1 / 27

Dispersion Cancellation in an HOM Interferometer: Collapse vs Correlations

This article discusses the concept of dispersion cancellation in an HOM interferometer and its usefulness for time measurements. It covers topics such as indirect measurements, energy-time uncertainty relation, and number-phase uncertainty relation in states of an electromagnetic mode.

Download Presentation

Dispersion Cancellation in an HOM Interferometer: Collapse vs Correlations

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. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Dispersion cancellation in an HOM interferometer (more "collapse versus correlations") (useful for time measurements) What are time measurements? (no time operator) (indirect measurements) (energy-time "uncertainty relation") States of an electromagnetic mode (number-phase "uncertainty relation") (homodyne measurements, et cetera) Phase of a single photon... Frequency and time... dispersion-cancellation, optical phase, etc. (AKA: A bunch of loosely connected stuff I decided I need to cover before I get to some other stuff...) 28 Oct 2003

  2. Entangled photon pairs(spontaneous parametric down-conversion) The time-reverse of second-harmonic generation. A purely quantum process (cf. parametric amplification) Each energy is uncertain, yet their sum is precisely defined. (For a continuous-wave pump!) Each emission time is uncertain, yet they are simultaneous.

  3. Hong-Ou-Mandel interferometer Remember: if you detect only one photon, the other photon "knows" where yours came from. Hence there is no interference (each detector sees 1/2 of the photons, irrespective of any phases or path-length differences). But: if you detect both photons, there is no way to tell whether both were reflected or both were transmitted. r2+t2 = (i2 + 12)/2 = 0. (any lossless symmetric beam splitter has a p/2 phase shift between r and t.) CAVEAT: there must be no way to tell which occurred. If the paths aren't aligned right, no interference occurs. If one photon reaches the beam splitter before the other, no interference occurs. How long is a photon?

  4. the famous dip COINCIDENCE RATE DELAY TIME (fs) Instead of an amplitude for each frequency component of each beam, there is an amplitude for each frequency-correlated pair of photons. Energy-entangled state. In every experiment to date, the width of this feature is limited only by the bandwidth of the photons; in other words, the photons are as tightly correlated as they could possibly be given their own uncertainty in time (Dt > 1/2Dw).

  5. What's the speed of a photon? Silly questions about group velocity, phase velocity, "collective" nature ofthe index of refraction, precursors, et cetera. More serious questions about how to quantize electromagnetic fields in a dispersive medium. Longstanding debate about "superluminal" tunneling.

  6. Problem with propagation measurements Quadratic term leads to group-velocity dispersion, broadening, chirp.

  7. But wait!

  8. So, what can we predict? Coinc. probability is an integral over all times at which D1 and D2 could fire: UGH! Each E is an integral over its own frequency! But... if T goes to infinity, life simplifies: We have only to integrate a†a†aa over all w1, w2. Detectors are "infinitely slow" (ns = 106 fs);... The physical meaning: calculate the probability for each pair of frequencies which might reach the two detectors, and then integrate. Why? No interference between paths leading to different frequencies at the detectors, because in principle one could go back and measure how much energy had been absorbed. Note: it took a long time-integral to enforce this. If the detector had been open only for 1 fs, it would be impossible to tell what frequency it had seen.

  9. No, we're not done yet... (one can always insert a complete set of states.) (the square of the two-photon amplitude) The probability of detecting a given frequency pair: But we only started with 2 photons, so if we annihilate 2, there will be 0 left: the phase difference is all that concerns us: Note 1: the GVD terms (quadratic in freq.) cancelled out. Note 2: the pattern moves at the group velocity. Note 3: the shape is the Fourier transform of f(w), like the pulse itself.

  10. Nonlocal cancellation of dispersion (Oh, and by the way... yeah, single-photon pulses travel at the group velocity.)

  11. The Feynman path picture REMEMBER: interference only occurs between two paths which yield the same w1 and the same w2. If in the TT path, a "blue" photon is detected at D1 (and a "red" at D2), then I must compare with the phase of an RR path with the same outcome... The two paths are indistinguishable even though in each case one of the pulses was broadened. Perfect interference occurs.

