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Page 1: Applications of Quantum Nonlocality and Conditions on Quantum …s-space.snu.ac.kr/bitstream/10371/129541/1/000000133242.pdf · 2019-11-14 · Quantum-to-classical transition is another

저 시-비 리- 경 지 2.0 한민

는 아래 조건 르는 경 에 한하여 게

l 저 물 복제, 포, 전송, 전시, 공연 송할 수 습니다.

다 과 같 조건 라야 합니다:

l 하는, 저 물 나 포 경 , 저 물에 적 된 허락조건 명확하게 나타내어야 합니다.

l 저 터 허가를 면 러한 조건들 적 되지 않습니다.

저 에 른 리는 내 에 하여 향 지 않습니다.

것 허락규약(Legal Code) 해하 쉽게 약한 것 니다.

Disclaimer

저 시. 하는 원저 를 시하여야 합니다.

비 리. 하는 저 물 리 목적 할 수 없습니다.

경 지. 하는 저 물 개 , 형 또는 가공할 수 없습니다.

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이학박사학위논문

Applications of Quantum Nonlocality

and Conditions on

Quantum-to-Classical Transition

양자비국소성의응용과

양자-고전전이의조건

2016년 2월

서울대학교대학원

물리·천문학부

임 영 롱

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Applications of Quantum Nonlocality and

Conditions on Quantum-to-Classical Transition양자비국소성의응용과

양자-고전전이의조건

지도교수정현석

이논문을이학박사학위논문으로제출함

2015년 12월

서울대학교대학원

물리·천문학부

임 영 롱

임영롱의이학박사학위논문을인준함

2015년 12월

위 원 장 안 경 원 (인)

부위원장 정 현 석 (인)

위 원 강 병 남 (인)

위 원 신 용 일 (인)

위 원 이 진 형 (인)

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Applications of Quantum Nonlocality and

Conditions on Quantum-to-Classical Transition

Youngrong Lim

Supervised by

Associate Professor Hyunseok Jeong

A Dissertation

Submitted to the Faculty of

Seoul National University

in Partial Fulfillment of

the Requirements for the Degree of

Doctor of Philosophy

February 2016

Department of Physics and Astronomy

Graduate School

Seoul National University

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Abstract

Applications of Quantum Nonlocalityand Conditions on

Quantum-to-Classical Transition

Youngrong Lim

Department of Physics and Astronomy

The Graduate School

Seoul National University

Nonlocality is one of the most distinguished features on quantum me-

chanics. Bell test is a tool which indicates how the given system is against

the rules of local-realism, i.e., very plausible governing rules of classical me-

chanics. Although we believe the reality of quantum nonloclaity and use many

applications of that, experimentally solid Bell test has own the significant im-

portance.

We propose a experimentally feasible scheme of loophole-free Bell test

on optical system using the macroscopic entanglement. By increasing the

macroscopicity of the system we can get rid of the detection loophole effi-

ciently. Also we suggest a tool performing entanglement swapping as more

practical application of quantum nonlocality. In this method we use optical

i

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hybrid entangled state and this has advantages in the situations of lossy chan-

nel and imperfect detections.

Quantum-to-classical transition is another very historical topic and this

can be strongly relate quantum nonlocality. Previous attempts pay attention

to the given quantum state or coarsening of measurement resolution. We pro-

pose a different view of sources of this transition which is the coarsened mea-

surement references. We control the parameters of measurement references

as coarsening the time of unitary operations. To see whether the transition

occurs, we observe the violation of Bell inequality and Leggett-Garg inequal-

ity as the indicator of quantum-to-classical transition. The results give us the

consistent explanation about quantum-to-classical transition.

Keywords : Coarse-grained measurement, Bell test, Optical systems, Quantum-

to-Classical transition

Student Number : 2008-20449

ii

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Contents

Abstract . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . i

I. Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . 1

II. Quantum Nonlocality Test . . . . . . . . . . . . . . . . . . . . . 3

2.1 Bell inequality . . . . . . . . . . . . . . . . . . . . . . . . . . 3

2.2 Loopholes in Bell test . . . . . . . . . . . . . . . . . . . . . . 4

2.2.1 Locality loophole . . . . . . . . . . . . . . . . . . . . 5

2.2.2 Detection loophole . . . . . . . . . . . . . . . . . . . 5

2.2.3 Other loopholes . . . . . . . . . . . . . . . . . . . . . 7

2.3 Loophole-free Bell test using macroscopic entanglement . . . 8

2.3.1 Photon polarization entangled state and entangled co-

herent state . . . . . . . . . . . . . . . . . . . . . . . 9

2.3.2 Entangled thermal state . . . . . . . . . . . . . . . . . 17

2.3.3 Decoherence effect . . . . . . . . . . . . . . . . . . . 20

2.4 Remarks . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21

III. Applications of Quantum Nonlocality . . . . . . . . . . . . . . 23

3.1 Entanglement swapping and their applications . . . . . . . . . 23

3.2 Optical hybrid states and preparation . . . . . . . . . . . . . . 24

3.3 Entanglement swapping with optical hybrid states . . . . . . . 25

iii

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3.3.1 Single photon detection . . . . . . . . . . . . . . . . . 32

3.3.2 Homodyne detection . . . . . . . . . . . . . . . . . . 33

3.4 Detection efficiency . . . . . . . . . . . . . . . . . . . . . . . 38

3.5 Remarks . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 39

IV. Interpretations of Quantum Mechanics . . . . . . . . . . . . . 40

4.1 Copenhagen interpretation . . . . . . . . . . . . . . . . . . . 41

4.2 Statistical interpretation . . . . . . . . . . . . . . . . . . . . . 42

4.3 Many world interpretation . . . . . . . . . . . . . . . . . . . . 42

4.4 Consistent histories . . . . . . . . . . . . . . . . . . . . . . . 43

4.5 Objective collapse model . . . . . . . . . . . . . . . . . . . . 44

4.6 Remark . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 45

V. Quantum-to-Classical Transition . . . . . . . . . . . . . . . . . 46

5.1 Decoherence theory . . . . . . . . . . . . . . . . . . . . . . . 47

5.2 Macrorealism . . . . . . . . . . . . . . . . . . . . . . . . . . 48

5.3 Coarsening of measurement . . . . . . . . . . . . . . . . . . . 49

5.3.1 Coarse-grained resolution . . . . . . . . . . . . . . . . 50

5.3.2 Measurement reference and resolution . . . . . . . . . 51

5.3.3 Applying to various optical states . . . . . . . . . . . 57

5.4 Different aspect of coarsening . . . . . . . . . . . . . . . . . . 64

5.5 Remarks . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 68

VI. Conclusion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 70

iv

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Bibliography . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 72

국문초록 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 86

v

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List of Figures

Figure1. Spacetime diagram for a Bell test. Two particles start

at reference point O and arrive at A and B, Alice and

Bob respectively. The decisions of orientation of mea-

surement axis are made at point S A and S B. If the particle

toward A is first measured then measurement of B is can

be inside the light cone of A which means that we face

the locality loophole(A can be locally interacted with B). . 6

Figure2. (a) Schematic diagram for Bell inequality test using po-

larization entangled states. States |nH⟩ and |nV⟩ are dis-

criminated by Alice using a polarization beam splitter

(PBS) and two photodetectors(On/Off type) A and B. BS1

and BS2 are modeling for decoherence(photon loss) and

detector efficiency, respectively. (b) Similarly, for entan-

gled coherent state |ECS⟩, and homodyne detection. Two

component states, |α⟩ and |−α⟩, of an entangled coherent

state are distinguished by homodyne detection. . . . . . . 10

vi

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Figure3. Optimized Bell function of the entangled polarization state

against η for two cases depicted in Fig. 2 (a). (a) The case

of photon losses after the unitary operation that is equiv-

alent to inefficient detection. As photon number n in-

creases, nonlocality shown by Bell-inequality violations

gets more robust against photon losses. The detection-

inefficiency threshold decreases to 35.6% for n = 4. (b)

Photon losses before the unitary operation. In this case

the opposite effect occurs as increasing n. . . . . . . . . . 13

Figure4. The optimized Bell function for an ECS. By increasing

the macroscopicity (amplitude α in this case), detection

efficiency threshold gets lower. For α=1, the detection-

inefficiency threshold is about 50%. . . . . . . . . . . . . 15

Figure5. (a) The optimized Bell function against the dimension-

less decoherence parameter γt and d for V = 10. The

floor of the figure shows the limit for local realistic theo-

ries. (b) The optimized Bell function against γt for V =

1.001, d = 5 (solid curve), V = 10, d = 5 (dashed curve)

and V = 10, d = 10 (dotted curve). . . . . . . . . . . . . 19

vii

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Figure6. (a) The optimized Bell function for three values of n

in an entangled polarization state plotted as variable η

when 5% losses occur before the unitary operation. (b)

The analogous quantity calculated for an ECS having

α = 1, 1.5 and 2 and subjected to 15% losses. . . . . . . . 20

Figure7. (a) a general BS (BS TA,B) mixes two coherent states |α⟩A

and |β⟩B. (b) a pair of hybrid entangled states |ΨHE⟩ are

used in ES protocol. The loss of the channel is described

by BS T and the middle BS BS 1/2B,D provides the opportu-

nity to erase the path information. The measurement out-

comes in modes B and D might reveal the entanglement

between A and C. . . . . . . . . . . . . . . . . . . . . . . 27

Figure8. Schematic diagram of homodyne and threshold detec-

tion. We use another BS 1/2 and amplitude tuned coherent

state to distinguish the vacuum state with others. . . . . . 34

Figure9. (a),(b) Success probability and (c),(d) entanglement neg-

ativity of ES as function of channel reflection rate R. (a)

and (c) when α = 0.3 and (b) and (d) when α = 0.7.

Entanglement negativity of two hybrid schemes having

different measurement setups are same. . . . . . . . . . . 35

viii

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Figure10. (a),(b) Success probability and (c),(d) entanglement neg-

ativity of ES as function of channel reflection rate R. (a)

and (c) when α = 0.3 and (b) and (d) when α = 0.7.

Assume all threshold detectors have efficiency 70%. . . . 37

Figure11. The optimized Bell function B of generic state of factor

n against (a) variance V = δ2 of the measurement reso-

lution and (b) variance V = ∆2 of the measurement ref-

erence. The dot-dashed line indicates the classical limit,

2. As the coarsening degree V of the final measurement

increases in panel (a), the Bell function decreases but this

effect can be compensated by increasing the size n of

macroscopic entanglement (dotted curve: n = 2, dashed:

n = 3, solid: n = 5). However, panel (b) shows that the

Bell function rapidly decreases independent of n when

the measurement reference is coarsened. . . . . . . . . . 56

Figure12. Optimized Bell function B for polarization entangled states

with number n against variance ∆2 of Gaussian coars-

ening angle for different values of detection efficiency

(solid curve: η = 1, dashed: η = 0.95, dotted: η = 0.9)

for (a) n = 1, (b) n = 2, (c) n = 3. In the case of n = 3,

all three curves closely overlap. . . . . . . . . . . . . . . 59

ix

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Figure13. Optimized Bell function B for entangled coherent states

with respect to (a) efficiency η of homodyne detection

and (b) variance ∆2 of Gaussian coarsening of measure-

ment reference for α = 5 (dotted curve), α = 10 (dashed)

and α = 30 (solid). Panel (a) shows α dependence of

coarsening resolution, on the contrary, panel (b) shows

decreasing Bell function regardless of values α. . . . . . . 60

Figure14. (a) Optimized Leggett-Garg function K as variance ∆2 of

Gaussian coarsening of the measurement reference for

different spin j states. The larger j values cause the faster

decrease of Leggett-Garg function along the coarsening.

(b) Optimized Leggett-Garg function K as variance ∆2

of Gaussian coarsening under the nonclassical Hamilto-

nian. Even in this restricted situation, we have no viola-

tion which is independent of j, when the proper amount

of coarsening of temporal reference is existed. . . . . . . 63

Figure15. Optimized Bell function B versus (a) efficiency η of ho-

modyne detection and (b) variance ∆2 of Gaussian coars-

ening of quadrature angle λ with α = 5 (dotted curve),

α = 10 (dashed) and α = 30 (solid). In panel (a), in-

efficiency of the homodyne detection is compensated by

increasing the value of α while it is not the case with

panel (b). . . . . . . . . . . . . . . . . . . . . . . . . . 67

x

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Chapter 1

Introduction

Classical physics before the creation of quantum mechanics is local and

realistic theory. However quantum physics has very different features; super-

position and entanglement. When the quantum mechanics starts many dis-

tinguished physicists argue the nonlocal correlation and action-at-a-distance

of quantum system but it takes several decades to clarify and quantify the

nonlocality of quantum mechanics. John Bell constructed a very exceptional

inequality that classical system should obey and the violation of the inequal-

ity means that we fail to explain the system having only local realistic theory.

