CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution...

92
CONTINUOUS VARIABLE QUANTUM INFORMATION Gerardo Adesso School of Mathematical Sciences The University of Nottingham [email protected] http://quantumcorrelations.weebly.com

Transcript of CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution...

Page 1: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

CONTINUOUS VARIABLE

QUANTUM INFORMATION

Gerardo Adesso

School of Mathematical Sciences

The University of Nottingham

[email protected]

http://quantumcorrelations.weebly.com

Page 2: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Plan

LECTURE I. • Introduction and examples

• Phase space formalism

• Gaussian states

LECTURE II. • Gaussian states: measures of information

• Gaussian states: measures of correlations

• Applications to quantum communication

LECTURE III. • Overview of continuous variable protocols

• Non-Gaussian resources

• Open problems and perspectives

Page 3: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

CONTINUOUS VARIABLE

QUANTUM INFORMATION

LECTURE I.

Page 4: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Qubits

*are not continuous variables systems!

Spin, polarisation, etc. are discrete

variables: upon measuring in a

given basis, you can obtain a finite,

discrete set of possible results, e.g.

0 / 1 for dichotomic variables

Page 5: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Continuous variables

are degrees of freedom associated to observables with a continuous spectrum,

for instance position 𝑞 and momentum 𝑝 of a free particle.

Continuous variable (CV) systems

are systems in which the relevant degrees of freedom are continuous variables.

With respect to those degrees of freedom, the quantum states of continuous

variable systems live in an infinite-dimensional Hilbert space

0 q

Page 6: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Motivation: CV entanglement

Einstein-Podolski-Rosen state: contains infinite entanglement

This state is unphysical as it is unnormalisable, but if you can approximate it

then you realise a very powerful resource for quantum protocols...

0 q

Page 7: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Quantum harmonic oscillator

• Canonical commutation relations 𝑞 , 𝑝 = 𝑖ℏ

• Ladder operators

• Annihilation 𝑎 =𝑚𝜔

2ℏ𝑞 +

𝑖

𝑚𝜔 𝑝

• Creation 𝑎 † =𝑚𝜔

2ℏ𝑞 −

𝑖

𝑚𝜔 𝑝

• Bosonic commutation relations 𝑎 , 𝑎 † = 1

• Number operator: 𝑛 = 𝑎 †𝑎

• Hilbert space = Fock space

• Basis: Fock states 𝑛 ∶ 𝑛 𝑛 = 𝑛 𝑛

Page 8: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Physical realisations

We need pairs of operators which satisfy the canonical commutation relations

… e.g. amplitude//phase quadratures of light

(q=“electric field”, p=“magnetic field”)

… or collective magnetic moment of atomic

ensembles (q=Sx/<Sz>, p=Sy/<Sz>)

Page 9: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Quantized electromagnetic field

• Each oscillator: a mode of the field

• Natural units: ℏ = 𝑐 = 1

• 𝑎 𝑘 =1

2𝑞 𝑘 + 𝑖 𝑝 𝑘 , 𝑎 𝑘

† =1

2𝑞 𝑘 − 𝑖 𝑝 𝑘

• 𝑞 𝑘 =1

2𝑎 𝑘 + 𝑎 𝑘

† , 𝑝 𝑘 =1

𝑖 2𝑎 𝑘 − 𝑎 𝑘

Page 10: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Quantized electromagnetic field

• We introduce a vector of canonical operators: 𝑅 = 𝑞 1, 𝑝 1, 𝑞 2, 𝑝 2, … , 𝑞 𝑁, 𝑝 𝑁

• Canonical commutation relations: • 𝑞 𝑗 , 𝑝 𝑘 = 𝑖 ℏ 𝛿𝑗𝑘

• 𝑞 𝑗 , 𝑞 𝑘 = 0, 𝑝 𝑗 , 𝑝 𝑘 = 0

• Introducing the N-mode symplectic matrix Ω𝑁 = Ω⊕𝑁, with Ω =0 1−1 0

,

then we can write the commutation relations compactly: 𝑅 𝑗 , 𝑅 𝑘 = 𝑖 Ω𝑁 𝑗𝑘

Page 11: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Phase space description

Classical

q

p

Quantum

q

p

vacuum

q

p

coherent

q

p

squeezed

here I attempted a measure of position: I localized

the particle but lost information on its momentum!

Page 12: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

• Introduce vectors 𝝃, 𝜿 ∈ ℝ2𝑁 of phase-space coordinates

• Weyl displacement operator

• Characteristic function

• Wigner function

• For one mode:

• Other choices (Glauber-Sudarshan P representation, Husimi Q function…)

Quasiprobability distributions

Page 13: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

The Wigner function is in 1-to-1 correspondence with the density matrix 𝜌

• General properties of the Wigner function (for N modes):

• W is real ( ⇔ 𝜌 is Hermitian)

• W can be negative (it is a quasi-probability distribution)

• W is normalised: 𝑑𝝃ℝ2𝑁 𝑊𝜌 𝝃 = 1 ( ⇔ tr 𝜌 = 1 )

• State purity: 𝜇 = tr 𝜌2 = 2𝜋 𝑁 𝑑𝝃ℝ2𝑁 𝑊𝜌 𝝃

2

Phase-space description

Page 14: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

The Wigner function is in 1-to-1 correspondence with the density matrix 𝜌

• General properties of the Wigner function (for N modes):

• The marginals reproduce the correct probability distributions.

