slide1 n.
Download
Skip this Video
Loading SlideShow in 5 Seconds..
Quantum information in bright colors PowerPoint Presentation
Download Presentation
Quantum information in bright colors

Loading in 2 Seconds...

play fullscreen
1 / 42

Quantum information in bright colors - PowerPoint PPT Presentation


  • 78 Views
  • Uploaded on

Quantum information in bright colors. Paulo A. Nussenzveig. Instituto de Física - USP. Paraty – 2009. The Team. Antônio Sales Felippe Barbosa Jonatas César Luciano Cruz Paulo Valente. Katiúscia Cassemiro Alessandro Villar Marcelo Martinelli Paulo Nussenzveig. Lectures.

loader
I am the owner, or an agent authorized to act on behalf of the owner, of the copyrighted work described.
capcha
Download Presentation

PowerPoint Slideshow about 'Quantum information in bright colors' - zarifa


An Image/Link below is provided (as is) to download presentation

Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author.While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server.


- - - - - - - - - - - - - - - - - - - - - - - - - - E N D - - - - - - - - - - - - - - - - - - - - - - - - - -
Presentation Transcript
slide1

Quantum information in bright colors

Paulo A. Nussenzveig

Instituto de Física - USP

Paraty –2009

slide2

The Team

Antônio Sales

Felippe Barbosa

Jonatas César

Luciano Cruz

Paulo Valente

Katiúscia Cassemiro

Alessandro Villar

Marcelo Martinelli

Paulo Nussenzveig

slide3

Lectures

  • 1st Lecture – Continuous variables (CV): entanglement, squeezing, OPO basics.
  • 2nd Lecture – More on OPOs, bipartite entanglement below and above threshold.
  • 3rd Lecture – Direct generation of tripartite three-color entanglement; “Entanglement Sudden Death” in a CV system.
slide6

EPR’s example

|y  d(x1 – x2 – L)d(p1 + p2) (localized in x1 – x2 and p1 + p2)

A measurement of x1 yields x2, just as a measurement of p1 gives p2. But x2 and p2don’t commute! ↔ [x, p] = i ħ

slide7

EPR’s conclusion

If (1) is false, then (2) is also false! Hence, (1) should be true: quantum theory, although it allows for correct predictions, must be incomplete. Measurements should just reveal pre-existing states, which are not described by this incomplete theory.

slide8

Bohr’s reply

Bohr discusses complementarity, but his paper does not give sufficient arguments to rule out the EPR program. (This story goes on with the theorems by John Bell and experiments to violate Bell’s inequalities, and GHZ-states etc.)

slide9

Quantum Optics

It is our purpose here to investigate these “spooky” correlations by using electromagnetic fields. Our bright beams of light have properties that are described just as position and momentum observables. We begin by describing these properties and then we will study them in a specific system, the optical parametric oscillator (OPO). Borrowing a line from an anonymous reviewer, these systems are of “great interest to the quantum information community, but also to a broad audience interested in the latest progress on sophisticated optical systems designed for quantum information applications”.

slide12

Field Quantization

Each mode is a harmonic oscillator, with the Hamiltonian

given the commutation relations

The electric field is:

slide13

Field Quadratures

The electric field can be decomposed as

And also as

X and Y are the field quadrature operators, satisfying

Thus,

slide14

Quantum Optics

Field quadratures behave just as position and momentum operators. Thus, we can expect to observe phenomena such as EPR-type correlations among optical fields.

Before we proceed, we notice that the uncertainty relation sets a minimum bound on the product of the variances of orthogonal quadratures. For coherent states the variances are both equal to 1 (the so-called Standard Quantum Limit – SQL). For squeezed states one variance is smaller than 1, while the orthogonal quadrature necessarily has excess noise.

slide16

Noise Measurements

±

S.A.

(Balanced) Homodyne Detection

D2

BS

D1

If field b is strong, we can replace the operator by its mean value

If field b is the vacuum, we can obtain A’s intensity noise by measuring n+

slide17

The Optical Parametric Oscillator (OPO)

The Optical Parametric Oscillator (OPO)

New quantum light from a classic system

slide18

Crystal

~1064 nm

532 nm

Optical Parametric Oscillator (OPO)

OPO

Idler

Pump

Signal

slide20

Optical Parametric Oscillator (OPO)

Let us describe classical properties of the system before we analyze quantum properties. We’ll consider a Triply Resonant OPO (TR-OPO) in a ring cavity (for simplicity).

a0in

a1out

R=1

a0out

a2out

The hamiltonian has three terms:

r0

r1

r2

R=1

slide21

Optical Parametric Oscillator (OPO)