Thus Bell test, whether a system violate Bell inequality, tell us that given sys-

tem is classical or not. It is very useful because it make metaphysics to real

physics, experimentally verifiable.

There are two important loopholes of Bell test, however, locality loop-

hole and detection loophole. Thus loophole-free Bell test is a goal and many

attempts have been so far. In optical system locality loophole can be closed

easily because we use photons or laser but detection efficiency is very impor-

tant to also close detection loophole in lossy channel. A macroscopic entan-

glement states can be used to rule out the detection loophole in our suggestion

1

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and this can be experimentally feasible.

We are not interested in only Bell test itself but many applications of

quantum nonlocality. Entanglement swapping, one of the good examples, is

general version of quantum teleportation and useful to quantum key distribu-

tion and so on. In this thesis we focus on optical system, especially discrete

and continuous variable hybrid optical system to perform efficient entangle-

ment swapping in various situations.

Back to the quickening of quantum physics, we may ask very important

and naive questions;What’s the real differences between quantum and classi-

cal physics? Why cannot we see the ’quantumness’ in our everyday life?

Many trials exist to answer those questions, decoherence theory, collapse

model, many world theory, consistent history etc but we suggest little bit dif-

ferent view which involve the coarsening of measurement references. Also

we focus on the various optical system and Bell inequality(or Leggett-Garg

inequality) is used to test the quantum-to-classical transition.

We firstly describe Bell test experiment and our suggestion for loophole-

free Bell test in chapter 2. In chapter 3, we briefly introduce the process of

entanglement swapping and show our proposal using optical hybrid states in

lossy environment. In chapter 4, before introduce our suggestions, briefly re-

view the interpretations of quantum mechanics and measurement problem.

In chapter 5, we focus quantum-to-classical transition and give a claim that

quantum-to-classical transition indeed be occurred by coarsening of measure-

ment references. Chapter 6 summarizes all topics and give a conclusion.

2

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Chapter 2

Quantum Nonlocality Test

2.1 Bell inequality

As mentioned in previous chapter, J.S. Bell reveals very surprising re-

sults that local realism is no longer tenable in quantum mechanics [1]. In this

chapter we briefly construct CHSH type inequality [2] which is general ver-

sion of original Bell inequality and review the meaning of it. Suppose there

are two observers, Alice and Bob, A and B who are spatially separate in space.

In each observer measurement has two outcome, +1 and −1. We represent this

measurement results by A(a) and B(b) and consider the correlation of those

results. Next step is putting hidden variable λ into this results which means λ

controls A(a, λ) and B(b, λ) deterministically. Also locality plays a role in a

sense that A(a, λ) is independent of the parameter b and B(b, λ) is also inde-

pendent of the parameter a. Then we can define correlation function as

E(a, b) =∫Γ

A(a, λ)B(b, λ)ρ(λ)dλ (2.1)

3

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where Γ is total space and ρ(λ) is normalized probability distribution. After

some calculations we arrive that

|E(a, b) − E(a, c)| ≤ 2 − E(b′, b) − E(b′, c) (2.2)

and let a′ ≡ c and triangle inequality we finally get

|E(a, b) − E(a, b′) + E(a′, b′) + E(a′, b)| ≤ 2. (2.3)

The inequality holds for local hidden variable theory, very natural for classi-

cal physics. However we easily find that quantum state and observables vi-

olate this inequality. This is a tremendous improvement of understanding of

quantum mechanics since it is a quantitative description of nonlocality and

experimentally verifiable that whether the system has quantum behavior. Of

course, the converse is not true which means that every quantum system do

not need to violate this inequality. The next goal is for experimentalists that

confirm the violation of Bell inequality, namely Bell test but there are several

issues for that.

2.2 Loopholes in Bell test

In the previous section we review the importance of Bell test. There are

several loopholes in experiments, however, which make Bell test to be invalid

at all. Two main loophole; locality loophole and detection loophole and sev-

4

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eral insignificant loopholes are existed.

2.2.1 Locality loophole

When we perform Bell test, there are two spatial modes so we let them go

opposite side each other and doing measurements. If two particles go slower

than light speed, they are in same light cone referenced at starting point so

they can have interactions locally by another unknown particles. Furthermore,

even if their moving speed is same with light, it must take time to perform

measurement. In other words, we cannot immediately get the result of a mea-

surement when the particle arrive at measurement apparatus therefore there

are also chances to interact locally between Alice and Bob. These are well

depicted in Fig. 1.

If we investigate a Bell test in the optical system, the locality loophole

can be handled by using ultrafast analyzers and photonic information carri-

ers, which guarantee the spacelike distribution of particles outside the light

cone [3].

2.2.2 Detection loophole

In a Bell test, Alice and Bob set up the measurement apparatus and read

the results. For an optical system, the observables are photon number parity,

on/off threshold, homodyne detection, etc. Then we repeat same experiment

many times and collect all results to get a correlation function. This procedure

assume that the detecting apparatus is perfectly operated. However, if detec-

5

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Figure 1: Spacetime diagram for a Bell test. Two particles start at referencepoint O and arrive at A and B, Alice and Bob respectively. The decisions oforientation of measurement axis are made at point S A and S B. If the particletoward A is first measured then measurement of B is can be inside the lightcone of A which means that we face the locality loophole(A can be locallyinteracted with B).

6

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tion is imperfect; photon number detector miscount the number of photons for

example, the final correlation function is not 100% be trusted. For instance,

82.8% detection efficiency is needed for minimum violation of Bell inequality

for maximally entangled qubit states [4].

There are considerable efforts have been directed towards the closing of

the detection loophole through the use of various sorts of quantum states and

measurement schemes [5, 6]. Generally speaking, Bell test in atomic systems

instead of photonic systems easily closes detection loophole but locality loop-

hole is very problematic in this case. Since we focus in photonic systems the

locality loophole is less important but detection loophole matters generally.

2.2.3 Other loopholes

There are several loopholes that have been debating but it is worth to

review some of them. First of all, we assume that all hidden variables have

rotational invariance but the general Bell test might not be thus it leads mis-

leading of correlation function. This is called failure of rotational invariance

but it is not crucial loophole because it can be enough though we only consider

rotationally symmetric case. Second one is more serious, memory loophole.

This is about when periodic or predictable measurement setting is used, we

can predict remote settings so we get violation artificially. It was firstly stated

by Aspect [7], the author assume no memory but the real solution is using

random setting and it was done [3] although the true randomness problem

remains.

7

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The coincidence loophole, related with detection loophole, is concerned

with joint property of two detections. If we use successive signals having very

short interval, we can have an error to determine the coincide set of particles

and this affects the correlations. For example, a simple local realistic model

with conditional coincidence probability of 87.87% can give the value 2√

2

in the CHSH inequality [8]. This can be overcome by using a pair of photons

emerges from the beam splitter, for example. Some experiments performed

pulsed-pump optical system to rule out the coincidence loophole [9, 10].

Finally, it is worth state the freedom of choice loophole which tells that

whether we can choose measurement settings randomly. In other words, the

settings really are independent each other, or the past events interrelate to

them. It is also called superdeterminism, we can never close this loophole by

scientific methods [11]. Therefore it is not physically wrong that we rule out

this loophole. There are also more loopholes that we skip explanation [12].

2.3 Loophole-free Bell test using macroscopic entan-

glement

In this section we suggest a method to get around the detection loophole

in optical system using macroscopic entanglement [13]. Then give examples

of that method and also discuss implementations and decoherence effects. The

argument below is somehow counterintuitive that we propose to solve the de-

tection loophole: we investigate optical settings for violation of Bell’s inequal-

8

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ity and show that only small increase of macroscopic parameter is sufficient to

overcome the detection loophole. Here, the macroscopic entanglement means

that entanglement between macroscopically distinct states and in this sense

we use also macroscopicity intended as macroscopic parameter for that. The

word “macroscopic” here is somewhat vague concept because it does not indi-

cate specific boundary between macroscopic and microscopic states. Instead

of that, it is kind of measure for parameter which can be corresponded the

macroscopic state when the parameter is large. This macroscopic entangle-

ment is very important in literature of modern quantum mechanics because

we want to see quantum behavior in macroscopic systems for application(e.g.

quantum computation) and theoretical issue of foundation of quantum me-

chanics(e.g. quantum-to-classical boundary). However this can be possible

only under very selective conditions [14, 15] and it could be destroyed by

decoherence phenomena [16]. What we suggest here is that the considered

optical states with appropriate decoherence can close the detection loophole

in Bell test in lower experimental requirement.

2.3.1 Photon polarization entangled state and entangled co-

herent state

We firstly consider the photon polarization entangled state defined as

|ψn⟩ =1√

2(|nH⟩|nV⟩ + |nV⟩|nH⟩), (2.4)

9

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Figure 2: (a) Schematic diagram for Bell inequality test using polarizationentangled states. States |nH⟩ and |nV⟩ are discriminated by Alice using a po-larization beam splitter (PBS) and two photodetectors(On/Off type) A and B.BS1 and BS2 are modeling for decoherence(photon loss) and detector effi-ciency, respectively. (b) Similarly, for entangled coherent state |ECS⟩, andhomodyne detection. Two component states, |α⟩ and | − α⟩, of an entangledcoherent state are distinguished by homodyne detection.

where |nH⟩ (|nV⟩) is a state of n photons, all with horizontal (vertical) polariza-

tion in a single spatial mode. State (2.4) is equivalent to a GHZ-type entangled

state |H⟩⊗2n + |V⟩⊗2n [17] in a sense that local unitary operations and mode re-

arrangement can convert each other. These state experimentally generated for

values of n up to 5 with fidelity 0.56 (n = 4 with 0.78) [17, 18]. We can treat

|nH⟩ and |nV⟩ of Eq. (2.4) as macroscopically distinguishable states when n is

large.

If we have only coarsened measurement detector, like naked eyes, so that

“macroscopic difference” only can be distinguished. Such a possibility has

10

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been investigated recently as verifying entanglement and non-locality involv-

ing macroscopic components experimentally [19, 20, 21, 22, 23, 24] as well

as quantum-to-classical transition [23, 25, 26, 27, 28]. As shown in Fig. 2, the

two states can be discriminated when n is large enough. In other words, the

detector A (B) clicks, one can conclude that input state was |nH⟩ (|nV⟩). If all

the incoming photons are lost, however, because of photon losses or detec-

tor’s missing, the measurement scheme fails. Therefore we can say success

probability is

Ps = 1 − (1 − η)n, (2.5)

where η is the efficiency of each detector. This can be reached arbitrarily close

to unity by increasing n when η is not zero.

We can introduce the measurement operator such as

O =n∑

k=1

(|kH⟩⟨kH | − |kV⟩⟨kV |

)+ |0⟩⟨0|, (2.6)

where the last term is meant a “no-click” event at both photodetectors in Fig. 2

(a) which represents undetected event in real experiment so that we cannot in-

clude this for calculating correlation function. However, we assume that we

can collect all events for get the correlation function in Bell test theoreti-

cally. If we exclude some events including no-clicking, then our local realis-

tic bound of Bell inequality should be modified. Therefore we need to include

the last term in the measurement operator and fix the bound of Bell inequality.

11

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After optimizing parameters, the violation of Bell inequality with last term in

Eq. (2.6) means that the system have no local realistic description even if all

non-detecting events lower the value of Bell function. The correlation func-

tion is

Ep(θa, θb, η)=Traba′b′[Oa ⊗ Ob|Ψn(θa, θb, η)⟩⟨Ψn(θa, θb, η)|] (2.7)

where the superscript p means polarization entangled states and

|Ψn(θa, θb, η)⟩=Bpaa′(η, θa) ⊗ Bp

bb′(η, θb)|ψn⟩ab|00⟩a′b′ . (2.8)

We have introduced Bpj j′(η, θ j) = B j j′(η)U p(θ j) ( j = a, b) with the beam split-

ter operator Bab(η) = eζ2 (a†b−ab†) of transmittivity η=(cos ζ)2 and U p(θ j) =

exp[iθ j(|nH⟩ j⟨nV | + h.c.)] is a rotation about the x-axis of the Bloch sphere

where the poles are polarization qubit {|nH⟩, |nV⟩} j encoded in mode j. Clearly

this unitary operation depends on the photon number n, so it should be dealt

with non-linear Hamiltonian Hn = g(anHa†nV eiϕ + h.c.) and we choose the in-

teraction time to get the value of θ j we want. Any universal Hamiltonian can

be decomposed into series of Gaussian and cubic operation [29, 30] so that

it can be implemented in principle, but this decomposed operations are much

complicated when n is large. However, as seen later, we don’t need such high

value of n, instead n = 4 is enough for the practical purposes.