• E.g. for one mode:

• 𝑑𝑞+∞

−∞ 𝑊𝜌 𝑞, 𝑝 = 𝑝 𝜌 𝑝

• 𝑑𝑝+∞

−∞ 𝑊𝜌 𝑞, 𝑝 = 𝑞 𝜌|𝑞⟩

Phase-space description

Page 15: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Wigner functions: examples

• Fock states 𝑛

a) 𝑛 = 0

b) 𝑛 = 1

c) 𝑛 = 5

q p

q p

q p

Page 16: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Gaussian states

q p

are states whose Wigner distribution

is a Gaussian function in phase space

• Recall: Gaussian probability function for one real variable:

• For 2N real variables, forming the phase-space vector 𝝃, we need:

• A vector of means 𝑅 (first moments): 𝑅 = 𝑅 𝜌 = 𝑞 1 , 𝑝 1 , … , 𝑞 𝑁 , 𝑝 𝑁

• A covariance matrix (second moments) 𝝈 of elements 𝜎𝑗𝑘

𝜎𝑗𝑘 = 𝑅 𝑗𝑅 𝑘 + 𝑅 𝑘𝑅 𝑗 𝜌 − 2 𝑅 𝑗 𝜌 𝑅 𝑘 𝜌

• Mean: 𝑥0

• Variance: 𝑉

generalisation

of 2V …

Page 17: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

q p

Gaussian states

are states whose Wigner distribution

is a Gaussian function in phase space

• Completely specified by:

• A vector of means 𝑅 (first moments): 𝑅 = 𝑅 𝜌 = 𝑞 1 , 𝑝 1 , … , 𝑞 𝑁 , 𝑝 𝑁

• A covariance matrix (second moments) 𝝈 of elements 𝜎𝑗𝑘

𝜎𝑗𝑘 = 𝑅 𝑗𝑅 𝑘 + 𝑅 𝑘𝑅 𝑗 𝜌 − 2 𝑅 𝑗 𝜌 𝑅 𝑘 𝜌

𝑊𝜌 𝜉 =exp − 𝜉 − 𝑅 𝑇𝝈−1(𝜉 − 𝑅 )

𝜋𝑁 det 𝝈

Page 18: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Very natural: ground and thermal states of all physical systems in the

harmonic approximation regime

Relevant theoretical testbeds for the study of structural properties of

entanglement and correlations, thanks to the symplectic formalism

Preferred resources for experimental unconditional implementations of

continuous variable protocols

Crucial role and remarkable control in quantum optics

coherent states

squeezed states

thermal states

Gaussian states

Page 19: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Gaussian operations

Gaussian states can be

efficiently:

displaced (classical currents)

squeezed (nonlinear crystals)

rotated (phase plates, beam splitters)

measured (homodyne detection)

Page 20: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Gaussian operations

Gaussian states can be

efficiently:

displaced (classical currents)

squeezed (nonlinear crystals)

rotated (phase plates, beam splitters)

measured (homodyne detection)

Page 21: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Gaussian operations

Gaussian states can be

efficiently:

displaced (classical currents)

squeezed (nonlinear crystals)

rotated (phase plates, beam splitters)

measured (homodyne detection)

Page 22: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Gaussian operations

Gaussian states can be

efficiently:

displaced (classical currents)

squeezed (nonlinear crystals)

rotated (phase plates, beam splitters)

measured (homodyne detection)

Page 23: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Gaussian operations

Gaussian states can be

efficiently:

displaced (classical currents)

squeezed (nonlinear crystals)

rotated (phase plates, beam splitters)

measured (homodyne detection)

Page 24: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

One-mode Gaussian states

• First moments: 𝑅 =𝑞

𝑝 =

𝑞 𝑝

• Covariance matrix: 𝝈 =𝜎𝑞𝑞 𝜎𝑞𝑝𝜎𝑞𝑝 𝜎𝑝𝑝

, 𝜎𝑞𝑞 = 2 𝑞 2 − 𝑞 2 = 2 Δ𝑞 2

𝜎𝑝𝑝 = 2 𝑝 2 − 𝑝 2 = 2 Δ𝑝 2

𝜎𝑞𝑝 = 𝑞 𝑝 + 𝑝 𝑞 − 2𝑞 𝑝

• Coherent state 𝛼 : 𝑅 =2 Re(𝛼)

2 Im(𝛼), 𝝈 =

1 00 1

• Squeezed state 𝑟 : 𝑅 =00

, 𝝈 = 𝑒−2𝑟 00 𝑒2𝑟

q

p

q

p

Page 25: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Multimode Gaussian states

• The first moments can be adjusted by local

displacements, i.e., local unitary operations

• All relevant quantitites for quantum information (e.g. state

purity, correlations, entanglement, etc.) are invariant

under local unitaries

• We can imagine all modes are locally centered in the

phase space, i.e., we can set all first moments to zero:

𝑅 = 0 without loss of generality

• Then, it is the shape of those Gaussians which matters:

• All the relevant information is in the covariance matrix

Page 26: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Multimode Gaussian states

• Covariance matrix has a block-form

• 𝝈𝒌: 2x2 reduced covariance matrix of mode 𝑘

• 𝜺𝒋,𝒌: 2x2 matrix of correlations between modes 𝑗 and 𝑘

• Partial trace over mode 𝑗: just eliminate 𝑗th row and column!

