angular momentum
J, henceforth also referred to as (effective) spin: J= 3/2or J= 1/2. At zero crystal
momentum kthese states are separated by a gap and the band originating from the
J= 1/2manifold, which is always lower in energy, is known as the split-off band.
More precisely, since rotational symmetry is broken in the crystal, the valence-band
states at k= 0 are classified by the Γ8and Γ7representations of the tetrahedral double
group Td[26, 27]. Furthermore, the crystalline potential leads to the hybridization of p
orbitals with dstates [28–32], which can significantly affect the form of the hyperfine
interaction [33, 34] (see Section 1.3). Despite these caveats, the fourfold degeneracy
of atomic J= 3/2states (corresponding to Γ8) is preserved. The existence of the
split-off band makes a difference for numerical values, especially in Si, but properties of
holes are usually well understood considering the states at the top of the valence band.
Therefore, the following Luttinger Hamiltonian [35, 36] is often taken as a fundamental
starting point for the description of holes:
HL(k) = γ1+5
2γ2~2k2
2m0
+γ2
~2
m0
(k2
xJ2
x+k2
yJ2
y+k2
zJ2
z)
+γ3
~2
2m0
({kx, ky}{Jx, Jy}+ c.p.),(1)
where {Ji}are spin-3/2matrices, γ1,γ2and γ3are the Luttinger parameters, m0is the
bare electron mass, {A, B}= (AB +BA)/2, and c.p. are terms obtained from cyclic
permutations of x, y, z. In contrast with conduction electrons, where perturbative spin-
orbit interactions arise from the valence band and are suppressed by the large band gap of
the semiconductor, the Hamiltonian describing the valence-band holes [Eq. (1)] features
a strong spin-orbit coupling between kand J. This coupling results in a splitting of the
fourfold degeneracy at k= 0 into two doubly degenerate bands at finite momentum.
The higher (lower) valence band states are denoted as heavy (light) holes, with angular
momentum Jz=±3/2(±1/2) in the limit k0. Since γ2,3are generally of the
same order as γ1, the spin-orbit splitting between heavy-hole and light-hole bands is
comparable to the total kinetic energy.
Envelope function approximation. In the presence of smooth external potentials
and magnetic fields, the microscopic Bloch wave at k= 0 is modulated by a slowly-
varying envelope that satisfies a multi-component Shrödinger equation [36, 37]. The
usual prescription for electronic states is to replace ~kπ=i~+eA(r)(e < 0
is the electron charge) in HL, where A(r)is the vector potential associated with the
Recent advances in hole-spin qubits 4
external magnetic field B. As usual, the components of the canonical momentum π
do not commute, in general, thus in the second line of Eq. (1) we have specified the
appropriate symmetrized products of k(which become unnecessary when B= 0). Some
care should be taken in writing the Hamiltonian for the state of a missing electron. First,
the electronic energy is subtracted from a filled valence band, which can be simply
accounted for by a global change of sign in the Hamiltonian. This leads to the following
Hamiltonian describing holes within the envelope-function approximation:
Henv =HL(π/~) + eV (r)+2κµBJ·B+ 2qµBJ·B,(2)
where eV (r)is the 3D confining potential and the last two terms describe the Zeeman
interaction [35, 36], with J=J3
x, J3
y, J3
zand µBthe Bohr magneton. While Eq. (2)
is a legitimate choice, giving the correct energy of the hole states, it still refers to the
electronic wavefunction and this should be taken into account when computing certain
observables. Recall, in particular, that a hole with quantum numbers (k, Jz)corresponds
to a missing (k,Jz)electronic state. To obtain directly the hole wavefunction, whose
angular momentum corresponds to the physical state, one can consider an alternative
version of Henv, by applying time-inversion to it. Since i~+i~upon time
inversion, the transformed Hamiltonian recovers the Peierls substitution appropriate for
a positively charged particle, i.e., π→ −i~eA(r)in Eq. (2). Furthermore, the
second and third terms of Eq. (2) change sign, since J→ −J.
Inversion-asymmetry and strain. In III-V zincblende materials, for which there is
no center of inversion symmetry, it is sometimes important to supplement Eq. (1) with
additional terms. These corrections are known as Dresselhaus spin-orbit couplings and
include the k-linear term:
H1=2
3Ckkx{Jx, J2
yJ2
z}+ c.p.,(3)
and a more convoluted k-cubic contribution [36]:
H3=b41 {kx, k2
yk2
z}Jx+ c.p.+b42 {kx, k2
yk2
z}J3
x+ c.p.