The Bell function [2] is straightforwardly constructed from the correla-

12

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0.80 0.85 0.90 0.95 1.00

1.8

2.0

2.2

2.4

2.6

2.8

0.4 0.5 0.6 0.7 0.8 0.9 1.0

1.8

2.0

2.2

2.4

2.6

2.8Bp

Bp

n=1n=2

n=3n=4

n=4

n=1n=2

n=3

(a) (b)

Figure 3: Optimized Bell function of the entangled polarization state againstη for two cases depicted in Fig. 2 (a). (a) The case of photon losses after theunitary operation that is equivalent to inefficient detection. As photon num-ber n increases, nonlocality shown by Bell-inequality violations gets morerobust against photon losses. The detection-inefficiency threshold decreasesto 35.6% for n = 4. (b) Photon losses before the unitary operation. In thiscase the opposite effect occurs as increasing n.

tion function Eq. (2.7) such as Bp(θa, θb, θ′a, θ′b, η) = Ep(θa, θb, η)+Ep(θa, θ

′b, η)+

Ep(θ′a, θb, η) − Ep(θ′a, θ′b, η), which should satisfy |Bp| ≤ 2 under the assump-

tions of local realistic theory. The explicit correlation function in our case is

Ep(θa, θb, η)=(1 − η)2n − [1 − (1 − η)n]2 cos [2 (θa + θb)] . (2.9)

The results corresponding to optimized Bell function against detection effi-

ciency η in Fig. 3 (a). In case of n = 1, the efficiency for minimum violation

(detection-inefficiency threshold) is 82.8%, which is consistent value for the

maximally entangled qubit states [4]. This threshold can be lowered if we in-

crease macroscopicity n which means increasing the macroscopic nature of

the entangled state. In other words, the detection loophole in this case can be

13

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overcome by a slight increasing of macroscopic character.

At this point, we should comment an important feature of photon losses.

If we only consider the losses after unitary operation which models the de-

tector inefficiency (BS2 in Fig. 2 (a)), the simple solution is increasing of n.

However, how about losses before unitary operation (BS1 in Fig. 2 (a))? In

order to consider this case, what we need to do is just replace B j j′(η, θ j) in

Eq. (2.8) with Bpj j′(η, θ j) = U p(θ j)B j j′(η) ( j=a, b). As clearly seen in Fig. 3

(b), the larger photon number n, the more sensitive to photon losses which is

indeed opposite behavior to the previous case. The reason of this effect is that

the losses before unitary operation destroy the coherence of initial state thus

it is treated as solely decoherence. Decoherence rate depends on the macro-

scopic parameter, here the bigger n has faster rate. Therefore we must consider

both effect to reach optimal value of n. This is also the reason we do not con-

sider higher n cases despite the n = 4 is not sufficiently macroscopic. In the

end of this chapter we revisit the issue of decoherence.

Next example is the entangled coherent state defined as(ECS) [31]

|ECS⟩ = N(|α, α⟩ + | − α,−α⟩), (2.10)

where |±α⟩ is a coherent state of amplitude ±α ∈ C and N=[2(1 + e−4|α|2)]−1/2

is a normalization factor. Using a 50:50 beam splitter and coherent-state su-

perpositions, |α⟩ + | − α⟩, this state can be generated experimentally [32, 33],

also a nonlocal generation is succeeded recently [34].

14

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0.2 0.4 0.6 0.8 1.0

1.8

2.0

2.2

2.4

2.6

2.8

Becs

α=1.0

α=1.5

α=2.0

Figure 4: The optimized Bell function for an ECS. By increasing the macro-scopicity (amplitude α in this case), detection efficiency threshold gets lower.For α=1, the detection-inefficiency threshold is about 50%.

The set-up is illustrated in Fig. 2 (b). Analogously the unitary operations

Uecsj j′ (θ j) ( j=a, b) are embodied by effective rotation in the space spanned by

the basis {|α⟩ , |−α⟩}. It is known that such transformation can be approximated

by cascade of single-mode Kerr-like nonlinearities and displace operations for

large |α| [23, 35, 36]. We are interested in relatively large value of α (|α| > 1)

so that we can use the approximation for simplicity. In this case we have

homodyne measurement instead of on/off photodetector, in order to get the

correlation function. Then the outcomes can be dichotomized by indicating

+1(−1) to positive (negative) expectation values of the quadrature operator in

phase space. In Refs. [23, 35, 36, 37, 38, 39], it is proven that this method

can be successfully used for investigation of non-classicality tests, including

multipartite nonlocality and quantum contextuality.

15

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We model inefficiency of homodyne detector in a same way that we deal

with photodetectors [cf. Fig. 2 (b)]. For simplicity and without loss of gener-

ality, we assume α ∈ R. The corresponding Bell function |Becs(θa, θb, θ′a, θ′b, η)|

can be gathered using the correlation functions Eecs(θa, θb, η) = P++ + P−− −

P+− − P−+, where we have defined the probabilities

Pkl=

∫ ks

ki

dx∫ ls

lidy⟨xaxb|Tra′b′[|Φ(θa, θb, η)⟩⟨Φ(θa, θb, η)|]|xaxb⟩ (2.11)

with |Φ(θa, θb, ηa′b′)⟩=Becsaa′(η, θa) ⊗ Becs

bb′(η, θb)|ECS⟩ab|00⟩a′b′ , Becsj j′ (η, θ j)

=B j j′(η)Uecs(θ j) ( j=a, b), the subscripts k, l=± that correspond to the assigned

measurement outcomes ±1 and the integration limits +s = ∞, +i = −s = 0

and −i = −∞. Also |xa⟩ (|xb⟩) is an eigenstate of the quadrature operator

xa = a + a† (xb = b + b†) with eigenvalue xa (xb).

We depict the Bell function against the homodyne detector efficiency η

for several values of α in Fig. 4. As expected, we get the robust violation of

Bell inequality by increasing macroscopicity (in this case the amplitude α).

For example, violation can be possible with only 50% detector when α = 1.

If we compare this to the case of polarization entangled states, ECS is much

stronger for detection inefficiency under same average photon number. For

example, the detection-inefficiency threshold is about 0.83 for the polariza-

tion entangled state but it is about 0.5 for the ECS when average photon

number is 2. Furthermore, similar to previous case, larger values α imply

more fragile to decoherence effect, the loss before unitary operation consid-

16

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ered. This can be easily seen by introducing the Markovian master equation

∂tϱ = γaϱa†− γ

2 (a†aϱ+ϱa†a) with ϱ the density matrix of a boson with associ-

ated annihilation (creation) operator a (a†), γ the loss rate and t the interaction

time. Indeed the decoherence effect described by this maser equation is equiv-

alent to the beam splitter loss with the relation given by η = exp[−γt].

2.3.2 Entangled thermal state

Now we study more general states than ECS, called entangled thermal

state (ETS) [40, 41]

ρetsab (θa, θb)=N+

∫ ∫d2αd2βPth

α (V, d)Pthβ (V, d) |ecs⟩ab⟨ecs| (2.12)

with |ecs⟩ = |α, β⟩ + |−α,−β⟩, N± = [2(1 ± e−4d2/V/V2)]−1 and Pthα (V, d) =

2π(V−1)e

−2|α−d|2(V−1) the Gaussian thermal distribution with variance V = 2(n − d2) +

1 (n is the mean photon number) and center d (with respect to the origin

of the phase space). It is clear that ECS is a special case of ETS and this

state can be created by entangling two single-mode thermal states mutually

displaced by d. It is used to prove violation of Bell inequality with coarse

grained homodyne measurements and thermal local states [23].

We replace ECS by Eq. (2.12) in order to calculate a correlation function,

then we finally get Cets(θa, θb) that enters in the Bell function Bets(θa, θb, θ′a, θ′b) =

17

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Cets(θa, θb) +Cets(θ′a, θb) +Cets(θa, θ′b) −Cets(θ′a, θ

′b),

Cets(θa, θb) =V1V2

{e4iθagη(θa)

[Qgη(θb)s(θb) + ie

2d2V V1h(θb)

(f−,η(θb) − e8iθb f+,η(θb)

)]+ V1h(θa)

[ie2θb(2i+ Vθb

d2 )gη(θb)s(θb)(

f−(θa) − e8iθb f+(θa))

+ 4V1h(θb)(e8iθa f−,η(θb) f+,η(θa) + e8iθa f−,η(θa) f+,η(θb)

)]}(2.13)

where s(θi) = sign(θi) and

h(θi) = e2(d4+θ2i )

d2V , gη(θ j)=Erfi

√2ηθ j

d√

V2 − η2V(V − 1)

,V1 = (1/8)(1 + V2e

4d2V )−1, V2 = e−4i(θa+θb)−

2(1+V2)(θ2a+θ2b)

d2V ,

Q = 8e4iθb+2V(θ2a+θ

2b)

d2 , f±,η(θ j)=Erf

√2η(d2 ± iVθ j)

d√

1 + η2(V − 1)

.(2.14)

A detailed behavior of Bets against V and d is included in Ref. [23]. Here

we point out that the detection inefficiency can be compensated by increasing

macroscopicity, the displacement amplitude d in this case. Therefore we can

confirm our previous idea in more general case. Photon losses before unitary

operation which might be imperfection of generation process of ETS for ex-

ample, however, cause true decoherence effect so that it cannot be made up

just by increasing macroscopicity.

To see this phenomenon, We can refer the formulation of the lossy evo-

lution of a bosonic system given by Phoenix [42] to calculate the correlation

function of ETS with losses at a rate γ despite that explicit analytic expression

18

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(a) (b)

0.010

2.5

5

7.5

10

2

2.4

2.8

0

0.005

Bets

Bets

Figure 5: (a) The optimized Bell function against the dimensionless deco-herence parameter γt and d for V = 10. The floor of the figure shows thelimit for local realistic theories. (b) The optimized Bell function against γt forV = 1.001, d = 5 (solid curve), V = 10, d = 5 (dashed curve) and V = 10,d = 10 (dotted curve).

is cumbersome. In Fig. 5 (a), we plot the behavior of the Bell function versus

the displacement d between the thermal components and the dimensionless

dissipation parameter γt for V = 10 (arbitrary pick). Obviously, modest val-

ues of d are enough to violate Bell inequality regardless any value of the

decoherence parameter. Furthermore, since our macroscopic states affected

by decoherence, large V requires a larger value of d to violate Bell inequality.

We make a comparison with Bell functions obtained for different values of V

and d in panel (b). It is seen that the increase of V does not boost the speed

of decrease of Bets with γt. For example, slopes of the curves in Fig. 5 (b) of

an ETS with V = 10 and d = 5 (dashed curve) and of a (nearly) pure ECS

with V = 1.001 and d = 5 (solid curve) are very close to each other. This

is because large V corresponds to a higher temperature which is not crucial

19

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0.6 0.7 0.8 0.9 1.0

2.0

2.4

2.8

p

n=1n=2

n=3

(a)

0.0 0.2 0.4 0.6 0.8 1.01.6

2.0

2.4

2.8Becs

1.5

2

1.6

(b)B

Figure 6: (a) The optimized Bell function for three values of n in an entan-gled polarization state plotted as variable η when 5% losses occur before theunitary operation. (b) The analogous quantity calculated for an ECS havingα = 1, 1.5 and 2 and subjected to 15% losses.

for nonlocality of the state. On the other hand, a larger separation in phase

space (i.e. larger d) results in quicker destruction of Bell violation because it

is closely related macroscopic nature of states. In general large macroscopic

states experience large decoherence effect.