1 12 1

12 2 2

1 2

N

TN

T TN N N

𝝈 =

Page 27: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Gaussian states

• Covariance matrix has to satisfy a bona fide condition,

𝝈 + 𝑖 Ω𝑁 ≥ 0 (⇔ 𝜌 ≥ 0) in order to describe a physical state 𝜌

• Unitary operations 𝑈 = exp (𝑖 𝜃 𝐻 ) where the Hamiltonians

𝐻 are at most quadratic in the canonical operators, i.e.,

𝐻 = 𝑓 𝑎 𝑘†, 𝑎 𝑘

†𝑎 𝑙,𝑎 𝑘†𝑎 𝑙

† + herm. conj. , are associated to:

• Symplectic transformations 𝑆 which act by congruence on

covariance matrices, 𝜎 ↦ 𝑆 𝜎 𝑆𝑇, where 𝑆 ∈ 𝑆𝑝2𝑁,ℝ by

definition satisfy 𝑆𝑇Ω𝑁𝑆 = Ω𝑁 (it follows that det 𝑆 = 1)

Gaussian operations: preserve Gaussianity

Page 28: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Gaussian operations

• Example: single-mode squeezing

• 𝑈 𝑟 = exp −𝑟

2𝑎 𝑘†2 − 𝑎 𝑘

2 ↔ 𝑆 𝑟 =𝑒−𝑟 00 𝑒𝑟

• 𝑟 = 𝑈 𝑟 0 ↔ 𝝈𝑟 = 𝑆 𝑟 𝝈0𝑆𝑇 𝑟 =

𝑒−𝑟 00 𝑒𝑟

1 00 1

𝑒−𝑟 00 𝑒𝑟

= 𝑒−2𝑟 00 𝑒2𝑟

• Example: two-mode beam splitter

• Unitary:

• Symplectic:

𝜏 = cos 𝜃

Page 29: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Symplectic diagonalisation

• Williamson’s theorem

There exists a global symplectic

transformation which brings the

covariance matrix into diagonal

form, 𝑆 𝝈 𝑆𝑇 = 𝝂

Hilbert space H Phase space G

Unitary operations U Symplectic operations S

Density matrix r Covariance matrix s

normal mode decomposition

1 12 1

12 2 2

1 2

N

TN

T TN N N

the 𝜈𝑖 ’s are the symplectic

eigenvalues

1 1

2

2

N

N

n n

n n n

n

O

𝑆

0

0

Page 30: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Symplectic diagonalisation

• In Hilbert space: the state with covariance matrix 𝝂 is a

tensor product of N thermal states, each at temperature 𝑇𝑘

1 12 1

12 2 2

1 2

N

TN

T TN N N

the 𝜈𝑖 ’s are the symplectic

eigenvalues

1 1

2

2

N

N

n n

n n n

n

O

𝑆

0

0

Page 31: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Using the symplectic spectrum

• Bona fide condition: 𝝈 + 𝑖 Ω𝑁 ≥ 0 ⇔ 𝜈𝑘 ≥ 1 ∀ 𝑘 = 1,…𝑁

• Purity of Gaussian states:

𝜇𝜌 = tr 𝜌2 = 2𝜋 𝑁 𝑑𝝃ℝ2𝑁 𝑊𝜌 𝝃

2≡

1

det 𝝈=

1

Π𝑘𝜈𝑘

• Pure Gaussian states: det 𝝈 = 1

• Mixed Gaussian states: det 𝝈 > 1

Exercise: prove this!

Exercise: prove this!

Page 32: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Summary of Gaussian states

G. Adesso & F. Illuminati, J. Phys. A: Math. Gen. 40, 7821 (2007)

Page 33: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

CONTINUOUS VARIABLE

QUANTUM INFORMATION

LECTURE II.

Page 34: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Recall: symplectic eigenvalues

• The symplectic eigenvalues can be calculated from the

standard (orthogonal) spectrum of the matrix 𝑖 Ω𝑁𝝈, which

has eigenvalues ±𝜈𝑘

1 12 1

12 2 2

1 2

N

TN

T TN N N

the 𝜈𝑖 ’s are the symplectic

eigenvalues

1 1

2

2

N

N

n n

n n n

n

O 0

0 𝑆𝑇 𝑆 =

𝝈

Page 35: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Measuring Gaussian information

• Purity: 𝜇𝜌 = tr 𝜌2 =1

det 𝝈=

1

Π𝑘𝜈𝑘

• Renyi entropies: 𝑆𝑝 𝜌 =log tr 𝜌𝑝

1−𝑝

• For Gaussian states: go to the Williamson form, to find:

• tr 𝜌𝑝 = 𝑔𝑝(𝜈𝑘)𝑘 , with 𝑔𝑝 𝑥 = 2𝑝/ 𝑥 + 1 𝑝 − 𝑥 − 1 𝑝

• Von Neumann Entropy: 𝑆 𝜌 = −tr 𝜌 log 𝜌 • Take the limit 𝑝 → 1

• 𝑆 𝜌 = 𝜈𝑘+1

2log

𝜈𝑘+1

2−

𝜈𝑘−1

2log

𝜈𝑘−1

2𝑁𝑘=1

Page 36: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

• Renyi entropies: 𝑆𝑝 𝜌 =log tr 𝜌𝑝

1−𝑝

• tr 𝜌𝑝 = 𝑔𝑝(𝜈𝑘)𝑘 , with 𝑔𝑝 𝑥 = 2𝑝/ 𝑥 + 1 𝑝 − 𝑥 − 1 𝑝

Measuring Gaussian information

0 1 2 3 4 50.0

0.5

1.0

1.5

2.0

2.5

3.0

n

Sp

p

1

2

1

2

3

5

10

20

for a single-mode

thermal state:

𝝈 =2𝑛 + 1 0

0 2𝑛 + 1

Page 37: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Measuring Gaussian information

• General remark: the von Neumann entropy is special in

quantum information theory because it is the only one

which satisfies the strong subadditivity inequality:

