nicolas gisinjointlab.upol.cz/icssur2009/talks/gisin-feynman09.pdf1 gap optique geneva university...
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Space, Time and Q nonlocality
Nicolas GisinGroup of Applied Physics
Geneva universitySwitzerland
a + b= x.y
Alice Bobx
a b
y
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My early carrier as a physicist...
Geneva 1995
... my job consist in playingwith nonlocal correlations.
Aspect 1982
How does Nature manage to produce nonlocal correlations ???
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Locality
Assumptions: 1. Alice can freely choose her input x and can read her outcome a, and similarly for Bob;
2. x & y are independent of λλλλ: I(x: λλλλ) = I(y:λλλλ) = 0;3. locality: p(a,b|x,y,λλλλ) = p(a|x,λλλλ) · p(b|y,λλλλ).
Conclusion: Bell inequalities
λλλλ λλλλ
See e.g.arXiv:0901.4255
By far the most natural assumption !… refuted beyond (almost) any reasonable doubts.
Hence, quantum correlations happen, but the probabilities of their occurrence are not determined by local variables.
λλλλ=physical state of the system accordingto QM or to anyfuture theories.
NonlocalityNonlocalityNonlocalityNonlocality
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Satigny – Geneva – Jussy
18.0 km Jussy
Geneva
Satigny
δ
NNNN
SSSS
EEEEWWWW
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� When is a quantum measurement finished ?
� Possibly only once a macroscopic mass has significantly moved, as advocated e.g. by Diosi and Penrose.
� In usual Bell tests, detection events only trigger the motion of electrons of insufficient mass to finish the measurement process.
space
time
ar
inputbr
output αααα ββββ
Adrian Kent noticed that according to this plausible assumption, no Bell test so far ensured space-like separation !
J. Franson, PRD 31, 2529, 1985 A. Kent, arXiv:gr-qc/0507045
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He-Ne Laser
Piezo
+
-BS
Single-photondetector
4VPhotodiode
100 nmMirror
Mirror
- 1 0 1 2 3 4 5 6 7 8- 1 . 0
- 0 . 5
0 . 0
0 . 5
1 . 0
1 . 5
2 . 0
2 . 5
3 . 0
3 . 5
4 . 0
4 . 5
- 3
0
3
6
9
1 2
1 5
1 8
2 1
2 4
2 7
3 0
Am
plitu
de (
V)
T i m e ( µ s )
Dis
tanc
e (n
m)
PR
L 100, 220404, 2008
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– Diósi’s equation
– For a parallelepiped mirror
– Numerical application in our case
Penrose-Diosi formula for collapse timeof the superposition: ψ1+ψ2
2223
dmG
Vd π
τ h=
sd µτ 1=310
6
10915.023
6.12
102
mmmmmmmV
nmd
kgm
−
−
⋅=××=
=⋅=
( )( )∫∫ −
−−=−
'
)'()'()()('
2
2
2
2
1
2
2
2
1332
1
rr
rrrrrdrd
Gmd
ψψψψτ
h
S. Adler, J.Phys. A40, 755 (2007)
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Bell test with true space-like separation
source
A B
time
space
The photon entersThe interferometer
A macroscopic mass hassignificantly moved
In usual Bell tests, detection events only trigger the motion of electrons of insufficient mass to finish the measurement process.
≈≈≈≈ 7 µµµµs
≈≈≈≈ 60 µµµµs≅≅≅≅ 18 km
quant-ph/0803.2425PRL100, 220404, 2008
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0 10 20 30 40 50 600
10
20
30
40
50
60
70
80
90
0
50000
100000
150000
200000
250000
300000
Coi
ncid
ence
s/60
s
Time (min)
Coincidences Sinusoidal fit: V=(90.5 ± 1.5)%
Sin
gles
(co
unts
/60s
)
Singles
Visibility > 90% ⇒⇒⇒⇒ nonlocal correlations between truly space-like separated events.
quant-ph/0803.2425PRL100, 220404, 2008
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How come the correlation ?
� How can these two locations out there in space-time know about each other ?
� via entanglement? (in Hilbert space) or
� via communication ? (in space-time)
� Let’s take the latter seriously. It requires to define faster than light “spooky action at a distance” in some preferred reference frame.
� If in this preferred frame the communication doesn’t arrive on time, then the correlation become local ! This can be tested.
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Let’s test these hypothetical preferred
reference frames
Alice and Bob, east-west orientation,perfect synchronization
with respect to earth⇒ perfect synchronization
w.r.t any frame movingperpendicular to theA-B axis
⇒ in 12 hours all hypothe-tical privileged framesare scanned.
