Quantum Interference 1 Claude Cohen-Tannoudji Scott Lectures Cambridge, March 7
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Quantum Interference 1 Claude Cohen-Tannoudji Scott Lectures Cambridge, March 7
Quantum Interference 1 Claude Cohen-Tannoudji Scott Lectures Cambridge, March 7th 2011 Collège de France 1 Description of the state of an atom by populations of the energy levels Atom in thermodynamic equilibrium The state is completely described by the populations n of the energy levels En. n = E n E n e En / k B T n : diagonal elements of the density operator in the basis {En}. The off diagonal elements are equal to zero. : statistical mixture of states En with weights n. Master equation for the populations The time evolution of the populations n of the states En can often be described in terms of transition rates Wnn‘ from one state to another one: n = Wn n n + Wnn n n n n n 2 Linear superpositions of states An atom can also be prepared in a linear superposition of the states En. = cn En n The physical properties of this atom then depend not only on the IcnI2, but also on the crossed terms cncn’* (with nn‘ ). If the state of the atom is not a pure state like , but a statistical mixture of states, the density matrix can have non diagonal elements nn‘ (with nn‘). En En = n n = cn cn* 0 cn cn* : average over the states of the statistical mixture. The relative phase of the coefficients cn and cn‘ does not average to zero. nn‘ is often called “coherence” between the states En and En‘ 3 Purpose of this series of lectures Review a few physical effects associated with the existence of atomic coherences ij •How to prepare and detect these coherences? •How do they evolve? •What are the new effects to which they give rise? •What are the possible applications? The states which are linearly superposed can be - two Zeeman sublevels of the same atomic level e or g in which case ij is called a “Zeeman coherence” - two different states corresponding to two different spatial localizations of the atom, in which case ij is called a “spatial coherence” - two different states of an ensemble of 2 systems 1 and 2. If this state 12 cannot be written as a product of a state 1 of 1 by a state 2 of 2, we have an “entangled state” with 4 remarkable properties Lecture 1 : Zeeman coherences •Level crossing resonances in excited and ground states •Quantum beats. Time resolved spectroscopy •Ramsey fringes and microwave atomic clocks •Dark resonances. Coherent population trapping Lecture 2 : Spatial coherences •Coherence length •Young’s fringes with atomic de Broglie waves •Feynman path approach to atomic interferometry •Atomic interferometers Lecture 3 : Entangled states •Examples of entangled states. How to prepare them •Entangled states and non separability. Bell’s inequalities •Entangled states and which path information •Entangled states and measurement process. Decoherence •Entangles states and two-photon interference 5 Outline of lecture 1 1 – Level crossing resonances in excited states 2 – Quantum beats. Time resolved spectroscopy 3 – Extension to ground states 4 – Ramsey fringes and microwave atomic clocks 5 – Dark resonances. Coherent population trapping 6 Level crossing resonance in the excited state e E e1 B0 Excitation with polarization e2 B0C Detection with polarization ' B0 A static magnetic field B0 is scanned around a value B0C where e1 and e2 cross (Ee1=Ee2), for example in B0=0. Optical excitation with polarization . Detection of the fluorescence with polarization ' et ' are linear superpositions of the polarizations 1 and 2 associated with transitions g-e1 and g-e2 . How does the intensity of the fluorescence vary with B0? 7 Interferences between scattering amplitudes g g e1 e2 g g There are two different pathes for going from the same initial state g, to the same final state g, , the first one passing through e1 , the second one through e 2 They are both open because and are linear superpositions of the polarizations of the transitions g e1 and g e2 The transition amplitude is a sum of 2 amplitudes, one for each path A ( e g ) e g = Ee Eg / 1 1 1 A1 A2 + + i ( e / 2) e g + i ( e / 2) ( ) 2 e g = Ee Eg / 2 2 e : Natural width of e Both amplitudes can be simultaneously large if e g = e g Resonant variations of the fluorescence near the crossing point 1 2 8 Equation of evolution of 12 The rate of variation of 12 is given by a sum of 3 terms: - A term describing the excitation process. For a broad line excitation, it is given by d 12 / d t exc = W gg ( ) W: rate coefficient proportional to the light intensity. For low intensity, one can neglect the depletion of g and replace gg by 1 - A term describing the free evolution (Larmor