  12. The collapse picture After D1 fires, it projects the light in arm 2 into a superposition of two identical chirped wave packets-- these two packets exhibit perfect interference.

  13. But how do you really measure time? Clock Oscilloscope x(t): Time-to-amplitude converter Vout = V' t There is no such thing as a direct time measurement, even classically. "The position of an electron" has some meaning... but what is "the time of an electron"? In QM (as in CM), time is a free parameter, not an operator/observable. Time is always measured by observing a pointer which is believed to evolve at a constant rate, and "triggering" its evolution (or at least readout).

  14. What's the shortest time you can measure? For this "clock" system to evolve appreciably in a time t, it must have an energy uncertainty greater than h/t. "Energy-time uncertainty principle." Warning: oddly, the reverse is not true. You can measure energy arbitrarily well in an arbitrarily short time [Aharonov + Bohm, Phys Rev 122, 1649 (1961)]. Why no rigorous uncertainty principle? Because time is not an operator. Energy (the Hamiltonian) is the generator of time-translations. A canonically conjugate time operator would generate energy-translations. But energy is bounded (at least from below); no Hermitian T-operator exists.

  15. Can you use photons as a clock? Of course; Electric field changes very rapidly, on the order of 1015 Hz: (even microwave -- Cs atomic clock -- yields 9•109 Hz) But wait... the energy of a photon is completely certain. Energy eigenstate = stationary state: In a single-photon state, there "are" oscillations with a known amplitude... but since their time origin is completely uncertain, so is E(t). Compare an eigenstate of the harmonic oscillator- the maximum X is related to the energy, but the particle's equally likely to be at +X or -X.

  16. What does this mean? Remember: two photons meeting at a beam-splitter don't interfere. |1> |1> n1 n2 The cross terms change n1 and n2; unless these numbers are uncertain, these terms vanish. Optical phase actually refers (roughly) to the quantum phase difference between the amplitude to have n photons and the amplitude to have n+1.

  17. Uncertainty relations? What is phase, except time? What is photon-number, except energy?

  18. Phase-space picture E2 (think p) E2 (think p) E2 (think p) |E| f E1 (think x) E1 (think x) E1 (think x) minimum phase-space area, as for X and P of a particle. A phase-space distribution for a 1-photon state A "coherent" or "quasiclassical" state. complex E = |E| eif e-iwt = E1 cos wt + E2 sin wt The vacuum isn't empty:

  19. Electric field of a coherent state (nice pictures stolen from Gerd Breitenbach's web page) E t

  20. How does one measure these things? With a radio-frequency field, of course, one measures E with an antenna, in real time. Not possible at optical frequencies - we can only detect power/energy/photons. Homodyning/heterodyning: interfere a signal with a strong oscillator. |Es eif + |ELO| |2 |ELO|2 + 2 |ELO|Es cos f + ... By varying phase of local oscillator, can measure different quadratures just by measuring intensity. Note: not so different from RF; your oscilloscope has a local oscillator too.

  21. E t E1 E2

  22. n

  23. Entangled state |01> + |10>; no definite number in either arm. Back to Bohr & Einstein(and Young and Taylor,...) So, does a single photon exhibit interference, or not?! |1>

  24. Some references (incomplete for now!) Dispersion cancellation: http://home.t-online.de/home/gerd.breitenbach/gallery/ for info & pictures about squeezed-states and their measurement. Uncountable textbooks & review articles... see for instance Loudon; Walls & Milburn; Scully & Zubairy. Glauber for quantum optics formalism Clauser for early work on classical versus quantum effects Grangier et al. for experiment on true single-photon interference. Thought for next week: atom number is conserved (unlike photon number). Can it be uncertain? Should two atom clouds interfere with one another or not?

More Related