A B
Ph. Eberhard, private communication
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0 30 60 90 120 150 180 210 2400
10
20
30
40
50
60
70
80
Coi
ncid
ence
s/60
s
Time (min)
Nature 454, 861, 2008
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0 3 0 6 0 9 0 1 2 0 1 5 0 1 8 05 0 0 0
7 5 0 0
1 0 0 0 0
2 5 0 0 0
5 0 0 0 0
7 5 0 0 0
1 0 0 0 0 0
2 5 0 0 0 0
Bo
und
on V
QI/c
χ (°)
Conclusion: the observed correlation is indeed truly nonlocal.
Indeed, to maintain a description based on spooky action at a distance, one would have to assume speeds even larger than thebound obtained in our experiment
PRL 88,120404,2002; J.Phys.A 34,7103,2001; Phys.Lett.A 276,1,2000
Bound assuming the Earth’s speed is ≤≤≤≤ 300 km/sNature 454, 861, 2008
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From all the performed experiments one has to conclude that quantum correlations can’t be explained as time-ordered events.
⇒ There is no spooky action at a distance: there is not a first event that influences a second event.
⇒ Quantum correlation just happen, somehow from outside space-time :there is no story in space-time that tells us how it happens !
… or … the influences propagate at surprisingly large speeds
PRL 88,120404,2002; J.Phys.A 34,7103,2001; Phys.Lett.A 276,1,2000
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Let’s play more with nonlocal correlations
� Simulate quantum correlations with simple nonlocal correlations.
� Independent locality.
� Leggett inequality.
� Multi-partite nonlocality.
� nonlocal correlations as a resource(e.g. cryptographic keys), see V. Scarani and A. Acin this afternoon.
� etc
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a + b= x.y
Alice Bobx ∈{0,1}
a ∈{0,1} b ∈{0,1}
y∈{0,1}
a + b= x.y
Simulation with a PR-box
Prob(a=1|x,y) = ½, independent of y ⇒ no signaling
The PR-box is a strictly weaker resource than communication.
Found.Phys. 24, 379, 1994
See Nicolas Brunner this afternoon.
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Simulating a singlet with a PR-box
),|,(),|,(21212/ baPddbaPQM
rrrrrrrr ββββααααλλλλλλλλββββαααα λλλλλλλλππππθθθθ ∫∫∫∫========
)( ++= λβrr
bsgb
a + b= x.y
)()( 21 λλrrrr
asgasg + )()( −+ + λλrrrr
bsgbsg
)( 1λαrr
asga +=
2100
01)( λλλ
rrr±=
<≥
= ±andxif
xifxsg
PRL 94,220403,2005.For partial entanglemtsee PRA 78,052111,2008
where the are uniformly distributed on the sphereand is defined by the PR-box as follows:
jλλλλr
21λλλλλλλλP
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Independent Locality (bi-locality)
Alice Bob Charly
EPR 1 EPR 2
x y z
a b c
⇒⇒⇒⇒ P(a,b,c|x,y,z)
λλλλ1 λλλλ1 λλλλ2 λλλλ2
Independent locality (bi-locality) : I(λλλλ1:λλλλ2) = 0, or P(λλλλ1,λλλλ2)=P(λλλλ1)·P(λλλλ2)
⇒⇒⇒⇒ ??? Bell-like inequalities ???
Pbiloc.(a,b,c|x,y,z,λλλλ1,λλλλ2) = p(a|x, λλλλ1) · p(b|y, λλλλ1, λλλλ2) · p(c|z, λλλλ2)
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Independent Locality (bi-locality)
Alice Bob
EPR 1 EPR 2
x y
a b
λλλλ1 λλλλ1 λλλλ2
z
c
Charly
λλλλ2
The assumption of independent locality when the sources EPR1 and EPR2are independent is as natural as Bell’s locality assumption.
It is implicitly assumed in all Bell test with Quantum Random Number Generators (QRNG).
Random choice ofmeasurement setting
QRNG
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Entanglement Swapping between 2 totally autonomous cw sources
t±ττττ t t ±ττττ t ±ττττ
ττττ ττττ
Nature Physics3, 692, 2007
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2 totally autonomous cw sources
10 pm λλλλ-filters
∆λ∆λ∆λ∆λ = 70 nm
λλλλ = 1559 ±0.01 nm
Intensity:2-10% photon-pairper coherence time
Nature Physics3, 692, 2007
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Set of bi-local correlations
Polytope of local correlations
Pbiloc.(a,b,c|x,y,z) = ∫∫∫∫dλλλλ1ρρρρ(λλλλ1)∫∫∫∫dλλλλ ρρρρ(λλλλ2) p(a|x, λλλλ1) · p(b|y, λλλλ1, λλλλ2) · p(c|z, λλλλ2)
The vertices of thelocal polytope arealso bi-local
(λλλλ1,λλλλ2) (λλλλ’ 1,λλλλ’ 2)
Local, but NOT bi-local
The set of bi-local correlations is NOT convex,Its exact shape is unknown.