precession) E1 E2 d 12 / d t free evol = i 12 = i 0 12 with E2 E1 = 0 ( ) - A term describing the departure rate from e with a rate (d 12 / dt ) spont em = 12 Adding these 3 rates, one gets d 12 = W + i 0 12 12 dt 9 Steady-state solution If the light intensity is constant, W is time independent and the equation of evolution of -1+1 has a steady-state solution: st 1+1 W = i 0 The detection signal contains a term proportional to Re -1+1 equal to W 2 + 02 which is a Lorentz curve centered around B0=0, with a width much smaller than the spectral width of the exciting light This zero field level crossing resonance has been observed for the first time by W.Hanle and it is called the “Hanle effect” W.Hanle, Z.Phys. 30, 93 (1924) and 35,346 (1926) Similar level crossing resonances have been also observed around the non zero magnetic field value where two Zeeman sublevels originating from 2 different hyperfine levels cross. This is called the “Franken effect”. F.Colegrove, P.Franken,R.Lewis,R.Sands, Phys.Rev.Lett. 3, 420 (1959) 10 Outline of lecture 1 1 – Level crossing resonances in excited states 2 – Quantum beats. Time resolved spectroscopy 3 – Extension to ground states 4 – Ramsey fringes and microwave atomic clocks 5 – Dark resonances. Coherent population trapping 11 Pulsed excitation. Quantum beats The rate coefficient W is then no longer constant and must be replaced by a delta function of t in the equation of evolution of 12 d 12 / d t = W0 (t) i 12 12 12 The solution of this equation is given by: 12 (t) = W0 (t) e i 12 t e t (t): Heaviside function The excitation prepares the coherence 12 in a very short time. This coherence then evolves freely at the frequency 12 and is damped with a rate . This evolution is detected as a damped oscillation of the intensity of the fluorescence light which contains a term proportional to 12. Analogy with the sound beats which are heard after a short percussion of 2 different piano strings 12 First observation of quantum beats Excited states of cadmium J. Dodd, R. Kaul, D. Warrington, Proc. Phys. Soc. 84, 176 (1964) See also E. Aleksandrov Optics and Spectroscopy 17, 522 (1964) Time-resolved spectroscopy An ultra short laser pulse (femtosecond laser) excites a linear superposition of vibration states of a molecule. One gets in this way a wave packet which oscillates at the vibration frequency of the molecule. A second ultra short laser pulse, shifted in time with respect to the first one, detects the evolution of the wave packet. Recent extension to the attosecond range (1as = 10-18 s) 13 Excitation with modulated light The equation of evolution of 12 for an excitation modulated at frequency d 12 / dt = W0 exp(it) i 12 12 12 has a solution oscillating at frequency : W0 12 = exp(it) + i 12 The intensity of the fluorescence light contains a component modulated at frequency , which exhibits resonant variations when the frequency of the excitation is scanned around 12 in an interval of width . ( ) First observation of this effect A. Corney, G. Series, Proc. Phys. Soc., 83, 207 (1964). 14 Outline of lecture 1 1 – Level crossing resonances in excited states 2 – Quantum beats. Time resolved spectroscopy 3 – Extension to ground states 4 – Ramsey fringes and microwave atomic clocks 5 – Dark resonances. Coherent population trapping 15 Extension to atomic ground states Optical pumping allows one to polarize atoms by accumulating them in a given Zeeman sublevel of the ground state g. One can also prepare atoms in linear superpositions of Zeeman sublevels of g if the angular momentum transferred from the pumping beam to the atoms is perpendicular to the static magnetic field. Transverse optical pumping Transverse physical quantities have a non zero average value only if the density matrix g has non zero off diagonal elements Equations of evolution can be established for the ground state density matrix g that are quite similar to those for e The spontaneous damping rate e in e has to be replaced by the relaxation rate g in g which is much weaker 16 Level crossing resonances in g Level crossing resonances can be very narrow because g is very small. They can be used to detect very small magnetic fields L is on the order of 1 MHz / Gauss. If g is on the order of 1 s-1, the width B0 of the resonance, given by L g is on the order of 10-6 Gauss. Magnetometer with a sensitivity of 510-10 Gauss J. Dupont-Roc, S. Haroche, C. Cohen-Tannoudji, Phys. Lett. 28A, 638 (1969) 17 Outline of lecture 1 1 – Level crossing resonances in excited states 2 – Quantum beats. Time resolved spectroscopy 3 – Extension to ground states 4 – Ramsey fringes and microwave atomic clocks 5 – Dark resonances. Coherent population trapping 18 Ramsey fringes