2.3.3 Decoherence effect

We have briefly seen the relation between decoherence effect and detec-

tion inefficiency in various states, but in this section, we consider both effects

at once for the more realistic situation. In the calculation this is encoded by

B j j′(η2)U(θ j)B j j′′(η1), where η1 (η2) is the parameter determining losses be-

fore the unitary operation (the losses after unitary operation) respectively. For

the case of polarization entangled states, the results in Fig. 6 (a) show that the

state of n = 3 requires detection efficiency to be larger than 61% under 5%

20

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losses before the unitary operation. This is indeed very low efficiency which

is attainable in real experiment as long as we maintain decoherence at appro-

priate low level. Meanwhile, if we have a state whose n is larger than 3, we

need more strict condition on decoherence rate to observe the violation of Bell

inequality so that it is not the optimistic situation. However, the ECS has an

advantage in this sense, as shown in Fig. 6 (b). For instance, we can still see

Bell violation at α = 2 when detection efficiency is only ≃ 17% and decoher-

ence 15%. This is significantly lower requirement than polarization entangled

state, considering that about 250m length for traveling photons would be suf-

ficient to be free from the locality loophole [3], this values are not far from

the state of art when using telecom fibers [43].

2.4 Remarks

We examined several examples of entangled photon states to reveal that

“macroscopic quantum correlation” performs a role for overcoming the limi-

tation of detection efficiency in the test of fundamental nonlocal test of quan-

tum mechanics. In other words, we increase value of a parameter indicating

macroscopic nature of entangled state to overcome loss of detection scheme,

detector inefficiency. Some authors tried to explain the concept of “macro-

scopic entanglement” quantitatively [44], there is no clear consensus for that.

Furthermore, increasing macroscopicity sometimes causes enlargement of di-

mension of Hilbert space, such that polarization entangled state in our case.

21

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Therefore the crucial point is that we keep our states in confined dimension

while we increase macroscopicity. This procedure is much more easy and ef-

ficient for ECS rather than polarization entangled state in practical point of

view. In addition we consider loss before unitary operation which models the

purely decoherence effect, and this is cannot be overcome by increasing of

macroscopic parameter of the state. We can conclude that our result reason-

ably confirm that macroscopic entanglement is robust to inefficient detection

and this can be used for closing detection loophole in Bell test. Also this can

be done under an applicable rate of decoherence thus experimentally verifi-

able.

22

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Chapter 3

Applications of Quantum

Nonlocality

Quantum nonlocality, the very special feature of quantum mechanics, is

a source which can be widely used for many quantum technical applications.

In this chapter, we focus on entanglement swapping which is the crucial tech-

nique for secure quantum cryptography and quantum repeater.

3.1 Entanglement swapping and their applications

A possession of entanglement between remotely distant parties has been

one of the challenges for the quantum information processing such as quan-

tum key distribution [45, 46], quantum repeater [47], and quantum secret shar-

ing [48]. Entanglement swapping is one of the tool that makes possibly having

entanglement between distant parties [49].

For qubits, the simplest case, a procedure of entanglement swapping is

following. Alice and Bob, who are far apart with each other, want to share an

entanglement. Firstly, they prepare a bipartite entangled state independently

and send one of the qubits to the place between them(e.g., sending qubit in

23

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mode B for Alice and in mode D for Bob). Then, by performing of joint

measurement (e.g., Bell-state measurement), the remained qubits of Alice and

Bob (e.g., qubits in mode A and C) can be entangled remotely. This process is

applied to quantum repeater which is used for quantum communication with

lossy channel. Consequently, robust-to-loss entanglement swapping is very

important goal.

3.2 Optical hybrid states and preparation

Before discussion about entanglement swapping further, it is worthy to

point that what optical hybrid states are, and what advantages make it useful.

For the implementation of entanglement swapping in optical system, there

have been with discrete variables [50, 51, 52], or continuous variables [53,

54]. Generally speaking, discrete variables are strong to lossy environment

and we have high success probability if we use continuous variables. There-

fore there is a scheme to take advantages of both [55] but we use ‘hybrid’ as

nothing but hybrid states, not hybrid swapping scheme.

24

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3.3 Entanglement swapping with optical hybrid states

Let us first define a maximally entangled two-qubit state given by

∣∣∣ψ±HV⟩

AB=

1√

2(|H⟩A |H⟩B ± |V⟩A |V⟩B) , (3.1)∣∣∣ϕ±HV

⟩AB=

1√

2(|H⟩A |V⟩B ± |V⟩A |H⟩B) , (3.2)

and the initial state is prepared in |ψHV⟩ABCD = |ψ+⟩AB |ψ

+⟩CD, which is a prod-

uct state between two distant users. For perfect ES with a unit probability, a

Bell-state measurement (BSM) (PBell = {|ψ±⟩ ⟨ψ±| , |ϕ±⟩ ⟨ϕ±|}) is performed in

modes B and D, which are sent from Alice and Bob respectively, and finally

entanglement moves to modes A and C. We can consider other kind of max-

imally entangled state which is made of vacuum and single photon state(|0⟩

and |1⟩) such as |ψ01⟩ABCD =∣∣∣ψ+01

⟩AB

∣∣∣ψ+01

⟩CD

instead of horizontal and verti-

cal polarized photon states. We also get the perfect ES in this case but it has

very different behavior under photon losses. The reason why we focus on the

vacuum-single-photon (VSP) state is that VSP entanglement can be used for

quantum computation [56] and entanglement swapping [57] because it can be

generated easier and has a broad potential [58].

However we cannot directly do BSM, one of the linear optical methods

for polarization entangled states is putting a polarization beam splitter(PBS)

in each mode after going through 50:50 beam splitter(BS). Then we can dis-

tinguish two of four Bell states so the success probability is 50% and this is

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the upper bound for linear optics [59]. Similarly there need only a 50:50 BS

for vacuum and single photon entangled state.

Now, we propose a simple scheme of ES using hybrid entangled states.

We define optical hybrid state as

|ψHE⟩AB =1√

2(|0⟩A |α⟩B + |1⟩A |−α⟩B) (3.3)

where |α⟩ is a coherent state with amplitude α. This is a hybrid of discrete

variable(Fock basis) and continuous variable(coherent basis). It can be exper-

imentally generated when α is small case [60]. For experimental considera-

tion we set the discrete part as vacuum and single photon states but essen-

tially same for polarization states |H⟩ , |V⟩ because they don’t undergo losses

or measurements. Let us assume that a pair of the initial state in Eq. (3.3) are

created in two distant locations and a part of them are sent off into a mea-

surement setup including a typical BS with threshold detectors in the middle

location (see Fig. 7 (b)).

For optical ES, a beam-splitter (BS) is in general an important element

in ES protocols not only for joint measurement in the middle location but

also for description of lossy conditions in a channel. Fig. 7 (a) shows how a

generalized BS acts on two coherent states given by

BS TA,B |α⟩A |β⟩B =

∣∣∣∣α√T − β√

1 − T⟩

A

∣∣∣∣α√1 − T + β√

T⟩

B, (3.4)

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B

TBSA

HE AB HE CD

A B D C

DDBD

Detection

(a)

(b)

1/ 2BS

TBS TBS

Figure 7: (a) a general BS (BS TA,B) mixes two coherent states |α⟩A and |β⟩B.

(b) a pair of hybrid entangled states |ΨHE⟩ are used in ES protocol. The lossof the channel is described by BS T and the middle BS BS 1/2

B,D provides the op-portunity to erase the path information. The measurement outcomes in modesB and D might reveal the entanglement between A and C.

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where T is a transmission rate (α and β are complex numbers). Then, a typical

50:50 BS (BS 1/2) is given by

BS 1/2A,B |α⟩A |β⟩B =

∣∣∣∣∣∣α − β√2

⟩A

∣∣∣∣∣∣α + β√2

⟩B

. (3.5)

For example, two coherent states are mixed with the same amplitude α such

as

BS 1/2A,B |α⟩A |α⟩B = |0⟩A

∣∣∣∣√2α⟩

B, (3.6)

BS 1/2A,B |α⟩A |−α⟩B =

∣∣∣∣√2α⟩

A|0⟩B , (3.7)

BS 1/2A,B |−α⟩A |α⟩B =

∣∣∣∣−√2α⟩

A|0⟩B , (3.8)

BS 1/2A,B |−α⟩A |−α⟩B = |0⟩A

∣∣∣∣−√2α⟩

B. (3.9)

Having this 50:50 BS and the photon number resolving detectors we can dis-

tinguish all four Bell states of mode B and D [61]. However due to very low

efficiency of photon number resolving detector [62], we consider more realis-

tic situation in the next section.

We here consider two types of detection schemes such as vacuum-one-

photon (VOP) threshold and homodyne detections. The VOP threshold detec-

tor is an extended version of a conventional threshold detector and able to de-

tect a vacuum and an one-photon state distinguished with the other states [63].

The description of generalized photon number detection is given by the

sum of n-photon projector P jn = |n⟩ j ⟨n| and the VOP detector consists of two

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projectors in spatial mode j [64, 65, 66, 67] given by

P j0 = |0⟩ j ⟨0| , P j

1 = |1⟩ j ⟨1| , P j,0,1 = 1 −

∑n=0,1

|n⟩ j ⟨n| , (3.10)

where |0⟩ and |1⟩ are vacuum and single photon states.

In addition to the threshold detection, a setup of homodyne detection in

general consists of a BS 1/2, a strong coherent field and two photodetectors

[68, 69]. If the homodyne measurement is performed on a input signal in

mode B1, the coherent field is injected with amplitude β in mode B2 and the

BS 1/2B1,B2 mixes the input state and the field. The intensity difference between

the two detectors located in the output fields is given by IB1−B2 = b1b†2 − b†1b2

for creation operator b†i in Bi. Then, the intensity difference is given by

IB1−B2 = 2|β|⟨xθ⟩, (3.11)

for xθ = (b1eiθ + b†1e−iθ)/2 [68, 70, 71, 72]. Its projection operator is equal to

P jxθ = |xθ⟩ j⟨xθ|, (3.12)

for axis angle θ in phase space and the probability amplitude is given by

⟨xθ|αeiφ⟩ =1

π14

exp[−

12

(xθ)2 +√

2ei(φ−θ)αxθ −12

e2i(φ−θ)α2 −12α2]. (3.13)

We investigate ES for hybrid states mentioned before and compare with

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non-hybrid cases. We consider only photon losses in the channel and not de-

tectors. More experimentally plausible cases are discussed in the last section.

Firstly, we perform ES using non-hybrid entangled state discussed earlier

|ψHV⟩ABCD =∣∣∣ψ+HV

⟩AB

∣∣∣ψ+HV

⟩CD

. The mode B and D travel via lossy channel

modeled by BS T where T is the transmission rate of BS. The loss also can

be obtained from master equation and connected as T = e−γτ, γ is decoher-

ence rate and τ is interaction time. Then the reflection rate is R = 1 − T =

1− e−γτ and R = 0 means no channel decoherence, R = 1 means full decoher-

ence(complete loss). Traveling mode B and D go through BS 1/2 for example

BS 1/2B,D |H⟩B |V⟩D = |H⟩B |V⟩D − |HV⟩B |0⟩D + |0⟩B |HV⟩D − |V⟩B |H⟩D ,(3.14)

BS 1/2B,D |H⟩B |V⟩D = |0⟩B |2H⟩D − |2H⟩B |0⟩D . (3.15)

From Eq. (3.14) and Eq. (3.15), the total state after a 50:50 BS is equal

to

|ψHV⟩ABCD = BS 1/2B,D

∣∣∣ψ+HV⟩

AB

∣∣∣ψ+HV⟩

CD. (3.16)

For the lossy case,

∣∣∣ψlossHV

⟩ABEbCDEd

= BS 1/2B,DBS T

B,EbBS TD,Ed

∣∣∣ψ+HV⟩

AB|0⟩Eb

∣∣∣ψ+HV⟩

CD|0⟩Ed . (3.17)

Due to the 50:50 BS in the lossy environment, all six spatial modes become

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entangled before the measurement in the middle. Then, if one performs mea-

surements in modes B and D in the presence of losses in modes Eb and Ed,

ρiAC ∝ trBDEb Ed

[Pi

∣∣∣ψlossHV

⟩ ⟨ψloss

HV

∣∣∣ Pi]

(3.18)

where i = 1, 2 and the suitable projection operators are

P1 = |HV⟩B ⟨HV | ⊗ |0⟩D ⟨0| + |0⟩B ⟨0| ⊗ |HV⟩D ⟨HV | (3.19)

P2 = |H⟩B ⟨H| ⊗ |V⟩D ⟨V | + |V⟩B ⟨V | ⊗ |H⟩D ⟨H| . (3.20)

One BS, two PBS and 4 threshold detector can be used for realization of the

projectors. Also success probability can be calculated as pHV = trAC[ρAC]=

T 2/4 for each projector thus total T 2/2 which is consistent with that 1/2 for

non-loss case(T = 1).