• However, if one restricts to Gaussian states, then there is

another entropy which satisfies the strong subadditivity:

the Renyi entropy of order 𝑝 = 2: 𝑆2 𝜌 =1

2log det 𝝈

• Interestingly, this entropy is essentially the Shannon

entropy of the Wigner function intended as a continuous

probability distribution in phase space…

G. Adesso et al., Phys. Rev. Lett. 109, 190502 (2012)

Page 38: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Entanglement of Gaussian states

• The continuous variable analogue of a Bell state is…

momentum- squeezed (𝑟)

position- squeezed (𝑟)

Beam Splitter 50:50

Two-mode squeezed state (‘Twin Beam’)

𝝈𝐴𝐵 𝑟

= 𝐵1,2 1 2 ⋅

𝑒2𝑟 00 𝑒−2𝑟

𝟎

𝟎 𝑒−2𝑟 00 𝑒2𝑟

⋅ 𝐵12𝑇 1 2

=

cosh 2𝑟 00 cosh (2𝑟)

sinh (2𝑟) 00 −sinh (2𝑟)

sinh (2𝑟) 00 −sinh (2𝑟)

cosh (2𝑟) 00 cosh (2𝑟)

Page 39: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Entanglement of Gaussian states

• It approximates the EPR state

momentum- squeezed (𝑟)

position- squeezed (𝑟)

Beam Splitter 50:50

Two-mode squeezed state (‘Twin Beam’)

• EPR correlations:

𝜁 =1

2Var 𝑞 𝐴 − 𝑞 𝐵 + Var 𝑝 𝐴 + 𝑝 𝐵

=1

2[ 𝑞 𝐴 − 𝑞 𝐵

2 + 𝑝 𝐴 + 𝑝 𝐵2 ]

= …

𝝈𝐴𝐵 𝑟

=

cosh 2𝑟 00 cosh (2𝑟)

sinh (2𝑟) 00 −sinh (2𝑟)

sinh (2𝑟) 00 −sinh (2𝑟)

cosh (2𝑟) 00 cosh (2𝑟)

Page 40: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Entanglement of Gaussian states

• It approximates the EPR state

momentum- squeezed (𝑟)

position- squeezed (𝑟)

Beam Splitter 50:50

Two-mode squeezed state (‘Twin Beam’)

• EPR correlations: 𝜁 = 𝑒−2𝑟

• # dB = 10 Log10 𝑒2𝑟

• 𝑟 ≈ 1.15

• EPR correlations: 𝜁 = 𝑒−2𝑟 ≈ 0.1

Page 41: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Quantifying entanglement: pure states

• Entropy of Entanglement :

• 𝐸 𝜌𝐴𝐵 = 𝑆 𝜌𝐴 = 𝑆 𝜌𝐵 where 𝜌𝐴 is the marginal state of mode

𝐴, obtained by partial trace over mode 𝐵 (and viceversa for 𝜌𝐵)

• 𝑆 𝜌 = 𝜈𝑘+1

2log

𝜈𝑘+1

2−

𝜈𝑘−1

2log

𝜈𝑘−1

2𝑁𝑘=1

• each mode is locally thermal, only one 𝜈𝑘 = cosh 2𝑟 … substitute…

𝐸 𝜌𝐴𝐵 = cosh2 𝑟 log cosh2 𝑟 − sinh2 𝑟 log sinh2 𝑟

𝝈𝐴𝐵 𝑟 =

cosh 2𝑟 00 cosh (2𝑟)

sinh (2𝑟) 00 −sinh (2𝑟)

sinh (2𝑟) 00 −sinh (2𝑟)

cosh (2𝑟) 00 cosh (2𝑟)

𝝈𝐴

Page 42: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Quantifying entanglement: pure states

• Entropy of Entanglement for a two-mode squeezed state

𝐸 𝜌𝐴𝐵 = cosh2 𝑟 log cosh2 𝑟 − sinh2 𝑟 log sinh2 𝑟

0 1 2 3 4 50

2

4

6

8

10

12

14

r

Eeb

its

For large 𝑟, it goes like

~2

ln 2 𝑟

𝑟 ≈ 1.15 corresponds to

a bit more than 2 ebits

Page 43: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Quantifying entanglement: pure states

• Multimode states: phase-space Schmidt decomposition

𝝈𝑝 =

𝝈1 𝜺1,2

𝜺1,2𝑇 𝝈2

𝜺1,3 𝜺1,4 𝜺1,5𝜺2,3 𝜺2,4 𝜺2,5

𝜺1,3𝑇 𝜺1,4

𝑇

𝜺1,4𝑇 𝜺2,4

𝑇

𝜺1,5𝑇 𝜺2,5

𝑇

𝝈3 𝜺3,4 𝜺3,5

𝜺3,4𝑇 𝝈4 𝜺4,5

𝜺3,5𝑇 𝜺4,5

𝑇 𝝈5

A

B

𝑁 = 5, 𝑁𝐴 = 2, 𝑁𝐵= 3

Page 44: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Quantifying entanglement: pure states

• Multimode states: phase-space Schmidt decomposition

Set:

Then, each

is a two-mode squeezed

state between one mode

in A and one mode in B

Page 45: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Quantifying entanglement: pure states

• Multimode states: phase-space Schmidt decomposition

• 𝐸 𝜌𝐴𝐵 𝑆(𝜌𝐴) = 𝜈𝑘+1

2log

𝜈𝑘+1

2−

𝜈𝑘−1

2log

𝜈𝑘−1

2𝑁𝑘=1

Set:

Then, each

is a two-mode squeezed

state between one mode

in A and one mode in B

Page 46: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Detecting entanglement: mixed states

• A mixed state is separable (=not entangled)

iff 𝜌𝐴𝐵 = 𝑝𝑖 𝜓𝑖 𝐴 𝜓𝑖 𝐴 ⊗ 𝜑𝑖 𝐵 𝜑𝑖 𝐵𝑖

Criteria for continuous variable systems

• Separability criteria based on uncertainty principle / EPR correlations:

• Define rotated quadratures: 𝑞 𝑗𝜃 = cos 𝜃 𝑞 𝑗 + sin 𝜃 𝑝 𝑗 , 𝑝 𝑗

𝜃 = cos 𝜃 𝑝 𝑗 − sin 𝜃 𝑞 𝑗 ,

• If a bipartite state 𝜌𝐴𝐵 is separable, then

• Sum of EPR variances (Duan et al): Var 𝑧 𝑞 𝐴𝜃 −

1

𝑧𝑞 𝐵𝜃 + Var 𝑧 𝑝 𝐴

𝜃 +1

𝑧𝑝𝐵𝜃 ≥ 𝑧2 +

1

𝑧2

• Product of EPR variances (Giovannetti et al): Var 𝑞 𝐴𝜃 − 𝑞 𝐵

𝜃 × Var 𝑝 𝐴𝜃 + 𝑝𝐵

𝜃 ≥ 1

• Entropic criteria (UFRJ, Walborn, Toscano et al): 𝐻𝛼 𝑞 𝐴𝜃 − 𝑞 𝐵

𝜃 + 𝐻𝛼 𝑝 𝐴𝜃 + 𝑝𝐵

𝜃 ≥ 𝑐𝛼

• If you violate any of the above inequalities, then the state 𝜌𝐴𝐵 is entangled

Page 47: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Criteria for continuous variable systems

• Separability criteria based on partial transposition

• (R Simon 2000) Transposition of 𝜌 ⇔ phase-space momentum reflection

𝜌 → 𝜌𝑇 ⇔ 𝑊𝜌 𝑞, 𝑝 → 𝑊𝜌(𝑞, −𝑝)

• PPT Criterion (Peres-Horodecki ‘96): If a bipartite state 𝜌𝐴𝐵 is separable, then

its partial transpose is positive-definite 𝜌𝑇𝐴 ≥ 0

• Hierarchy of inequalities for continuous variables involving higher order moments

(Shchukin-Vogel 2006) to detect violation of PPT

• Necessary and sufficient criterion for entanglement in 1-vs-N mode Gaussian states

based on second moments only

Page 48: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

PPT criterion for Gaussian states

• 𝜌𝐴𝐵 → 𝜌𝐴𝐵𝑇𝐴 ⇔ 𝝈𝐴𝐵→ 𝝈 𝐴𝐵 = 𝜃𝐴|𝐵𝝈𝐴𝐵𝜃𝐴|𝐵

• Simply flip the sign of all rows and columns referring to 𝑝𝑗 operators

(i.e. the even ones) for the modes 𝑗 belonging to subsystem A

• PPT: if 𝜌𝐴𝐵 (Gaussian) is separable, then 𝝈 𝐴𝐵 is bona fide: 𝝈 𝐴𝐵 + 𝑖Ω𝑁 ≥ 0

• PPT: in terms of symplectic eigenvalues of the partially transposed

covariance matrix, 𝜈 𝑘, then 𝜌𝐴𝐵 separable ⇒ 𝜈 𝑘 ≥ 1 ∀𝑘 = 1,… ,𝑁

• PPT: if 𝜌𝐴𝐵 is Gaussian with min 𝑁𝐴, 𝑁𝐵 = 1 then we have a necessary

and sufficient condition: 𝜌𝐴𝐵 is entangled iff there exists some 𝜈 𝑘 < 1

Page 49: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

PPT criterion for Gaussian states

𝜌𝐴𝐵 → 𝜌𝐴𝐵𝑇𝐴 ⇔ 𝝈𝐴𝐵→ 𝝈 𝐴𝐵 = 𝜃𝐴|𝐵𝝈𝐴𝐵𝜃𝐴|𝐵

Simply flip the sign of all rows and columns referring to 𝑝𝑗 operators (i.e.

the even ones) for the modes 𝑗 belonging to subsystem A

• PPT: if 𝜌𝐴𝐵 (Gaussian) is separable, then 𝝈 𝐴𝐵 is bona fide: 𝝈 𝐴𝐵 + 𝑖Ω𝑁 ≥ 0

• PPT: in terms of symplectic eigenvalues of the partially transposed

covariance matrix, 𝜈 𝑘, then 𝜌𝐴𝐵 separable ⇒ 𝜈 𝑘 ≥ 1 ∀𝑘 = 1,… ,𝑁

• PPT: if 𝜌𝐴𝐵 is Gaussian with min 𝑁𝐴, 𝑁𝐵 = 1 then we have a necessary

and sufficient condition: 𝜌𝐴𝐵 is entangled iff there exists some 𝜈 𝑘 < 1

Page 50: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Two-mode Gaussian states

• By means of local unitary operations, i.e. 𝑆𝐴 ⊕𝑆𝐵 at the phase

space level, the covariance matrix can be transformed in the

above standard form, completely specified by 4 real elements

• 𝑎, 𝑏, 𝑐+, 𝑐−.

• They are in one-to-one correspondence (once we fix the

convention 𝑐+ ≥ 𝑐− ) with the four local symplectic invariants

• det 𝜶 , det 𝜷 , det 𝜸 , det 𝝈

Page 51: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Two-mode Gaussian states

• Apply partial transposition:

~ ~

~

det 𝜶 , det 𝜷 , det 𝜸 , det 𝝈 .

Define 𝚫 = = det 𝜶+ det 𝜷+ 2det 𝜸

det 𝜶 , det 𝜷 , det 𝜸 , det 𝝈 .