The amplitudes will be given in photon flux (photons per second). If we consider that the single pass gain is small, we can approximate the equations for the amplitudes, for propagation inside the crystal as:

And, for a round trip:

slide22

Optical Parametric Oscillator (OPO)

If djj is small, we can write:

where the total loss for each mode is defined

Normalizing the detuning, we have

slide23

Optical Parametric Oscillator (OPO)

A first solution of these equations is a1 = a2 = 0, corresponding to operation below threshold. We are more interested in above-threshold operation. Multiplying the complex conjugate of the third equation by the second, we have: 

The intracavity pump power is easily obtained and we see it is “clipped”: above-threshold it is always the same

Besides, for , we also have

The classical equations are already signaling that the intensities of signal and idler beams should be strongly correlated and that the pump must be depleted.

slide24

Optical Parametric Oscillator (OPO)

From the first equation we can derive the threshold power, given the intracavity pump field (a1 = a2 = 0)

An important parameter will be the ratio of incident power to threshold power on resonance:

Substituting a2 in the first equation, we have

slide25

Optical Parametric Oscillator (OPO)

and

Since

We get

Solving for aj

slide26

Optical Parametric Oscillator (OPO)

This gives the photon flux. Considering, for the sake of the argument, the frequency-degenerate case (w1=w2=w0/2), we can obtain the total output power and the efficiency

Where hmax is the maximum efficiency leading to

We will see that the parameter x determines the maximum squeezing in the above-threshold OPO.

slide27

Quantum properties of the OPO

We resume from the Hamiltonian and the master equation:

We will sketch the general method, which consists of choosing a representation (quasi-probability distribution) and converting the master equation into a set of stochastic differential equations. Our choice is to use the Wigner function, in spite of the fact that higher-order derivatives appear, which we simply neglect…

slide28

Quantum properties of the OPO

The operators are replaced by amplitudes

and the density operator is replaced by

Using the rules

slide29

Quantum properties of the OPO

We obtain

Neglecting higher-order derivatives, we have a Fokker-Planck equation

slide30

Quantum properties of the OPO

Which is equivalent to a set of Langevin equations

The mean values in steady state are the same as in the classical treatment. Since we will (typically) deal with intense fields, we proceed by linearizing the fluctuations, neglecting products of fluctuating terms:

slide32

Quantum properties of the OPO

The subspace related to the subtraction of the fields decouples from the sum and the pump fluctuations. However, q- does not have any decay term, thus the solutions are not strictly stable. As a matter of fact, there is phase diffusion and the subtraction of the phases is unbounded. Nevertheless, this is a slow process and we will be interested in measuring phases with respect to the phase of the mean field (in other words, we will follow “adiabatically” the diffusion).

Instead of solving these equations in the time domain, we look instead in the frequency domain.

wiener khintchine theorem

This problem was removed by Wiener and Khintchine who noticed that the auto-correlation function

is well defined for a large number of functions z(t), approaching zero when    if z(t) = 0.

Wiener-Khintchine theorem
  • We wish to study a stationary random process z(t)
  • We can try

where S() would represent the strength of fluctuations associated to a Fourier component of z(t).

  • However, z(t) is nonzero for t  , so the above definition is not mathematically sound.

From Optical Coherence and Quantum Optics, L. Mandel e E. Wolf

slide34

Wiener-Khintchine Theorem

The auto-correlation function and the spectral density (or power spectrum) are related by Fourier transforms.

Experimentally

Spectrum Analyzer

Time series of photocurrent measurements

Power spectrum

Auto-correlation function

Wiener-Khintchine theorem

slide35

Singularities in the power spectrum

  • A well-behaved function can be obtained again by writing z(t) = z + z0(t), where z0(t) has a zero mean. For z0(t), we have

0(0) gives the variance of z(t)

Singularity removal in S()

Experimentally

Our Detector

light

z0(t)

Spectrum Analyzer

DC Filter

z(t)

HF output

z(t)

Oscilloscope

DC output

  • If z  0, then ()  |z|2 for   . This causes singularities to appear in S().
slide36

Wait: not so fast!

What do we really measure? How about the commutation relations? How do we define the SQL?

i(t)

Field operators depend on time, leading to slight changes in the commutation relations:

slide37

Wait: not so fast!

In the frequency domain,

In every detection system, we have a finite bandwidth, so we measure

slide38

OK, back to the OPO

We concentrate on the subtraction subspace:

The Fourier transform is

giving

slide39

OK, back to the OPO

The output field fluctuations are

Finally,

slide40

OK, back to the OPO

The subtraction subspace gives a minimum uncertainty product, for D = 0.

Twin beams!