To check how good the performance of ES has done, the negativity indi-

cating the degree of entanglement can be used as given by

E(ρAC) = −2∑

i

λ−i , (3.21)

where λ−i ’s are negative eigenvalues of the partial transpose of the density op-

erator. The outcome state of ES can be also represented in the fidelity between

the outcome state and one of the maximally entangled states given by

F = trAC[ρAC ρ

maxAC], (3.22)

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for ρmaxAC = {|ψ±⟩AC ⟨ψ

±| , |ϕ±⟩AC ⟨ϕ±|}. For H and V polarization entangled

states, negativity has always value 1. We will discuss more in detail later

Secondly ES for vacuum-single photon entangled states, |ψ01⟩ABCD =∣∣∣ψ+01

⟩AB

∣∣∣ψ+01

⟩CD

is performed by similar methods. The appropriate projectors

are

P1 = |0⟩B ⟨0| ⊗ |1⟩D ⟨1| (3.23)

P2 = |1⟩B ⟨1| ⊗ |0⟩D ⟨0| (3.24)

and the corresponding success probability is p01 = T (2 − T )/4 for each pro-

jector and total T (2 − T )/2. Also the entanglement negativity is

E01 =

√(1 − T2 − T

)2+( 12 − T

)2−

1 − T2 − T

. (3.25)

3.3.1 Single photon detection

Here we show how to perform ES using two VOP threshold detectors in

hybrid case. In a perfect channel (without loss: T = 1), the state after BS 1/2

in Eq. (3.3) is given by

|ψHE⟩ABCD ∝∑s=±

[|ψs⟩AC |0⟩B

∣∣∣∣S CS s√

⟩D+ |ϕs⟩AC

∣∣∣∣S CS s√

⟩B|0⟩D], (3.26)

where∣∣∣S CS ±α′

⟩= Nα′ (|α′⟩ ± |−α′⟩) for normalization factor Nα′ .

As in Eq. (3.26), if we distinguish even or odd SCS by parity measure-

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ment(i.e., number-resolving detection) then we get the unit success probabil-

ity of ES. However parity measurement is usually very hard to task, the key

idea of the protocol is that a detection of a single photon state only in a mode

(either B or D) gives an opportunity to measure an odd SCS in that mode. In

other words, if we reject all other results except single photon in one mode

and vacuum in the other mode then the successful ES is performed. These

projectors are same with Eq. (3.23) and Eq. (3.24) and the final state of lossy

case is

ρiAC ∝ trBDEb Ed

[Pi

∣∣∣ψlossHE

⟩ ⟨ψloss

HE

∣∣∣ Pi

]. (3.27)

Then we can easily calculate the negativity and total success probability as

EHE = e−4(1−T )|α|2 (3.28)

pHE = 2T |α|2e−2T |α|2 . (3.29)

3.3.2 Homodyne detection

In this subsection, we combine the schemes of threshold and homodyne

detections. For the no-loss case, we perform threshold detections in mode

B with additional BS 1/2 and a coherent state such as∣∣∣∣√2α

⟩along mode E

as Fig. 8. A homodyne detection along xπ/2 in mode D in Eq. (3.3). This

additional part is needed since we cannot distinguish vacuum state with even

SCS by homodyne detection in general. More explicitly we focus mode B and

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Figure 8: Schematic diagram of homodyne and threshold detection. We useanother BS 1/2 and amplitude tuned coherent state to distinguish the vacuumstate with others.

D after first BS 1/2 then such proportional to |0⟩B∣∣∣∣S CS ±√

⟩D+∣∣∣∣S CS ±√

⟩B|0⟩D.

This is combined another BS 1/2 with∣∣∣∣√2α

⟩in mode E and use Eq. (3.6) to

Eq. (3.9)

|0⟩D (|0⟩B |2α⟩E ± |−2α⟩B |0⟩E) +∣∣∣∣S CS ±√

⟩D|−α⟩B |α⟩E . (3.30)

If we perform threshold photo detection(no need VOP type) in mode B and E,

we can distill SCS in mode D to keep the result that both detector click ‘on’.

In this case we do homodyne detection along xπ/2 in mode D then final state

is

|ψho⟩AC =1√

2(|00⟩AC + e4iαx π

2 |11⟩AC). (3.31)

Note that fidelity between this state and Bell state is not unity because

of relative phase but still negativity is maximized. This relative phase should

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0.2 0.4 0.6 0.8 1.0R

0.1

0.2

0.3

0.4

0.5

p

0.2 0.4 0.6 0.8 1.0R

0.1

0.2

0.3

0.4

0.5

p

PHV

P01

PHE

PHEho

0.2 0.4 0.6 0.8 1.0R

0.4

0.6

0.8

1.0

E

0.2 0.4 0.6 0.8 1.0R

0.2

0.4

0.6

0.8

1.0

E

EHV

E01

EHE

EHEho

Figure 9: (a),(b) Success probability and (c),(d) entanglement negativity ofES as function of channel reflection rate R. (a) and (c) when α = 0.3 and (b)and (d) when α = 0.7. Entanglement negativity of two hybrid schemes havingdifferent measurement setups are same.

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be classically controlled for repeated ESs. The lossy case can be treated in

similar manner but we should input∣∣∣∣√2Tα

⟩considering channel loss. The

final state for lossy case is

ρAC ∝ trBDEb Ed

[P

π2DΠB

∣∣∣ψlossHE

⟩ ⟨ψloss

HE

∣∣∣ ΠBPπ2D

]. (3.32)

where Π = 1 − |0⟩ ⟨0|. The corresponding success probability and entangle-

ment negativity are

phoHE =

12

(1 − e−T |α|2)2 (3.33)

EhoHE = e−4(1−T )|α|2 . (3.34)

Note that the negativity is same with two threshold case. It will be discussed in

next section that this is no longer same if we consider detector imperfection.

These all results are summarized in Fig. 9. When α = 0.3(Fig. 9 (a),(c)) the

hybrid scheme has no advantage about success probability unless decoherence

very high but negativity is higher than vacuum and single-photon entangled

state. In case of α = 0.7(Fig. 9 (b),(d)), hybrid state with two threshold de-

tections has success probability advantage over polarization entangled state

when reflection rate is about 0.15.

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0.2 0.4 0.6 0.8 1.0R

0.1

0.2

0.3

0.4

p

0.2 0.4 0.6 0.8 1.0R

0.1

0.2

0.3

0.4

p

PHV

P01

PHE

PHEho

0.2 0.4 0.6 0.8 1.0R

0.4

0.6

0.8

1.0

E

0.2 0.4 0.6 0.8 1.0R

0.2

0.4

0.6

0.8

1.0

E

EHV

E01

EHE

EHEho

Figure 10: (a),(b) Success probability and (c),(d) entanglement negativity ofES as function of channel reflection rate R. (a) and (c) when α = 0.3 and (b)and (d) when α = 0.7. Assume all threshold detectors have efficiency 70%.

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3.4 Detection efficiency

Previously we assume perfect threshold detection but inefficiency should

be addressed in real experiments. To consider this effect, we simply put an-

other BS T ′ right before the final measurement process. Straightforwardly we

get detection efficiency T ′(i.e., T ′ = 1 means perfect detection) dependent

success probability and entanglement negativity such as,

p′01 = TT ′(2 − TT ′)/2 (3.35)

E′01 =

√(1 − TT ′

2 − TT ′)2+( 12 − TT ′

)2−

1 − TT ′

2 − TT ′(3.36)

p′HE = 2TT ′|α|2e−2TT ′ |α|2 (3.37)

E′HE = e−4(1−TT ′)|α|2 (3.38)

p′hoHE =

12

(1 − e−TT ′ |α|2)2 (3.39)

E′hoHE = e−4(1−T )|α|2 . (3.40)

Note that E′hoHE does not depend detector efficiency T ′ because we only col-

lect situation that both threshold detectors click ‘on’ in Fig. 8 which does not

degrade the fidelity of final state. Plausible efficiency of VOP threshold de-

tection is only about 70%. For On/Off detector used in homodyne detections

the efficiency is slightly higher than VOP detector thus this is an advantage of

homodyne detection in hybrid scheme. We compare previous results with this

detector efficiency(transmission rate 0.7) in Fig. 10. With imperfect thresh-

old detectors, the hybrid scheme with homodyne measurement now has more

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entanglement after ES except polarization entangled states. This is because

quantity of entanglement is not depend of measurement efficiency in our ho-

modyne measurement scheme but measurement imperfection lower success

probability of ES.

3.5 Remarks

We investigate ES using hybrid optical qubit and compare with non-

hybrid cases. We also suggest two measurement schemes for hybrid case, two

VOP threshold detectors and one homodyne with one VOP threshold detector.

We make a comparison the results altogether in success probability and entan-

glement negativity. Hybrid entangled states with the threshold detections has

advantage over vacuum and single-photon states in lossy channel. Also hybrid

entangled states with homodyne and threshold detection has good advantage

in inefficient measurement situations.

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Chapter 4

Interpretations of Quantum

Mechanics

Although quantum mechanics is a very precise well established theory,

many scientists still debate the issues of interpretation. Some reasons for that

are (1) measurement problem, (2) reality of wave function. Measurement

problem is about how a collapse occurs in wave function description which is

the standard tool of quantum physics. Reality problem is whether wave func-

tions have objective reality or not. Interesting point is that although these are

unsolved puzzles in quantum mechanics yet, we can still calculate probabil-

ities and predict experiment results in nature. Interpretations I will discuss

about from now don’t change the consequences of quantum mechanics or

predict new results. Nevertheless, the interpretation is invaluable because we

don’t have fully understood the quantum mechanics. Can we fairly describe

a single particle by a wave function? Why is large physical system behav-

ing only classically? Dynamics of entire universe is unitary? To answer these

natural questions, we need to investigate interpretations of quantum mechan-

ics in following sections. We cannot check all interpretations but relatively

important and related to quantum-to-classical transition which is the topic in

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next chapter.

4.1 Copenhagen interpretation

In the quickening period of quantum mechanics, there is no well estab-

lished interpretation. First meaningful one is suggested by Niels Bohr and

Werner Heisenberg in the years 1925 to 1927. This is called ‘Copenhagen

interpretation’ and it still remains most standard interpretation of quantum

mechanics [73]. In the Copenhagen interpretation, wave function describe all

physical state and there are no additional hidden variables. Then the state

evolves by unitary evolution until someone measure the system. The mea-

surement processes are classical so the results of the measurement should be

classical, and when measurement have done the system ‘collapse’ to one of

the eigenstates corresponding measurement apparatus. This collapse must be

non-unitary but Copenhagen interpretation do not say further. Moreover, Born

rule, the probabilistic nature of quantum mechanics, is as kind of proposition

of quantum mechanics so we accept it without question. Finally, when quan-

tum number are large, the system corresponds to a classical system. This is

the corresponding principle.

Copenhagen interpretation is very practical: it does not go deep into

probabilistic nature and measurement process. Therefore it can be a ‘basic’

interpretation at starting point. More radical and problematic interpretations

are in following sections.

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4.2 Statistical interpretation

Statistical interpretation, other name is minimal interpretation or ensem-

ble interpretation, is more practical than Copenhagen interpretation because

it has fewer assumptions as possible [74]. Wave function description is only

useful for ensemble of preparations, not single system which means that we

cannot assign wave function to the single system. In other words, wave func-

tion itself does not correspond to real physical quantity, but tools giving us

probabilities. Therefore we can keep distance from the problems; collapse of

state vector and Schrodinger cat states because wave function only applies to

an ensemble of systems, so there is no restriction for single system to have

more than one states simultaneously. There is no reduction of the wave func-

tion and wave function describe only statistical feature of an ensemble of

system.

It is counterintuitive that we cannot describe a single system. However,

what statistical interpretation suggest is that metaphysics and interpretations

can be ignored and deal with quantities that we can observe.