Define 𝚫 = = det 𝜶+ det 𝜷− 2det 𝜸

Page 52: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Two-mode Gaussian states det 𝜶 , det 𝜷 , det 𝜸 , det 𝝈 .

Define 𝚫 = = det 𝜶+ det 𝜷+ 2det 𝜸

det 𝜶 , det 𝜷 , det 𝜸 , det 𝝈 .

Define 𝚫 = = det 𝜶+ det 𝜷− 2det 𝜸

• Symplectic eigenvalues of the covariance

matrix 𝝈:

𝜈± =𝚫 ± 𝚫2 − 4det 𝝈

2

• Symplectic eigenvalues of the partial

transpose 𝝈 :

𝜈 ± =𝚫 ± 𝚫 2 − 4det 𝝈

2

In general for two modes, only 𝜈 −can be smaller than zero, so we need only to check it!

Page 53: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Two-mode Gaussian states

• Symplectic eigenvalues of the covariance

matrix 𝝈:

𝜈± =𝚫 ± 𝚫2 − 4det 𝝈

2= 1, 1

• Symplectic eigenvalues of the partial

transpose 𝝈 :

𝜈 ± =𝚫 ± 𝚫 2 − 4det 𝝈

2= 𝑒2𝑟 , 𝑒−2𝑟

for a two-mode

squeezed state

Page 54: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Entanglement measures for mixed states

• Entanglement of formation

• Based on a convex-roof procedure:

• 𝐸𝐹 𝜌𝐴𝐵 = inf{𝑝𝑖,|𝜓𝐴𝐵𝑖⟩

} 𝑝𝑖𝐸(|𝜓𝐴𝐵𝑖⟩) 𝑖 , where 𝜌𝐴𝐵 = 𝑝𝑖 𝜓𝐴𝐵𝑖 𝜓𝐴𝐵𝑖𝑖

is a pure-state decomposition of 𝜌𝐴𝐵

• Logarithmic negativity

• Based on the violation of the PPT criterion

• 𝐸𝑁 𝜌𝐴𝐵 = log ||𝜌𝐴𝐵𝑇𝐴||1 , where ||𝑜||1 is the trace distance, i.e.

the sum of the absolute values of the operator 𝑜

Page 55: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Entanglement measures for mixed states

for Gaussian states

• (Gaussian) Entanglement of formation

• 𝐸𝐹 𝜌𝐴𝐵 = inf{𝑝𝑖,|𝜓𝐴𝐵𝑖⟩

} 𝑝𝑖𝐸(|𝜓𝐴𝐵𝑖⟩) 𝑖

• One restricts the decomposition into pure Gaussian states 𝜓𝐴𝐵𝑖

• Gives in general an upper bound on 𝐸𝐹 (is it tight? open problem)

• For two-mode symmetric Gaussian states, this is exact: the Gaussian decomposition is optimal (Giedke et al 2003)

• Logarithmic negativity

• 𝐸𝑁 𝜌𝐴𝐵 = log ||𝜌𝐴𝐵𝑇𝐴||1 depends on the symplectic eigenvalues of

the partial transpose which can be smaller than 1 (no bona fide)

𝐸𝑁 𝜌𝐴𝐵 =

0, if 𝜈 𝑘 ≥ 1 ∀𝑘

− log 𝜈 𝑘𝑘: 𝜈 𝑘<1

Page 56: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Two-mode Gaussian states

symmetric two-mode states

i.e. 𝑎 = 𝑏, i.e. det 𝜶 = det 𝜷

Page 57: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Two-mode Gaussian states: example

momentum- squeezed

thermal (𝑟, 𝑛 )

position- squeezed

thermal (𝑟, 𝑛 )

Beam Splitter 50:50

Two-mode squeezed thermal state

Page 58: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

CONTINUOUS VARIABLE

QUANTUM INFORMATION

LECTURE III.

Page 59: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Using bipartite entanglement

• Precondition for quantum key distribution (Ekert)

• Quantum dense coding

• Quantum teleportation

• Demonstrations of

nonlocality

• …

Page 60: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Continuous variable teleportation

Two-mode entangled state

A

input state

B

B

A B

(Braunstein & Kimble ‘98

Furusawa et al ‘98)

Page 61: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Continuous variable teleportation

The output converges to the input only for infinite shared entanglement

In general the fidelity between input and output

quantifies the performance of the teleportation network

The optimal fidelity (maximized over local unitaries on the shared symmetric resource state) is a monotonic function of the entanglement distributed between A and B, when the input is a generic coherent state

ℱ =1

1 + 𝜈 −

Page 62: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Benchmark: experiments must achieve fidelities higher than the classical

threshold to demonstrate a genuine quantum transfer based on entanglement

To determine such a threshold: a nontrivial problem of quantum estimation

“ ” Fidelity of the optimal

“measure-and-prepare”

strategy:

classical threshold

Quantum teleportation benchmarks

Cheating teleportation without entanglement

Page 63: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

q

p Input: coherent states with totally unknown displacement

(Hammerer et al. PRL 2005)

(first experiment: Furusawa et al. Science 1998)

Benchmark: 50%

q

p Input: arbitrary single-mode Gaussian state

Benchmark?