+b51 {kx, k2
y+k2
z}{Jx, J2
yJ2
z}+ c.p.+b52 k3
x{Jx, J2
yJ2
z}+ c.p..(4)
In particular, the k-cubic terms were shown early on to give a significant spin-orbit
splitting in symmetric GaAs quantum wells [38]. A recent theoretical analysis [39] has
assessed the relative importance of H1over H3in GaAs 2DHGs. Furthermore, a different
type of coupling induced by inversion-asymmetry, but also depending on the external
potential V(r), has been discussed [39]:
HE=eaBχ
3[Ex{Jy, Jz}+ c.p.],(5)
where E=Vis the local electric field, aBis the Bohr radius, and χis a material
parameter. Equation (5), which involves the gradient of the potential and includes
interband matrix elements between heavy- and light-hole states, goes beyond the
Recent advances in hole-spin qubits 5
usual envelope-function approximation. Such pseudospin-electric coupling physically
originates from the interaction between the electric field and the dipole operator, which
takes the general form of Eq. (5) when expressed in the subspace of valence-band states.
A first-principles evaluation gives a relatively large value χ'0.2in GaAs [39].
For Si and Ge, the above Dresselhaus terms are absent in the bulk. However, it is
important to account for finite strain when modelling, e.g., high-mobility SiGe/Ge/SiGe
quantum wells [40, 41] as well as core-shell nanowires [42, 43]. In general, the effect of
strain is described by the well-known Bir-Pikus Hamiltonian Hε=(av+5
4bv)(εxx +
εyy +εzz ) + bv(J2
xεxx + c.p.) + 2
3dv({Jx, Jy}εxy + c.p.), where {εij }are the strain tensor
elements and av, bv, dvare material-specific deformation potentials [44]. Assuming that
only hydrostatic and uniaxial strain are present, i.e., εxy =εyz =εzx = 0 and εxx =εyy,
the effect of Hεis to induce different offsets for the heavy-hole (Jz=±3/2) and light-hole
(Jz=±1/2) states [40–42].
1.1. Spin-orbit interaction of confined holes
The description of confined hole systems can be based directly on the general four-band
formalism just described, eventually supplemented by the split-off band. However,
many of the hole-spin qubits of interest are fabricated from low-dimensional systems
such as quantum wells or nanowires, where additional gates realize the zero-dimensional
confinement. It is therefore useful to describe the effective Hamiltonians governing such
2D or 1D systems. Because such effective models are relatively simple, they are often
taken as starting points to characterize various important effects, such as spin relaxation
or electrical manipulation of spin qubits.
Quantum wells. For quasi-2D holes the potential in Eq. (2) may be taken as V(z)
if the growth direction is along a main crystal axis. Then, for B= 0 and zero in-
plane wavevector, kk= (kx, ky) = (0,0), Eq. (2) simplifies considerably, giving two
decoupled Schrödinger equations in 1D. The two sectors correspond to the Jz=±3/2
and Jz=±1/2subspaces, characterized by different effective masses m0/(γ1±2γ2).
The lowest-energy subband is formed by heavy-holes (Jz=±3/2) and the energy gap
to the lowest light-hole subband can be estimated as LH '2γ2(π~/L)2/m0, assuming
an infinite potential well of width L. For more realistic scenarios, the value of LH
depends of the detailed shape of V(z)and, as discussed already, is modified by uniaxial
strain. In general, the four-dimensional degeneracy of the Luttinger Hamiltonian has
been broken by the confining potential, generating naturally a two-level pseudospin. For
the low-energy states, we can identify the effective spin up/down eigenstates with the
Jz=±3/2eigenvalues, i.e., |⇑i =|+3/2iand |⇓i =|−3/2i.
Despite the simple decoupling described above (which, we stress, is exact only at
zero in-plane momentum), the light-hole/heavy-hole mixing terms still play a crucial role
in the effective 2D Hamiltonian. As seen from Eq. (1), finite values of kx,y will induce
matrix elements between the two subspaces, through the action of the Jx,y operators.
It is this coupling between light- and heavy-hole subbands what generates the desired
摘要:

Recentadvancesinhole-spinqubitsYinanFang1,PericlesPhilippopoulos2,DimitrieCulcer3;4,W.A.Coish5,andStefanoChesi6;71SchoolofPhysicsandAstronomy,YunnanUniversity,Kunming650091,China2NanoacademicTechnologiesInc.,MontréalQC,Canada3SchoolofPhysics,UniversityofNewSouthWales,SydneyNSW2052,Australia4Australi...

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