4.3 Many world interpretation

We have seen two interpretations in the previous sections. By Copen-

hagen interpretation, wave function collapse and unitarity is broken by mea-

surement. In the statistical interpretation, there is no collapse and superposi-

tions in single state. Here is another interpretation, called many world inter-

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pretation, which is different with other two [75]. In the many world interpreta-

tion we adopt only unitary evolution, not wave function collapse. Total state,

the whole universe for example, always evolves by unitary transformation but

in a local system with measurement process, many worlds arise in following

observables that we can measure. For example, there is a superposition state

of spin-up and spin-down initially. When an observer measure the direction

of spin, she ‘entangled’ with the system and a bifurcation arises as

|up⟩ + |down⟩ ⇒ |up⟩ |observer(up)⟩ + |down⟩ |observer(down)⟩ , (4.1)

where |observer(up)⟩ is the state of the observer with measurement outcome

‘up’, |observer(down)⟩ is with ‘down’. Since ‘up’ and ‘down’ outcomes are

classical which means we cannot measure ‘up’ and ‘down’ simultaneously,

we are only in a world after the measurement. This is the different point with

Copenhagen interpretation. Instead of collapse, the worlds branch with en-

tangled observer. Moreover whole state still has the coherence between ‘up’

and ‘down’ state, thus unitarity of total system is not broken by measurement.

Also the coherence is saved in the total state of universe, it is in principle

possible we make up the coherence.

4.4 Consistent histories

In this section we introduce slight different interpretation, ‘consistent his-

tories’ [76], or slightly different version, decoherent histories [77]. It includes

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many world interpretation and decoherence model so it is worthy to note that

we follow basic assumptions and concepts. It starts from an attempt that re-

veals history of wave function of universe. In other words, from the informa-

tions of present we retrodict to past of early universe. Therefore the important

thing is the histories of total system. keeping unitarity, there is no collapse

in here too. Instead of that, there are state, projection measurement, unitary

operation. The projections can occur at any time t in a complete set. For ex-

ample, position projection at t1 and spin-z projection at t2 etc. Then we define

a history such that the successive projections and unitary transformation to

state in a sequential order. A consistent condition is that for given initial state,

interference among the all histories are zero except same histories. The con-

sistency condition written as [78]

Tr(P(in)n , ..., P(i1)

1 ρiP( j1)1 , ..., P( jn)

n = δi1 j1 , ..., δin jn p(i1, ..., in), (4.2)

where p(i1, ..., in) is the probability of the history P(i1)1 , ..., P(in)

n . Here P(im)m means

the projection P(im) occurs at time tm. Then classical theory can be arisen with

appropriate coarsening (binding) of histories and consistent condition.

4.5 Objective collapse model

Objective collapse model is not just an interpretation but it modifies

quantum mechanics itself. In Copenhagen interpretation collapses are oc-

curred by classical measurements but it doesn’t mind how come. Objective

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collapse model deals with collapse, non-unitary evolution by introducing new

term in Schodinger equation. A measurement make a non-unitarity and also

probabilities so the additional term is a stochastic term appropriately. This

modified Schodinger equation should be matched to ordinary Schodinger equa-

tion.

This model has an advantage and a drawback. The bad thing is that what

the physical originality of the additional term is. It is not from a first principle,

the parameters are arbitrary so justification should be taken. The good news is

that it is modified version of quantum mechanics which means that it predicts

different results not followed by original quantum mechanics. It is true, the

many experiments are setting up to verify the collapse models [79].

4.6 Remark

We have reviewed several interpretations of quantum mechanics. There

are two big problems in quantum mechanics, measurement problem (collapse)

and reality of wave function. Copenhagen interpretation and objective col-

lapse model adopt the concept of wave function collapse, but others rule it

out. These interpretations are related also with quantum-to-classical transition

which is the topic in next chapter. Now we are prepared to discuss quantum-

to-classical transition.

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Chapter 5

Quantum-to-Classical Transition

Since quantum physics was born, it has been verified by tremendously

many experiments. Quantum mechanics is one of the most precise and com-

plete theory so far, it should be applied to all of scales in nature. However, we

never see the superpositions or entanglements in our everyday life. In other

words, it seems hardly the quantum behavior in some large scale or ‘classi-

cal regime’. There are many attempts in both directions to find the quantum-

classical border. One direction is from microscopic system obeying quantum

mechanical rules, investigating that the system maintains quantumness as the

size is increasing [80]. The other direction is opposite that from the system

classically well understood, it can be found the conditions on transition to

quantum behavior [81]. It is still debating that quantum-to-classical border

is really exist. In other words, there can be no such boundary at all or there

also can be objective transition by collapse [82, 83]. In any case, we call this

phenomena the quantum-to-classical transition and this should be explained

well. In this chapter we assume quantum mechanics is complete itself. Thus

we rule out the possibility of objective collapse. Also we start from decoher-

ence model, which well be accepted by many physicists and the good point to

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open our discussion.

5.1 Decoherence theory

The quantum-to-classical transition deeply related with interpretation of

quantum mechanics and measurement problem as mentioned earlier. The one

of the appealing explanations is the decoherence program [84, 85, 86]. This

theory describes that every system is surrounding by environment and the in-

teraction between the system and environment leads the system to become

mixture. The point is that this interaction with environment is ubiquitous and

uncontrollable in a system consisted of large number of particles. It is very dif-

ficult to disjoint the system-environment entanglement in general so it gives

irreversibility in nature [87, 88]. This is the reason why we cannot see the

quantum effect in classical regime but only in microscopic and isolated sys-

tems.

However, this does not mean environmental decoherence ‘really’ break

the coherence of the system. Since decoherence program deals with only uni-

tary evolutions, the coherence of the system remains in the total system which

consists of system and environment. Therefore there’s possibility that an ob-

server make a recovery of coherence by collecting the informations in the

environment. Decoherence program is not modification or interpretation of

quantum mechanics itself. However It can explain quantum-to-classical tran-

sition in a sense that classical system generally interact with large number of

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degree of freedom in its environment thus locally it loses coherence fast.

Although decoherence program is successful, it cannot explain definite

outcome problem in measurements [89]. Also the criterion to make a division

between system and environment is not clear. If we want to investigate the

quantum-to-classical transition in isolated system, the decoherence program

cannot help. This motivates the need to find another explanation of quantum-

to-classical transition.

5.2 Macrorealism

Before starting the discussion of coarsening of measurement, it helps for

us to review the concept ‘macrorealism’. Macrorealism is a word by which

Leggett and Garg firstly suggest [90]. It is defined by two postulates such

“Macrorealism per se: A macroscopic system with two or more macroscop-

ically distinct states available to it will at all times be in one or the other of

these states. Noninvasive measurability: It is possible, in principle, to deter-

mine the state of the system with arbitrarily small perturbation on its subse-

quent dynamics.”

A classical system, like situation of localrealism, is surely obeying these

postulates of macrorealism thus what we are interested in is quantum mechan-

ical system which do not obey the rules of macroscopic realistic theory. To de-

rive Leggett-Garg inequality, consider a system and a measurement Q, which

gives values ±1 similar to the case of CHSH inequality. In this case, instead

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of two remote spacelike separable parties, only one party with two temporal

measurements. In other words, it needs temporal correlation function rather

than spatial correlation in Bell inequality. Then we get the inequality that any

macrorealistic obey [90],

K = C12 +C23 +C34 −C14 ≤ 2. (5.1)

where Ci j =⟨Q(ti)Q(t j)

⟩is a temporal correlation function when ti < t j. Same

as Bell inequality, it can be violated up to 2√

2 by quantum systems. This

Leggett-Garg inequality with Bell inequality, can be used to test a system

having quantum properties and also investigate quantum-to-classical transi-

tion.

5.3 Coarsening of measurement

Decoherence theory deals with interactions between the system and its

environment but there is one more thing which is measurement outcome to get

a physical quantity. In other words, we move focusing from system to mea-

surement and find a reason of quantum-to-classical transition. The concept of

coarse-grained measurement already exists but combining with macrorealism

and leading classical physics from quantum mechanics is originally discussed

by Kofler [26]. If we start from fully quantum system, the spin- j state for ex-

ample, how can we arrive classical by manipulating parameters? One possible

answer is considering classical limit [91]: j→ ∞. However, that’s not enough

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if we can do sharp measure in the sense that every quantum eigenvalues can

be distinguished. In following sections, we investigate the conditions on tran-

sition from quantum to classical physics through coarsening of measurement

in various schemes.

5.3.1 Coarse-grained resolution

The natural trying to introduce a imperfection in measurement process is

a coarse-grained measurement which weakens measurement resolution. For

example, if the system is a spin- j coherent state [92], we make a ‘slot’ that

subdivides 2 j + 1 possible outcomes m into a number of 2 j+1∆m . This leads

quantum-to-classical transition in appropriate conditions [26]. There are coun-

terexamples, however, that we can still observe large violation of the Bell

inequality [23, 13] and also of the Leggett-Garg inequality [27]. Thus just

fuzzy resolution of measurement is not sufficient condition for quantum-to-

classical transition. Also there is another example that local realistic descrip-

tion is possible under coarsening measurements with stronger restriction [93].

Many attempts have been existed to clearly define conditions for quantum-to-

classical transition [25, 40, 94, 95, 96] and there is no quantum-to-classical

transition even in the expecting conditions [40, 95, 96]. Therefore the seeking

of consistent conditions on quantum-to-classical transition is very important

fundamentally and also for practical purposes.

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5.3.2 Measurement reference and resolution

To solve the problem arisen in previous section, it needs to look deeper

a process of measurement. It consists of two parts, one is setting reference

and the other one is projection to a measure. Past approaches are only focused

on the second part of measurement process, the resolution of measure. How-

ever, as we have seen, this is not enough for quantum-to-classical transition.

Instead, we investigate another point which involves coarsening of measure-

ment references that might be an essential condition for quantum-to-classical

transition [97]. In the test of Bell inequality or Leggett-Garg inequality, we

need to choose an measurement axis which is corresponded to unitary oper-

ation on the measurement operator in the Heisenberg picture. Therefore the

action of coarsening measurement references is realized as coarsening of uni-

tary operation, especially the rotation angle θ = wt in the Hilbert space. There

is also issue about coarsening because it can be originated from the time coars-

ening or Hamiltonian itself. The deeper discussion about this problem is out

of scope of this thesis but here we can reasonably say that the coarsening is

originally from the time coarsening because we assume that the Hamiltonian

is given and well defined. Anyway, in the following, we treat the coarsening

is about θ only, regardless where it is from.

To show the general property of coarsening of measurement reference,

let us introduce a state with an infinite dimensional orthonormal basis {|on⟩}

where n takes integer indexes from the minus to the plus infinities. Then we

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define an observable Ok = Ok+ − Ok

− where

Ok+ =

∞∑n=k+1

|on⟩⟨on|, Ok− =

k∑n=−∞

|on⟩⟨on|. (5.2)

This observable assigns eigenvalues ±1 in the case of sharp measurement.

Now we consider a fuzzy version of the observable such as

Oδ =

∞∑k=−∞

Pδ(k)Ok (5.3)

where Pδ(k) = 1δ√

2πexp[− k2

2δ2 ] is the normalized Gaussian kernel with standard

deviation δ. The distribution Pδ(k) makes the border fuzzy with the degree of

δ because the border which discriminates +1 and −1 is on the k and Pδ(k) is

a Gaussian distribution with mean k and variance δ2. We assume δ > 1 for

proper normalization. This coarsening is a kind of fuzzy resolution about bor-

der, bind the neighbor eigenvalues together in the ordinary sense. Then using

this fuzzy observable Oδ, we can discriminate two macroscopically distinct

states with error probability Pe. For the extreme case, |on⟩ and |o−n⟩ can be

identified with the error probability as

Pe = 1 −

∞∑k=−∞

1

δ√

2πe−

k2

2δ2 χn−k

2 (5.4)

where χ j is 1 for j > 0 (−1 for j ≤ 0). Next step is to establish a state we are

interested in. For the test of local realism or macrorealism, it is convenient to

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construct a maximally entangled state but in this case we confine the dynam-

ical dimension of Hilbert space as 2 in which two extreme eigenvalues line.

So the natural initial state as follows

|Mn⟩ =1√

2(|on⟩|o−n⟩ + |o−n⟩|on⟩). (5.5)

This can be behaved as macroscopic entanglement state if n is large enough.

As we said, the unitary operation are chosen to confine the dimension of

Hilbert space such as,

U(θ)|on⟩ = cos θ|on⟩ + sin θ|o−n⟩,

U(θ)|o−n⟩ = sin θ|on⟩ − cos θ|o−n⟩.