**OPEN PROBLEM**

Quantum teleportation benchmarks

Page 64: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Long-term vision

In order to implement quantum

interfaces one needs to be able to:

Entangle multiple nodes

Teleport information through the

channels

Store and retrieve quantum

states from light to matter

Light Atomic ensembles

7

Page 65: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Continuous variable teleportation/storage

• Quantum memory for light (coherent states, squeezed

states) onto atoms (Polzik: Nature 2004, Nature Phys 2011)

• Quantum teleportation between light and matter (Nature 2006)

Page 66: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Continuous variable teleportation/storage

• Deterministic teleportation between macroscopic atomic

ensembles at room temperature (Polzik: Nature Phys. 2013)

Page 67: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Hybrid teleportation (discrete/continuous)

• Using continuous variable teleportation with two-mode

Gaussian resources to teleport non-Gaussian, non-classical

states (e.g. Schroedinger’s kittens) or single-photon states (Furusawa: Science 2011; Nature to appear 2013)

Page 68: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Hybrid teleportation (discrete/continuous)

• The other way around: using qubit teleporters in parallel to

teleport input continuous variable states (Andersen-Ralph, theory,

PRL 2013)

Page 69: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Multipartite quantum resources

mom-sqz r1

pos-sqz r2

pos-sqz r2 BS t =1/N

pos-sqz r2

pos-sqz r2

BS t =1/(N-1)

BS t =1/2

Multipartite symmetric state

Page 70: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Multipartite quantum resources

mom-sqz r1pos-sqz r2

pos-sqz r2BS =1/N

pos-sqz r2

pos-sqz r2

BS =1/(N-1)

BS =1/2

r r ≡≡ ((rr11++rr22)) 22–– //

mom-sqz r1pos-sqz r2

pos-sqz r2BS =1/N

pos-sqz r2

pos-sqz r2

BS =1/(N-1)

BS =1/2

mom-sqz r1pos-sqz r2

pos-sqz r2BS =1/N

pos-sqz r2

pos-sqz r2

BS =1/(N-1)

BS =1/2

r r ≡≡ ((rr11++rr22)) 22–– //

• Genuine N-partite entanglement

Page 71: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Teleportation networks

mom-sqz r1pos-sqz r2

pos-sqz r2BS =1/N

pos-sqz r2

pos-sqz r2

BS =1/(N-1)

BS =1/2

r r ≡≡ ((rr11++rr22)) 22–– //

mom-sqz r1pos-sqz r2

pos-sqz r2BS =1/N

pos-sqz r2

pos-sqz r2

BS =1/(N-1)

BS =1/2

mom-sqz r1pos-sqz r2

pos-sqz r2BS =1/N

pos-sqz r2

pos-sqz r2

BS =1/(N-1)

BS =1/2

r r ≡≡ ((rr11++rr22)) 22–– //

A B

B

B

B B

B

B

B

B B

B

B

B

input state

Page 72: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Teleportation networks (Furusawa, Nature 2004)

Page 73: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Multipartite quantum resources

• More general (non-symmetric) Gaussian tripartite states (P. Nussenzveig, USP, Science 2009)

Page 74: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Open problems with Gaussian states

• Entanglement of formation for general Gaussian states

• Strong monogamy of multipartite entanglement for arbitrary Gaussian states

• Quantum teleportation benchmarks for Gaussian states* *not open for long

• Quantum benchmarks for cloning, amplifying, etc…

• Additivity of the output entropy for Gaussian channels

• Nonlocality: are all mixed Gaussian entangled states nonlocal? Maximal violations of Bell inequalities?

• Are Gaussian measurements optimal for quantum discord?

• Technological challenges: increase squeezing level etc.

• …

Page 75: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Gaussian states

Page 76: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Limitations and no-go’s

• Extremality of Gaussian states (Wolf-Giedke-Cirac PRL 2006)

• “Among all continuous variable states with given first moments and

covariance matrix, the Gaussian state has the lowest entanglement”

• Consequences (-): criteria based on second moments can only give

sufficient conditions to detect entanglement in non-Gaussian states

• Consequences (+): e.g. at fixed

squeezing, you can engineer

non-Gaussian states with higher

entanglement than the twin-beam

• This can be done e.g. by

de-Gaussifying the state

(e.g. photon subtraction/addition)

(Grangier PRL 2007)

Page 77: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Limitations and no-go’s

• Gaussian entanglement distillation

• “It is impossible to distill Gaussian states with Gaussian operations”

• You need to resort to de-Gaussification (and re-Gaussification)

(Furusawa, Nat. Photon. 2010)

Page 78: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Limitations and no-go’s

• Gaussian quantum error correction

• Gaussian quantum bit commitment

• …

• Optimal cloning of a coherent state

Fidelity of the best Gaussian

clone: 2/3=0.6666…

Optimal fidelity (for a non-

Gaussian clone): 0.6826…

Page 79: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

One-way CV quantum computation

• Gaussian cluster states can be used, but

• Non-Gaussian measurements are required

Page 80: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

One-way CV quantum computation

• Gaussian cluster states can be used, but

• Non-Gaussian measurements are required

10000-temporal-mode cluster state!!!

(Furusawa, …, S. Armstrong,… Nat. Phot. 2013)

Page 81: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Parameter estimation

We need to transmit quantum states through a noisy medium (e.g. an optical fiber)

We can model the channel by means of a master equation

that depends on some parameter, say f

To gain a control over the state transfer one needs to estimate f

This consists in two steps:

1. Devising the optimal input state (probe)

2. Determining the optimal measurement on the output

After repeating N times, one constructs an estimator for f

Optimal estimation minimum variance of the estimator

in out

f

PREPARE

TRANSMIT

MEASURE

ˆ

Page 82: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Quantum Estimation Theory (basics) • For each prepare and measure strategy S, one can construct an

unbiased estimator of minimum variance given by

where the classical Fisher Information is a figure of merit

characterizing the performance of the strategy

• At fixed input probe, the quantum Cramér-Rao bound states that

for any strategy one has

• There exists an optimal POVM yielding maximum sensitivity, that

consists of projections on the eigenstates of the symmetric

logarithmic derivative L, defined implicitly as

• The classical Fisher information associated to such optimal

measurement is known as quantum Fisher information (QFI)

• The QFI can be also computed from the Bures metric of the evolved

states and is thus related to the quantum fidelity between

infinitesimally close states

• Finding the QFI solves the second step, optimizing over the output

measurement. We are left to find the optimal input probe states.