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Leggett’s “locality”
Leggett assumes that locally everything is “normal”, i.e. that individual particles are always in pure states:
),|,(),|,( baPdbaPQMrrrr βαλβα λθ ∫=
“Only” the correlations C µνµνµνµν are nonlocal. They just happen, without any classical explanation. They are only constraint by Pµνµνµνµν ≥≥≥≥ 0
Found.Phys. 10,1469,2003
( )),()()(14
1),|,( baCbMaMbaP BA
rrrrrr
λλλλ αββαβα ⋅+⋅+⋅+=⇒
non-signaling
( )),(14
1baCbaPrrrrrr
µννµµν αβσηβσηα
νµλ
⋅+⋅+⋅+=
⊗=
0 <η ≤ 1
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Leggett’s inequalities
(((( ))))BABA
BA
MMCMM
baCbMaMbaP
λλλλλλλλλλλλλλλλλλλλ
λλλλλλλλλλλλλλλλ αβαβαβαβββββααααββββαααα
−−−−−−−−≤≤≤≤≤≤≤≤++++++++−−−−⇔⇔⇔⇔
≥≥≥≥⋅⋅⋅⋅++++⋅⋅⋅⋅++++⋅⋅⋅⋅++++====
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0),()()(141
),|,(rrrrrr
42
2cos2
2ϕϕϕϕϕϕϕϕ −−−−≈≈≈≈====QM
In strong contrast toBell’s inequalities, herethe bound depends on themeasurement settings
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2sin
3
22)',(),(
3
1 ϕηϕη −≈−≤+⇒ ∑=xyzj
jjjj baCbaCrrrr
Modern formof Leggett’sinequality
⇒⇒⇒⇒ …
Branciard et al. Quant-ph/0801.2241Nature Physics 4, 681-685, 2008
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Experimental refutation of Leggett’s model
� integration time:4 x 15 sec / setting
� maximal violation:L=1.925 ± 0.0017(40.6 σ) at φ = -25°
L=1.922 ± 0.0017(38.1 σ) at φ = +25°
φ
L3
QM
Leggett
for 60 sec/setting:
L3(-30°)=5.7204±0.0028 (83.7 σ)
1.4
1.5
1.6
1.7
1.8
1.9
2
0-90° -60° -30° 30° 60° 90°
PRL 99,210406,2007PRL 99,210407,2007Branciard et al. Quant-ph/0801.2241Nature Physics 4, 681-685, 2008
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Multi-partite nonlocality bw n players
A1
x1
a1
A2
x2
a2
A3
x3
a3
An
xn
an
……
Objective: define and quantify the amount of multi-partite nonlocality
p(ai|xi)
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Multi-partite nonlocality bw n players
Example #1: grouping
How few groups m suffice in order for the n playersto reproduce the correlation p(ai|xi) with only shared randomness and communication inside each group (but no communicationin-between the different groups) ?
Example #2: broadcastingx1
a1How many players n-m have tobroadcast their inputs and outputsin order that the players can reproduce the correlation p(ai|xi) with only shared randomness ?
x2 x3 x4
a2 a3 a4
2/)(2 mnmnS −≤Theorem: arXiv:0903.2715
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Conclusions� Q nonlocality is a mature topic. Lots of progress have been achieved, but many important and fascinating questions are still open.
� Quantum correlations are very peculiar. They combine nonlocal correlations with non-trivial marginals in a way that is difficult to reproduce.
� Bell-type inequalities can be derived for all kinds of hypothesis, not only Bell locality, and all sorts of nonlocal resources.
� There are connections to experiments:- moving masses to ensure space-like separation- east-west Bell tests with good synchronization- asymmetric atom-photon entanglement
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Applications1...11)sin(0...00)cos( θθθ +=GHZ
0...100...010...
010...001...0
+++
+=W
k=2 parties that broadcastor m=n-2 groups suffice
n=65-pa
rtite
non
loca
l
4-pa
rtite
non
loca
l3-
part
ite n
onlo
cal
2-pa
rtite
non
loca
l
Fully n-partitenonlocal