(5.6)

It is a rotation between two states |on⟩, |o−n⟩ with angle θ. The reason why

we chose this kind of special dynamics is that in fact this ”non-classical”

Hamiltonian was a counterexample of naive attack for quantum-to-classical

transition [27]. In other words, instead of ordinary Hamiltonian correspond-

ing to classical dynamics, this type of confined and extremal dynamics still

has quantumness even if the coarse-grained measurement is performed in or-

dinary sense. Therefore, it is a good strategy that we examine our suggestion

for that unitary operation. Then we easily construct the coarsened measure-

ment operator in which the coarsening unitary operation applied as

Oδ,∆(θ0) =∫

dθP∆(θ − θ0)[U†(θ)OδU(θ)

](5.7)

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where P∆(θ− θ0) is the Gaussian distribution with average θ0 and standard de-

viation ∆. Eq. (5.7) make a coarsening for unitary operation itself, particularly

interpreted as measurement references in the Heisenberg picture. Obviously,

it is not coarsening in the space of real world, but indeed in Hilbert space. We

will give more discussions about that.

To confirm the quantum-to-classical transition, our method needs to in-

vestigate CHSH type Bell inequality [1, 2] with Eq. (5.5). Here, we should

point out that originally Bell inequality can be a witness of quantumness,

but not vice versa. In other words, we have no means of validation of clas-

sicality so we cannot say that the quantum-to-classical transition occurs at

certain time. However, we still can show the tendency that confirmed by Bell

inequality, in a direction that violation is monotonic decreasing and no viola-

tion finally. Of course this is not the strict condition because non-monotonic

behavior of quantum-to-classical transition is existed [96], but it is not the

case in our argument. In our case the controlled parameter is the amount of

coarsening which obviously has monotonic behavior only with Bell function.

The next procedure is getting correlation function such as

Eδ,∆(θa, θb) = ⟨Oδ,∆(θa) ⊗ Oδ,∆(θb)⟩a,b (5.8)

where we consider both type of coarsening indicated by parameters δ and ∆.

For the fair comparison, we fix the controlled parameter in each situation, not

both at once. First case is that ∆ = 0 and δ > 1, which imply that measurement

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resolution is coarsened with perfect reference. Then the explicit expression

correlation function Eδ(θa, θb) as

Eδ(θa, θb) =12

[fδ(n, θ1) fδ(−n, θ2) + fδ(−n, θ1) fδ(n, θ2) + 2gδ(n, θ1)gδ(n, θ2)

](5.9)

where fδ(n, θ) =∑∞

k=−∞ Pδ(k)(

cos2 θχn−k+sin2 θ χ−n−k)

and gδ(n, θ) = sin θ cos θ

×∑∞

k=−∞ Pδ(k)(χn−k − χ−n−k

). This leads following Bell function,

B = Eδ(θa, θb) + Eδ(θ′a, θb) + Eδ(θa, θ′b) − Eδ(θ′a, θ

′b), (5.10)

whose absolute value is bounded above 2 by the assumption of local hidden

variable model [2]. In Fig. 11 (a), the numerically optimized Bell function for

several n with varying δ is depicted. It can be shown apparently that even large

coarsening of measurement resolution is balanced by increasing the factor n

for the violation of Bell inequality.

Second case is opposite with δ = 0 and ∆ > 0, which means that mea-

surement resolution is sharp but the reference is coarsened. The corresponding

correlation function is

E∆(θa, θb) = −∫ ∞

−∞

∫ ∞

−∞

dϕadϕbP∆(ϕa − θa)P∆(ϕb − θb) cos[2(ϕa + ϕb)].

(5.11)

We can figure out that this correlation function does not depend on the value

of n because we constrain the dimension of eigenspace as the state having ex-

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B

1.0

1.5

2.0

2.5

4 6 8 10 12 14

(b)

0.02 0.04 0.06 0.08 0.101.6

2.0

2.4

2.8

Δ2

n=2

n=3

n=5

δ2

(a)B

Figure 11: The optimized Bell function B of generic state of factor n against(a) variance V = δ2 of the measurement resolution and (b) variance V = ∆2 ofthe measurement reference. The dot-dashed line indicates the classical limit,2. As the coarsening degree V of the final measurement increases in panel (a),the Bell function decreases but this effect can be compensated by increasingthe size n of macroscopic entanglement (dotted curve: n = 2, dashed: n =3, solid: n = 5). However, panel (b) shows that the Bell function rapidlydecreases independent of n when the measurement reference is coarsened.

treme eigenvalues (n and −n), so that coarsening of unitary operation cannot

destroy the confinement. In other words, coarsening of reference always ruins

the coherence of the state and this cannot be made up by increasing n. This

can be depicted in Fig. 11 (b), only slight increasing of coarsening makes the

violation disappeared. Same argument can be applied for Leggett-Garg in-

equality, which deals with temporal correlation instead of spatial one, but for

the some technical issues we exercise this on the specific physical examples.

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5.3.3 Applying to various optical states

First example is polarization entangled state introduced in Chapter 2 as

|ψn⟩ =1√

2(|nH⟩|nV⟩ + |nV⟩|nH⟩). (5.12)

Clearly this state is identical to Eq. (5.5) if we set |nH⟩ ≡ |on⟩ , |nV⟩ ≡ |o−n⟩.

As stated in Chapter 2, the Hamiltonian governing the dynamics is nonlinear,

Hn = g(anHa†nV eiϕ + h.c.), and is in principle implementable in experiment [29,

30].

The next step is constructing a measurement operator in perfect case as

Op =

n∑k=1

(|kH⟩⟨kH | − |kV⟩⟨kV |

)+ |0⟩⟨0| (5.13)

and |0⟩⟨0| is inserted to calculate correlation function for ”no-click” event.

There is a difference here, compared to the measurement operator in generic

case (i.e. Ok) that we add here another term instead of moving border which

determines dichotomic outcomes ±1 for the fuzzy version of measurement.

The reason for this is that in the generic case we assume coarsening the bound-

ary classifying outcomes but in this physical example it is not the case. A PBS

can still well behave in an inefficient detecting case, thus inefficient detection

characterized the photon losses with perfection detection is more appropri-

ately corresponded to coarsening measurement resolution.

Therefore let us define coarsened measurement here is perfect projection

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with beam splitter, written as Opη = tra′[B

aa′OpBaa′] where a beam splitter

operator Baa′(η) = eζ(a†a′−aa′†)/2 and transmittivity η=(cos ζ)2. Here a′ is a vac-

uum mode so we should trace out after operating beam splitter. As shown in

chapter 2, this measurement inefficiency can be compensated by increasing n,

thus the result is redundant. In addition, if we move focusing on the situation

that coarsening of measurement reference occurs with perfect detection effi-

ciency, “no-click” term in the Eq. (5.13) is no longer having any meaning, so

the final correlation is equivalent to Eq. (5.11).

More interesting approach includes the both effects, as expecting new

results and more realistic scenario. Straightforwardly the coarsened measure-

ment operator is

Opη,∆

(θa) =∫

dθP∆(θ − θa)[U†(θ)Op

ηU(θ)]

(5.14)

and followed correlation function as

Eη,∆(θa, θb) = ⟨Opη,∆

(θa) ⊗ Opη,∆

(θb)⟩a,b. (5.15)

This correlation function cannot be formulated analytically, but we can

use numerical optimization method to get the Bell function with arguments

η and ∆. The results are illustrated in Fig. 12. In case of n = 1, the detec-

tion efficiency affects the maximum value of Bell function when there is no

reference coarsening. However, the slopes for different values of efficiency

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0.02 0.06 0.10 0.14

1.5

2.0

2.5

0.02 0.06 0.10 0.14

2.0

2.4

2.8

0.02 0.06 0.10 0.14

2.0

2.4

2.8

(a) (b)B

B

B

(c)

Δ2 Δ2

Δ2

Figure 12: Optimized Bell function B for polarization entangled states withnumber n against variance ∆2 of Gaussian coarsening angle for different val-ues of detection efficiency (solid curve: η = 1, dashed: η = 0.95, dotted:η = 0.9) for (a) n = 1, (b) n = 2, (c) n = 3. In the case of n = 3, all threecurves closely overlap.

are almost same because the effect by coarsened measurement reference is

dominant. Moreover, as increase of n, three curves merge to one represented

optimal one. Therefore we can say that coarsening of measurement reference

is much more important for quantum-to-classical transition when n is large,

macroscopic entanglement.

Second example is an entangled coherent state [34, 98] |ψα⟩ ∝ |α, α⟩ +

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0.02 0.04 0.06 0.08 0.10

2.8

2.4

2.0

Δ2

B

η

(a) (b)

B

2.8

2.4

2.0

0.02 0.04 0.06 0.08 0.10

α=5

α=10

α=30

Figure 13: Optimized Bell function B for entangled coherent states with re-spect to (a) efficiency η of homodyne detection and (b) variance ∆2 of Gaus-sian coarsening of measurement reference for α = 5 (dotted curve), α = 10(dashed) and α = 30 (solid). Panel (a) shows α dependence of coarsening res-olution, on the contrary, panel (b) shows decreasing Bell function regardlessof values α.

| − α,−α⟩, where |±α⟩ are coherent states of amplitudes ±α, is already men-

tioned in Chapter 2. Also what we have known is that the effective rotations

spanned the space about {|α⟩ , |−α⟩} [99], can be realization when α is not

small. Then we can construct dichotomic measurement using homodyne de-

tection with efficiency η corresponding eigenvalue +1(−1) is match to the

positive (negative) expectation value of a quadrature in the phase space. This

measurement operator can be written as Oh =∫ ∞

0|x⟩⟨x|dx −

∫ 0

−∞|x⟩⟨x|dx, and

inserting this in Eqs. (5.15) and (5.14) instead of Op gives the proper correla-

tion function. Here we should comment about coarsening measurement reso-

lution that indeed generic case study exactly matches to this situation. Since

homodyne measurement assigns a boundary between positive and negative re-

gion of phase space, coarsening resolution coincides the fuzzy boundary that

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is same concept in the generic case only except dealing with continuous vari-

able in this case. This fuzziness is related with width of homodyne detection

that is also an issue, however, we used here efficiency of homodyne detection

meaning photon losses before final measurement. This is why we use same

coarsening as the case of polarization entangled state.

In Fig. 13, our results summarized there. As expected, efficiency of final

measurement cannot block the violation of Bell inequality, in the sense that

for any small efficiency except zero, we can see the violation by increasing

macroscopic parameter α. This is in Fig. 13 (a). On the contrary, as shown

panel (b), coarsening of rotation angle θ cannot be balanced in this manner. It

evidently causes quantum-to-classical transition and is independent of value

α. More issues about homodyne width, and fixing reference in real space are

briefly discussing in the last of this chapter.

Now we introduce another approach in order to verify quantum-to-classical

transition, mentioned previous section, Leggett-Garg inequality [90]. This is

nothing but CHSH type Bell inequality, using temporal correlation instead

of spatial one. Thus a violation of Leggett-Garg inequality means that there

is no macrorealistic description for given state and dynamics, which can be a

kind of witness for quantum-to-classical transition. We follow the examples in

Refs. [26, 27] that the dichotomic parity measurement as Q =∑ j

m=− j (−1) j−m |m⟩ ⟨m|

where |m⟩ is a spin eigenstate of the spin- j operator Jz. Then we introduce a

unitary operation, U j(θ) = e−iθJx with θ = ωt, that corresponding to classical

rotation in real space and assume the initial state is the maximally mixed state

61

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j∑m=− j|m⟩⟨m|/(2 j+ 1) without loss of generality. Similar to previous procedure,

we easily get the coarsened measurement operator as Q∆(θ0) =∫

dθP∆(θ −

θ0)[U†j (θ)QU j(θ)

]. Also, the temporal correlation function between two times

ta and tb can be gained as Cab = p+a+b + p−a−b − p+a−b − p−a+b , where p+a+b

is a conditional probability for measuring + at ta and then + at tb if tb > ta.