Atomic beam velocity v L Two-level atoms g1, g2 with Eg2 Eg1 = A cross 2 cavities fed by the same coherent field with frequency 0 . The transition probability P g1 g2 is measured versus 0 If a single cavity is used, one gets a resonance with a frequency width 1/, where = / v is the time of flight through a single cavity. Time-frequency uncertainty relation If two cavities are used, interference fringes appear inside this resonance with a spacing proportional to 1/T, where = L / v is the time of flight between the 2 cavities. Ramsey fringes. Analogy with Young’s two-slit interference fringes, with a spacing determined by the distance between the 2 slits, appearing inside a diffraction profile whose width is determined by the width of each slit ( ) 19 P ( g1 g2 ) 2/T A 0 0 1 / Interference between 2 transition amplitudes For going from g1 to g2, the atom can follow 2 paths: - Interaction with the field in the first cavity - Interaction with the field in the second cavity g2 g1 t T 20 Cesium atomic clocks Principle The microwave oscillator is locked to the frequency of the central Ramsey fringe Orders of magnitude The width of the central Ramsey fringe is on the order of 1 / 2T ~ v / 2L. If L=0.5 m, v=100 m/s, one gets 100Hz How to go farther? Instead of increasing L for diminishing v/L, one can try to diminish v by using ultracold atoms. 21 Improving atomic clocks with ultracold atoms Fountains of ultracold atoms Cloud of atoms cooled by laser cooling to temperatures on the order of 1 μK Throwing this cloud of ultracold atoms upwards with a laser pulse to have them crossing the same cavity twice, once in the way up, once in the way down, and obtaining in this way 2 coherent interactions separated by a time interval T H H = 30 cm T = 0.5 s The width of the Ramsey fringes is 100 times smaller than the width obtained with thermal atoms 22 Examples of atomic fountains - Sodium fountains : - Cesium fountains : Stanford S. Chu BNM/SYRTE C. Salomon, A. Clairon Stability : 1.6 x 10-16 for an integration time 5 x 104 s Relative accuracy : 3 x 10-16 A relative accuracy of 10-16 corresponds to an error smaller than 1 second in 300 millions years! 23 From terrestrial clocks to space clocks •Time reference and global clock comparison •Validation of space clocks •Fundamental tests (General relativity, Variation of fundamental constants) ACES project (ESA, CNES) 24 Gravitational shift of the frequency of a clock An observer at an altitude z receives the signal of a clock located at the altitude z+z and measures a frequency A(z +z) different from the frequency, A(z), of his own clock 2 clocks at altitudes differing by 1 meter have apparent frequencies which differ in relative value by 10-16. A space clock at an altitude of 400 kms differs from an earth clock by 4 x 10-11 . Possibility to check this effect with a precision 70 times better than all previous tests with rockets Another possible application : determination of the “geoid”, surface where the gravitational potential has a given value 25 Optical clocks 26 Outline of lecture 1 1 – Level crossing resonances in excited states 2 – Quantum beats. Time resolved spectroscopy 3 – Extension to ground states 4 – Ramsey fringes and microwave atomic clocks 5 – Dark resonances. Coherent population trapping 27 Discovery of dark resonances Optically pumped sodium vapor put in a gradient of magnetic field parallel to the z-axis. The splitting between 2 Zeeman sublevels g1 et g2 depend on z g1 h h z0 h z g1 An applied RF field with frequency can induce resonant transitions between the 2 sublevels only at the point z0 where the splitting between the 2 sublevels is equal to h Modification of the populations of g1 and g2 in z0 which results in a change of the light intensity emitted by the atoms of the beam in z0 Analogy with Magnetic Resonance Imaging (MRI) Spatially resolved magnetic resonance 28 Bright resonances and “dark” resonances Bright resonance: appears at the point z0 where the splitting between g1 and g2 is equal to h 1 2 g2 g1 Dark resonance: appears also in the absence of RF, but only if the laser contains at least 2 modes with frequencies 1 and 2. The dark resonance appears at the point z'0 where the splitting between g1 and g2 is equal to (1-2) Raman resonance condition Eg2 Eg1 = ( 1 2 ) G. Alzetta, A. Gozzini, L. Moi, G. Orriols, Il Nuovo Cimento, 36B, 5 (1976) 29 Basic physical effect 1- We first consider the situation at time t=0. The atom is put in a linear superposition of g1 and g2 such that the 2 absorption amplitudes g1e and g2e interfere destructively ci : Amplitude for the atom to be in state gi (i=1,2) i (Rabi frequencies): Amplitudes for the atom to absorb a photon i from the state gi (i=1,2). D : atomic dipole moment The state c1 g1 + c2 g 2 is called "dark state" The atom is put in a linear superposition of states which cannot absorb light because of destructive interference Phenomenon called “Coherent Population Trapping” (CPT) 30 Basic physical effect (continued) 2- If a state is dark at t=0, can it remain dark at a later time t? The coefficients ci acquire phase factors exp(-iEit/) due to the energies Ei of the states gi The laser fields Ei acquire phase factors exp(-iit) due to their frequencies i The total absorption amplitude thus becomes: It still vanishes, as in t=0, if and only if the 2 phase factors multiplying c11 and c22 are the same, i.e. if: One recovers the Raman resonance condition and one understands why the dark resonance only appears when this condition is fulfilled. If it is not fulfilled, a state which is dark at a certain time t=o will no longer be dark at a later time, and it will be then able to absorb light 31 Variations of the fluorescence rate RF with the detuning from the unperturbed Raman resonance One varies the splitting between g1 and g2, 1 and 2 being fixed. Or one sweeps 2, 1 being fixed The dark resonance has a width ’ determined by the relaxation time in the ground state, much smaller than the width determined by the lifetime of the excited state It is their very small width which explains the interest of dark resonances for applications Example of application: « Electromagnetically Induced Transparency (EIT) » An atomic vapor with a great optical depth for a laser 1 exciting the transition g1e becomes transparent for this laser if one adds a second laser 2 exciting the transition g2e with a frequency fulfilling the Raman resonance condition. The index of refraction for the laser 1 varies also very rapidly 32 in the neighborhood of the dark resonance slow light Subrecoil laser cooling by Velocity Selective CPT R(v) 0 v 0 v - Because of the Doppler effect the fluorescence rate R is v-dependent and can be adjusted to vanish for v=0. Atoms with zero are in dark states and thus protected from the « bad effects » of light (random recoils due to the spontaneous emission processes). - Atoms with non zero velocity are no longer dark because the Doppler shift changes. They absorb light and the velocity changes due to the the random recoils following spontaneous emission can make them falling in the region near v=0 where they remain trapped and pile up - The longer the interaction time , the narrower the interval v in which the atoms can remain trapped during this time. One can have p = m v < k (subrecoil cooling) A. Aspect, R. Kaiser, N. Vansteenkiste, E. Arimondo, C. Cohen-Tannoudji PRL. 61, 826 (1988) Cooling mechanism leading to temperatures in the nK range 33 Quantum Monte-Carlo simulation of 1D-VSCPT Calculation by the dressed atom approach of the distribution of the time intervals between 2 successive spontaneous emissions of photons by the atom Between 2 emissions, the momentum quantum number remains constant and changes in a random way after each emission F. Bardou, J-P. Bouchaud,O. Emile, A.Aspect,C. Cohen-Tannoudji, PRL. 72, 203 (1994) Anomalous random walk along the time axis dominated by a few rare events where p remains close to zero. Self-similarity at all scales Analogy with other situations involving ‘Lévy flights” 34 35 Stimulated Raman Adiabatic Passage (STIRAP) Klaas Bergmann e 2 1 g2 g1 Dark state D = c1 g1 + c2 g2 c11 + c22 = 0 i : Rabi frequencies c2 c1 = 2 1 1 2 The dark state coincides with g2 2 1 The dark state coincides with g1 By starting with 1 2 , by reducing adiabatically 1 while increasing adiabatically 2 until 2 becomes much larger than 1 , atoms are selectively transferred adiabatically from g2 to g1 Anti-intuitive order The system always remains in a dark state, so that e is never populated (no spontaneous transitions from e). Selective transfer of molecules from one state to another 36 Conclusion Atomic physics experiments provide interesting examples of physical effects demonstrating the importance of linear superpositions of states These effects discovered several decades ago are revisited and are playing now an important role in modern developments (nonlinear optics, laser cooling, molecular physics, atomic fountains,…) Atomic clocks with ultracold atoms are now used in all metrological institutes. They have reached an impressive relative accuracy (10-17) allowing them to perform very precise tests of basic theories (general relativity, variation of fundamental constants,…) Their very high sensitivity to the gravitational field clearly shows that a universal time reference should now be delivered, not by clocks on earth, but by clocks in space 37