Construction of ecient Schmidt number witnesses for high-dimensional quantum states Nikolai Wyderka1Giovanni Chesi2Hermann Kampermann1Chiara Macchiavello2and Dagmar Bru1

2025-04-27 0 0 982.02KB 7 页 10玖币
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Construction of efficient Schmidt number witnesses for
high-dimensional quantum states
Nikolai Wyderka,1Giovanni Chesi,2Hermann Kampermann,1Chiara Macchiavello,2and Dagmar Bruß1
1Institut f¨ur Theoretische Physik III, Heinrich-Heine-Universit¨at D¨usseldorf,
Universit¨atsstr. 1, D-40225 D¨usseldorf, Germany
2Istituto Nazionale di Fisica Nucleare Sezione di Pavia, Via Agostino Bassi 6, I-27100 Pavia, Italy
(Dated: March 1, 2023)
Recent progress in quantum optics has led to setups that are able to prepare high-dimensional
quantum states for quantum information processing tasks. As such, it is of importance to benchmark
the states generated by these setups in terms of their quantum mechanical properties, such as their
Schmidt numbers, i.e., the number of entangled degrees of freedom.
In this paper, we develop an iterative algorithm that finds Schmidt number witnesses tailored to
the measurements available in specific experimental setups. We then apply the algorithm to find a
witness that requires the measurement of a number of density matrix elements that scales linearly
with the local dimension of the system. As a concrete example, we apply our construction method
to an implementation with photonic temporal modes.
I. INTRODUCTION
Over the course of the last decades, different physical
platforms have been developed to perform quantum in-
formational tasks. The requirements for such platforms
have been formalized at various occasions. One of the
most often used list of requirements was formulated by
DiVincenzo, and includes among other things the capa-
bility of robust state preparation, state manipulation and
measurements [1]. While most platforms available today
are limited to the generation and manipulation of qubits,
it has become more and more evident over the last years
that higher-dimensional systems can provide advantages
in specific tasks including quantum communication [2–
7] and quantum computing (see Ref. [8] and references
therein). However, embedding these additional degrees
of freedom in trapped ions or superconducting qubits
has been challenging [9, 10]. In contrast, time-energy
degrees of freedom in photonic states can be used to
encode very high-dimensional quantum states. Further-
more, using quantum pulse gates allows for robust and
precise manipulation and measurement of these signals,
and therefore provides a viable candidate for a platform
for high-dimensional quantum tasks [11].
In this paper, we develop theoretical tools that help
to characterize the state preparation capabilities of these
and similar setups. Recent work focused on the con-
struction of high-dimensional entanglement witnesses for
these setups that allow for efficient entanglement detec-
tion of the prepared quantum states [12, 13]. In this
work, we construct easily measurable Schmidt number
witnesses for such setups. Apart from detecting whether
a state is entangled, the Schmidt number of a state car-
ries additional information about the dimensionality of
the entanglement. We develop an algorithm to generate
witness candidates that use only few of the experimen-
tally available measurement settings. Consequently, we
then apply the algorithm to the measurements available
in the setup described in Ref. [11] and show that the
obtained observable indeed is a proper Schmidt number
witness, i.e., it certifies the Schmidt number of the gen-
erated quantum state. While proposals exist to certify
Schmidt numbers with measurements in only two local
bases [14], these ideas do not apply to the setup at hand,
as here only certain linear combinations of the entries of
the density matrix can be measured.
The paper is organized as follows. In section II we re-
view the notion of Schmidt numbers and Schmidt num-
ber witnesses, in section III we develop and explain the
algorithm that generates Schmidt number witness candi-
dates. In Section IV we apply the algorithm to obtain a
Schmidt number witness using only O(d) measurement
settings to certify the Schmidt number of the generated
states, and compare its noise robustness to that of other
Schmidt number witnesses. In the Appendix, we provide
an explicit construction for an experiment using photonic
temporal modes.
II. SCHMIDT NUMBERS AND SCHMIDT
NUMBER WITNESSES
Throughout this paper, we consider bipartite quantum
systems in CdCd. We denote the set of linear maps
from Cdto itself by Md.
The Schmidt number of a bipartite quantum state is
an entanglement measure that is related to the hardness