In fact, here is some problem for getting temporal correlation functions be-

cause it consists of two measurement at different times. Indeed, the fuzziness

must be cumulated twice and calculation is complicated. What we want is

not double-counting this coarsening so that we assume that first measure-

ment in early time is sharp. Therefore the correlation function has the form

as Ci j = ⟨Q(ti)Q∆(θ0)⟩ where θ0 = ω(t j − ti) if t j > ti. Then we finally get

explicitly as

Cab =

j∑m=− j

∫ ∞

−∞

dθ′P∆(θ′ − θb−a)e2imθ′/ (2 j + 1), (5.16)

where θb−a = ω(tb − ta). It is illustrated in Fig. 14 (a) that coarsening of mea-

surement reference destroys the violation of Leggett-Garg inequality. More-

over, the rate of destruction is faster when j is larger because large j state

more sensitive by that kinds of coarsening. This is obviously opposite phe-

nomenon compared to the large value of n in the case of polarization entan-

gled state. This is because in case of polarization entangled state, we confined

dimension of dynamics, by adapting special Hamiltonian which maintains the

coherence between two extreme eigenstates. However, in this case, we con-

62

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0.2 0.4 0.6 0.8 1.0

2.0

2.2

2.4

2.6

2.8

K

0.2 0.4 0.6 0.8

0.5

1.0

1.5

2.0

2.5j=1/2

K

j=3/2

j=5/2

j=7/2j=49/2

Δ2 Δ2

(a) (b)

Figure 14: (a) Optimized Leggett-Garg function K as variance ∆2 of Gaus-sian coarsening of the measurement reference for different spin j states. Thelarger j values cause the faster decrease of Leggett-Garg function along thecoarsening. (b) Optimized Leggett-Garg function K as variance ∆2 of Gaus-sian coarsening under the nonclassical Hamiltonian. Even in this restrictedsituation, we have no violation which is independent of j, when the properamount of coarsening of temporal reference is existed.

sider the “classical Hamiltonian” in a sense that it represents a rotation in

real space not Hilbert space. So the next question naturally following is about

“nonclssical Hamiltonian” in the paper [27].

In that paper this nonclassical Hamiltonian generates macroscopic su-

perposition thus Leggett-Garg inequality is still violated even with extreme

coarsened measurement. This unitary operation can be written in the form as

U(θ) = exp[iθ(|+ j⟩ ⟨− j| + h.c.)] with θ = ωt and it should be noted that this is

equivalent one in Eq. (5.6) if |± j⟩ are alternated with |o±n⟩. The corresponding

nonclassical Hamiltonian is

H = iω(|− j⟩ ⟨+ j| − |+ j⟩ ⟨− j|). (5.17)

63

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If let us set an initial state |+ j⟩, we can straightforwardly calculate the tem-

poral correlation function as Cab = e−∆2/2 cos[ω(tb − ta)] under coarsening

of measurement reference. Definitely it is independent of value of j so that

Leggett-Garg violation fades by coarsening of the reference as plotted in

Fig. 14 (b).

5.4 Different aspect of coarsening

In the previous section, we have investigated two type of coarsening with

two type of inequality, and also two type of dynamics. Focusing on the coars-

ening part again, coarsening of measurement references solely occurs with

dynamics in the Hilbert space. This means that only for the classical dynam-

ics (Hamiltonian), it is matched to fuzzy reference in the real world. It is

somewhat counterintuitive, however, because in ordinary sense reference of

measurement should be in the real space and fuzzy reference also indicates

the vagueness in the real space. At least, we can consider an effect by such

coarsened reference in real space for any dynamics. In this section we exam-

ine that kind of coarsening with a familiar example.

The entangled coherent state is a typical nonclassical continuous vari-

ables state such

|ψ⟩ = N(|α, α⟩ + | − α,−α⟩), (5.18)

where |±α⟩ are coherent states of amplitudes ±α and N = {2(1 + e−4|α|2)}−1/2

the normalization factor. For the sake of simplicity, we assume that α is real

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and positive. Entangled coherent states are helpful for many applications to

quantum information processing [98] and also implemented experimentally

with optical fields [34]. There are many generation schemes that are dealt

with superconducting LC modes [101], Bose-Einstein condensates [102], and

motional degrees of freedom of trapped ions [103] and nano-cantilevers/nano-

mirrors [104, 105].

It needs unitary operation Uα(θ) to test Bell inequality by homodyne

measurement which can be implemented using single-mode Kerr nonlinearity

operation and displacement such as [13, 23, 35, 99]

Uα(θ) = UNLD(iθ/4α)UNL (5.19)

where D(β) = exp[βa† − β∗a], UNL = exp[−iπ(a†a)2/2] are the displacement

operator and a single-mode Kerr nonlinear interaction respectively. When

alpha is not so small, this operation is well approximated to a rotation along x-

axis in the space spanned by the {|α⟩ , |−α⟩} [23, 35, 99]. A dichotomic quadra-

ture measurement defined as

Oh =

∫ ∞

0|x⟩ ⟨x| −

∫ 0

−∞

|x⟩ ⟨x| (5.20)

where |x⟩ is an eigenstate of a quadrature operator. Then this measurement

can be realized by homydne measurement using optical fields [106].

Now we can compare several types of coarsening of measurement. Firstly

65

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we consider the case of inefficient homodyne measurement with efficiency η.

The correlation function is obtained as

Eη(θa, θb) = ⟨Ohη(θa) ⊗ Oh

η(θb)⟩a,b (5.21)

with

Ohη(θa) = tra′[U†α(θa)B†aa′O

hBaa′Uα(θa)], (5.22)

where Baa′ is the beam splitter operator with the transmission ratio η defined

in the previous section with a′ the vacuum mode. We simply get this correla-

tion function explicitly,

Eη(θa, θb) =1

1 + e−4α2 [erf(√

2ηα)]2 cos[2(θa − θb)]. (5.23)

This has α dependence, and its properties discussed in previous section (See

also Fig. 15 (a)).

As stated in former section, there are two aspects to coarsening of mea-

surement reference. First one is already studied, coarsening of reference in

Hilbert space where the state is governed by the dynamics. This can be writ-

ten by just Gaussian coarsening of parameter for unitary evolution. Under the

assumption of perfect measurement efficiency it is

Oh∆(θ0) =

∫dθP∆(θ − θ0)[U†α(θ)OhUα(θ)]. (5.24)

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0.02 0.04 0.06 0.08 0.10 0.2 0.4 0.6 0.8 1.0

2.8

2.4

2.0

2.8

2.4

2.0

Δ2

B B

η

(a) (b)

α=30

α=10

α=5

Figure 15: Optimized Bell function B versus (a) efficiency η of homodynedetection and (b) variance ∆2 of Gaussian coarsening of quadrature angle λwith α = 5 (dotted curve), α = 10 (dashed) and α = 30 (solid). In panel(a), inefficiency of the homodyne detection is compensated by increasing thevalue of α while it is not the case with panel (b).

Also the correlation function is

E∆(θa, θb) = ⟨Oh∆(θa) ⊗ Oh

∆(θb)⟩a,b. (5.25)

This can be noted explicitly,

E∆(θa, θb) =e−4∆2

1 + e−4α2 [erf(√

2α)]2 cos[2(θa − θb)]. (5.26)

The Bell function constructed from this correlation function is discussed in

the previous section too (See Fig. 13 (b)).

At this point, it is very interesting to consider the meaning of coarsened

reference in real experiment. We introduce general a quadrature variable such

67

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as

xλ =1√

2(ae−iλ + a†eiλ) (5.27)

where λ is the phase angle to the reference quadrature x. Then independent of

dynamics (Hamiltonian), we can think about a case that this quadrature ref-

erence is not sharply defined. Imagine a situation in which under assumption

of perfect efficiency and unitary operation, only this kind of coarsening is re-

mained. Then the correlation function can be determined that |x⟩ and P∆(θ−θ0)

are replaced by |xλ⟩ and P∆(λ − λ0) respectively. The correlation function is

then

E∆(θa, θb) =1

1 + e−4α2

∫ ∞

−∞

e−λ2

2∆2 α cos(λ)erf[√α2(1 + cos(2λ))]

∆√

2πα2cos2(λ)dλ

2

cos[2(θa−θb)].

(5.28)

In Fig. 15 (b), we can see that for this kind of coarsening, the violation of Bell

inequality is still disappeared by increasing the amount of coarsening. Also

this behavior is almost not affected by the value of α. That means, this kind

of coarsening also plays a crucial role to the quantum-to-classical transition.

5.5 Remarks

At the moment finishing of our work, similar result has published in

preprint [100]. They propose that outcome precision or control precision need

to increase in order to see quantum effect for a superpositions of coherent

states. This control precision is a concept which is consistent with our mea-

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surement reference. There have been many researches to verify the quantum-

to-classical transition. They have concentrated on evolution of quantum state

or measurement resolution. However we have known that there are such coun-

terexamples recently. In this chapter we briefly introduce our suggestion that

remarks new approach attacking the reference of measurement. We showed

this consistent conditions on quantum-to-classical transition in various states,

discrete and continuous variable systems. In addition, our approach is ap-

plicable to not only Bell test, but Leggett-Garg inequality which makes our

suggestion be more general.

There are also weaknesses in our approach. Bell inequality and Leggett-

Garg inequality does not tell us when quantum-to-classical transition exactly

occurs. Instead, this indicates just the tendency from quantumness to classi-

cality. In addition, the coarsening of reference has at least three meanings: in

Hilbert space, in our real space, in phase space. There is no justification for

choosing one of them. Though we have not fully considered all these cases,

but we suspect that the coarsening for quantum-to-classical transition have

to deal with dynamics of system, the Hamiltonian. Therefore for the most

general cases, a coarsening the unitary operation in Hilbert space might be

needed. It is closely related with time measuring that is physical source of

fuzziness. This is a work for future researches.

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Chapter 6

Conclusion

Nonlocality in quantum mechanics is crucial aspect which is not involved

in classical physics. Bell inequality is a indicator of this nonlocality and Bell

test experiment can verify that system has quantum nonlocality by violation

of inequality. However, in real experiment there are several loopholes for Bell

test, especially detection loophole matters when we are using optical system.

We suggest that macroscopic entangled optical state can overcome this detec-

tion loophole by increasing macroscopic parameter of the system.

Also applications of quantum nonlocality are very important in practical

situations rather than the confirmation of nonlocality itself. One of the strik-

ing examples is entanglement swapping which is the crucial technique for

quantum repeater and can be applied to quantum communications, i.e. quan-

tum key distribution. We propose the scheme of entanglement swapping using

optical hybrid state and two measurement methods, single-photon threshold

detection and homodyne measurement. We show that entanglement swapping

using optical hybrid states is more robust to photon losses than using only

discrete variables. In addition, the scheme with homodyne measurement has

great advantages for the case of inefficient detectors.

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Bell inequality, with Leggett-Garg inequality, also can be used to test

more fundamental question, quantum-to-classical transition for example. We

briefly review various interpretations of quantum mechanics to make the prob-

lem be clear. We focus on the coarsening of measurement references rather

than measurement resolution or state itself. Consequently, it can consistently

explain quantum-to-classical transition for more general cases. It gives us a

kind of answers to question about quantum-to-classical transition in such in-

tuitive, consistent way.

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국문초록

비국소성은양자역학에있어서가장특징적인성질중의하나이다.벨

실험은고전역학에서잘맞아떨어지는국소-실재주의가주어진계에서얼

마나 어긋나는지 알려주는 지표라고 할 수 있다. 벨 부등식의 위배를 측정

하는 벨 실험을 통해 우리는 양자역학의 비국소성을 증명할 수 있고 이를

응용한많은일들을왔해지만,허점없는벨실험자체의성공적인수행또

한굉장히중요한문제이다.

우리는 광학계에서의 거시적인 얽힘을 이용하여 허점없는 벨 실험을

할 수 있는 실험 가능한 제안을 하였다. 이 때 거시성을 나타내는 변수의

값을 증가시키면서 벨 실험에서의 측정 허점을 제거할 수 있다. 또한 우리

는이러한비국소성을응용할수있는실용적인방법으로얽힘교환에대한

제안을하였다.채널손실이있고측정기의정확도가낮은상황에서도얽힘

교환을 성공적으로 할 수 있도록 광학계에서의 혼성 얽힘 상태를 이용하

였다.

비국소성은 또한 양자역학의 매우 근본적인 주제와도 밀접한 관련이

있는데,양자-고전전이가그대표적인예이다.지금까지의시도는양자상

태 자체에 초점을 맞추거나 측정의 정확도에 대한 연구였는데, 우리는 측

정을하는데에필요한기준의모호함이이러한양자-고전전이를일으키는

핵심이라고주장하였다.이를위해유니터리변환의시간을모호함의매개

변수로두었다.전이의기준점을위해우리는벨부등식과레겟-가부등식의

위배를 관찰하였다. 그 결과로부터 우리는 양자-고전 전이에 대한 일관된

86

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설명중하나를제시할수있었다.

주요어 : 거친측정,양자-고전전이,광학계,양자비국소성

학번 : 2008-20449

87