1ˆ Var[ ] ( )N I S

0 0 0( , ) ( , ) ( )I I H

2 /d dr

2

0( ) Tr[ ]rH

0

Page 83: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Bosonic channels

Dissipation channel

Amplification channel

Dephasing channel

0

tan [ ]d

L ad

†tanh [ ]d

L ad

†tan [ ]d

aL ad

† † †[ ] 2L o o o o o o o

Gaussian channels (map Gaussian states

into Gaussian states)

Page 84: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

out

out

Ultimate bounds on precision

f

0

0

BEAM SPLITTER

(transmittivity)

f

0

0

PARAMETRIC

AMPLIFIER

(squeezing)

DIS

SIP

AT

ION

A

MP

LIF

ICA

TIO

N

…measuring system + environment…

n : mean input energy

max 4H n

max 4 1H n

These bounds are tight! (B. Escher, .. L. Davidovich, Nature Phys. 2011)

Page 85: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

The optimal probes are non-Gaussian D

ISS

IPA

TIO

N

AM

PL

IFIC

AT

ION

n : mean input energy

max 4H n

max 4 1H n

0 p

8

p

4

p

2 3 p

8

p

2

2.0

2.5

3.0

3.5

4.0

f

H

n = 1

0 p

8

p

4

p

2 3 p

8

p

2

10 12 14 16 18 20

f

H

n = 5

0 p

8

p

4

p

2 3 p

8

p

2

40

50

60

70

80

f

H

n = 20

0 p

8

p

4

p

2 3 p

8

p

2

100 120 140 160 180 200

f

H

n = 50

Ultimate bound ≡ Fock input and photon counting strategy

Best Gaussian probes

Coherent states and

heterodyne detection

(G. Adesso et al. PRA(R) 2008, PRL 2010)

Page 86: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Non-Gaussian wild world

Page 87: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Continuous variables: more open problems

• Resource theory for non-Gaussianity

• The cheap states/operations are Gaussian (like separable

states/LOCC for entanglement)

• A measure of non-Gaussianity for a general state 𝜌 is the minimum

relative entropy between 𝜌 and the closest Gaussian state (Genoni et

al 2009)

• This measure is well motivated, invariant under symplectic

operations, obviously zero for Gaussian states, and moreover it can

be computed…

• The closest Gaussian state is the one with the same first and second

moments as 𝜌 (Marian & Marian 2013)

• So what is missing?

• An operational interpretation for non-Gaussianity

Page 88: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Continuous variables: more open problems

• Efficient criteria for entanglement of non-Gaussian states

• Efficiently computable entanglement measures/bounds

• Optimal strategies for parameter estimation of CV channels

• …

• Technological improvements for generation, manipulation, measurement

of non-Gaussian states (better sources, better detectors, etc. etc.)

• Hybrid, hybrid, hybrid: use the best of different worlds for integrating

quantum communication networks (e.g. for cryptography, teleportation,

computation)

• … .. …

• Just follow your curiosity

Page 89: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

CONTINUOUS VARIABLE

QUANTUM INFORMATION

Page 90: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Further reading

• Quantum information with continuous variables

• (General) S. L. Braunstein and P. van Loock, Rev. Mod. Phys. 77, 513 (2005).

• (Gaussian) C. Weedbrook, S. Pirandola, R. Garcia-Patron, N. J. Cerf, T. C. Ralph, J.

H. Shapiro, and S. Lloyd, Rev. Mod. Phys. 84, 621 (2012).

• (Book) "Quantum information with continuous variables" edited by S. L. Braunstein

and A. K. Pati (Springer, 2003)

• (Book) "Quantum Information with Continuous Variables of Atoms and Light” edited by

N. Cerf, G. Leuchs, and E. S. Polzik, (Imperial College Press, 2007).

• Introduction to continuous variable entanglement

• (General) J. Eisert and M. B. Plenio, Int. J. Quant. Inf. 1, 479 (2003)

• (Gaussian) G. Adesso and F. Illuminati, J. Phys. A: Math. Theor. 40, 7821 (2007)

• State engineering / physical implementations

• (General/optics) F. Dell’Anno, S. De Siena, and F. Illuminati, Phys. Rep. 428, 53 (2006)

• (Atoms/interfaces) H. Ritsch, P. Domokos, F. Brennecke, and T. Esslinger, Rev. Mod.

Phys. 85, 553 (2013)

• […]

Page 91: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Thank you!

Gerardo Adesso

School of Mathematical Sciences

The University of Nottingham

[email protected]

http://quantumcorrelations.weebly.com

https://www.facebook.com/QuantumCorrelations

Page 92: CONTINUOUS VARIABLE QUANTUM INFORMATION · Gaussian states q p are states whose Wigner distribution is a Gaussian function in phase space • Recall: Gaussian probability function

Let’s thank the organisers

of this fantastic school !!!

Antonio Zelaquett Khoury (Fluminense Federal University - UFF)

Eduardo Novais (Federal University of ABC - UFABC)

Fabricio Toscano (Federal University of Rio de Janeiro - UFRJ)

Ivan Oliveira (Brazilian Center for Physics Research- CBPF)

Marcos Cesar de Oliveira (State University of Campinas - UNICAMP)

Raul O. Vallejos (Brazilian Center for Physics Research- CBPF)

Roberto Imbuzeiro Oliveira (National Institute of Pure and Applied Math - IMPA)