of generating a quantum state using local operations and
classical communication [15]. For pure states, it is de-
fined as the number of non-vanishing Schmidt coefficients
in the Schmidt decomposition of the state, i.e., for ev-
ery bipartite quantum state |ψi, written in the compu-
tational basis as
|ψi=
d1
X
i,j=0
cij |iiA|jiB,(1)
one can find local orthonormnal bases, {|iiA},{|jiB}for
arXiv:2210.05272v2 [quant-ph] 28 Feb 2023
2
subsystems Aand B, respectively, such that
|ψi=
k1
X
i=0
λi|iiA|iiB,(2)
where λiR, λi>0 and Pk1
i=0 λ2
i= 1. The kdnon-
vanishing numbers λiare called Schmidt coefficients of
|ψi, and kis called the Schmidt rank of |ψi, or SR(|ψi) in
short [16]. In order to generalize this measure to mixed
states ρ, one uses the convex roof construction of the
Schmidt rank, called Schmidt number, or SN(ρ) [17]:
SN(ρ) := min
ρ=Pipi|ψiihψi|max
iSR(|ψii),(3)
i.e., it is given by the maximal Schmidt rank within a
given decomposition of ρ, minimized over all decompo-
sitions. Due to the minimization, it is usually hard to
calculate the Schmidt number of a given quantum state.
For a bipartite system of dimension d×d, the maximal
Schmidt number is given by d, and one can define the sets
of Schmidt number kas
Sk={ρ: SN(ρ)k}.(4)
Clearly, SkSk+1, and S1is the usual set of sep-
arable states. The maximally entangled state |φ+i=
1
dPd1
i=0 |iiiis member of Sd, but not Sd1, and it can
be shown that [17, 18]
hφ+|ρk|φ+i ≤ k
d(5)
for all states ρkSk.
In order to certify a specific Schmidt number experi-
mentally, it is useful to define an analogon to entangle-
ment witnesses for Schmidt numbers [19]. We say that
an observable Wkis a Schmidt-number-(k+ 1) witness,
if
Tr(Wkρk)0 for all ρkSk,
Tr(Wkρ)<0 for at least one ρ.
Thus, whenever one finds in an experiment that
Tr(Wkρ)<0, then ρmust have at least Schmidt number
k+ 1. Note that for k= 1, we recover the usual notion
of an entanglement witness [16]. An important exper-
imental advantage of using theses witnesses lies in the
fact that a negative expectation value certifies a certain
Schmidt number for any experimental input state, pure
or mixed. In order to certify that a given observable is a
Schmidt-number-(k+ 1) witness, it is sufficient to min-
imize its overlap w.r.t. pure states in Skand show that
the minimum is non-negative. This can be seen from the
fact that the sets Skare compact, thus, one can find a
(potentially mixed) optimal quantum state ρ?
ksuch that
ck:= minρkSkTr(Wkρk) = Tr(Wkρ?
k). As SN(ρ?
k)k,
it exhibits a decomposition ρ?
k=Pipi|ψiihψi|with
SR(|ψii)k. Thus, ck=Pipihψi|Wk|ψii ≥ Pipick=
Figure 1. The sets Skof states of Schmidt number kfor d= 3,
as well as their outer approximations SR
kdefined in Eq. (8).
ck, implying that the inequality is an equality and each
of the pure |ψiiachieves the same minimal value of ck.
The observation of Eq. (5) can be directly transformed
into a Schmidt-number-(k+1) witness via the observable
[19]
Wk=1d2d
k|φ+ihφ+|.(6)
We refer to this witness as the standard Schmidt-number
witness, and we will compare our constructions to this
one in the end.
The problem remains that in general, the minimization
over pure states with fixed Schmidt rank remains chal-
lenging, and in many cases no analytical solution can be
found. This can be remedied by relaxing the optimiza-
tion slightly.
To that end, note that there exists a characterization
of the set Skin terms of positive maps [17]: It holds that
ρSkif and only if (1dΛk)(ρ)0 for all k-positive
maps Λk:Md→ Md, where 1ddenotes the identity
map in dimension d. A map Λkis called k-positive, if
1kΛkis a positive map.
This characterization is useful, as it allows to define
slightly larger sets than Sk, which can be characterized
with less effort. To that end, we define the generalized
reduction map [16, 17]
Rp(ρA) = Tr(ρA)1dA,(7)
where ρA∈ Mdis a single qudit mixed state. It was
shown that Rpis k-positive, but not k+ 1-positive, iff
p(1
k+1 ,1
k] [17, 20]. For p= 1 one recovers the usual
reduction map. We use it to define
SR
k={ρ: (1dR1
k)(ρ)0}.(8)
Using the relation between k-positive maps and states
of Schmidt number k, it is clear that SkSR
k. Thus,
we can use these sets as an outer approximation of Sk,
as they can be characterized by semi-definite constraints.
The general embedding situation is displayed in Fig. 1.
We use this fact to find a lower bound on the optimal
value of ck= minρkSkTr(Wkρk)minρkSR
kTr(Wkρk).
摘要:

ConstructionofecientSchmidtnumberwitnessesforhigh-dimensionalquantumstatesNikolaiWyderka,1GiovanniChesi,2HermannKampermann,1ChiaraMacchiavello,2andDagmarBru11InstitutfurTheoretischePhysikIII,Heinrich-Heine-UniversitatDusseldorf,Universitatsstr.1,D-40225Dusseldorf,Germany2IstitutoNazionalediFi...

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