Atomic clocks with cold atoms
Transcription
Atomic clocks with cold atoms
Atomic Atomic clocks clocks with with cold cold atoms atoms Pierre Lemonde Bureau National de Métrologie – SYRTE (UMR CNRS 8630) Observatoire de Paris, France LASER COOLING and APPLICATIONS September 2004 Les Houches, France Accuracy Accuracy of of atomic atomic clocks clocks SYRTE Why Why atomic atomic clocks clocks ?? • Metrology – – • Fundamental physics – – – • Measurements of fundamental constants Test QED Test equivalence principle… High Tech – – • Time scales Most of the units in turn rely on the SI second… Navigation Telecom networks Atomic physics – – – Spectroscopy Cold collisions Funding… Definition linked to SI seconds Practical realisation with atomic clocks Attempts to redefine Overview Overview • Introduction – Principle of operation of atomic clocks • Basics of signal analysis and metrology – – – – • Phase/frequency Different types of noise Stability Accuracy Atomic fountains – Principle of operation – Lineshape computation – Sources of noise in a fountain/stability – Accuracy overview, collisions • Next generation of atomic clocks – Space projects – Optical clocks • Example of applications – Atomic Atomic clocks clocks basics basics Frequency of an atomic transition Atomic frequencies are universal and stable (equivalence principle) as opposed to macroscopic oscillators (quartz cristal, pendulum, earth rotation...) Idea of a "perfect" frequency in practice Pure AM Time Pure PM s(t) s(t) s(t) AM+PM Time Time Signal Signal analysis analysis Instantaneous frequency Frequency stability: "magnitude" of relative frequency fluctuations Frequency Stability is characterized with the Allan variance typical frequency fluctuations averaged over with , converges for most of the types of noise met experimentally Experimentally White White frequency frequency noise noise 3 0 - 3 3 0 - 3 3 0 - 3 3 0 - 3 Flicker Flicker frequency frequency noise noise 2 0 - 2 2 0 - 2 2 0 - 2 2 0 - 2 Frequency Frequency accuracy accuracy The signal average frequency differs from the atomic frequency is the sum of all possible frequency shifts (Zeeman, Stark, Collisions, Doppler...) which are evaluated from frequency measurements Accuracy: uncertainty on Accuracy and stability are strongly linked Noise of the measurements (stability) ultimately determines the accuracy e.g. 10-15 is reached after 104 seconds (3 hours) 10-16 after 106 seconds (10 days) An accuracy evaluation below 10-16 is impossible Conversely, a good control of the frequency shifts is necessary to avoid long term degradation of the frequency stability (flicker floor, frequency drift) Tjoelker et al. 1996 Atomic Atomic clock clock principle principle atomic resonance macroscopic oscillator 1 correction atoms interrogation 0 atomic quality factor -as high as possible (Cs: 10 GHz, Hg+: 1 PHz) + transition should be insensitive to external perturbations -low natural width (Cs: 10-13 Hz, Hg+: 2 Hz) -Fourier limit, long interaction time (Cs: 1 Hz, Hg+: 6 Hz) -low oscillator spectral width (Cs: 10-5 Hz, Hg+: 0.1 Hz) -Large atom number (Cs: 107, Hg+: 1) -low noise detection scheme -low noise oscillator Cs fountain (SYRTE): 10-14 τ -1/2, accuracy 7 10-16 Optical Hg+ (NIST): 4 10-15 τ -1/2, accuracy 10-14 Atomic Atomic Fountains Fountains 10 fountains in operation (SYRTE, PTB, NIST, USNO, PENN state, ON, IEN, NPL) with an accuracy of ~10-15. Several projects (NIJM, NIM, KRIISS, VNIIFTRI...) See e.g. Proc. 6th Symp. Freq. Standards and Metrology (World Scientific 2002) BNM-SYRTE (F) PTB (D) NIST (USA) Energy Energy levels levels Cs Cs 133Cs 133Cs hyperfine splitting is the basis for the definition of the SI second. Atomic Atomic fountains: fountains: Principle Principle of of operation operation Nat ~2×109 σr ~1.5−3mm T ~1µK ∆V ~2 cm.s-1 4m.s-1 Vlaunch ~ H ~1m T ~500ms Tc ~0.8-2s Selection 3 2 1 Detection BNM -SYRTE fountain BNM-SYRTE fountain ensemble ensemble Dual Dual atomic atomic fountain fountain Rb+Cs Rb+Cs • Transverse collimation of an atomic beam + Chirp cooling î 109 atoms loaded in 200 ms in optical molasses Operating parameters • • • • • • • Beam collimation Nat ~ 109 σ ~ 3 mm T ~ 1 µK v ~ 4 m/s H~1m 100 ≤ Tload ≤ 500 ms 1.1 ≤ Tcycle ≤ 1.5 s AA key key technique: technique: The The moving moving molasses molasses Due to the first order Doppler effect, the frequency of the upper and lower laser beam is the same in the frame moving upwards at For Cs: Measurement Measurement of of the the transition transition probability probability 7 0 0 e s ta te f s ta te 6 0 0 a r b itr a r y u n its 5 0 0 J b/2 J 4 0 0 J b/2 s 3 0 0 2 0 0 1 0 0 0 0 2 0 4 0 tim e ( m s ) 6 0 8 0 1 0 0 The area Ae and Af of the time of flight signals in calculated. The transition probability is given by Response of the detection: area per atom Technical noise ~ 400 atoms time spent in laser beam (s) gain amp. photodiode collection (V.A-1) response (A.W-1) efficiency radiated power (W) vacuum vacuum chamber chamber and and cavity cavity The 2 outermost shields are removed Interrogation region with magnetic and thermal shields Compensation coils Collimator for molasses beams Optical molasses optical optical bench bench Laser diode based system, can be made compact and reliable Acousto-optic modulator Optical fibers Cs vapor cell Injection locked diode laser External cavity diode laser Frequency Frequency synthesis synthesis Typical requirements: - low phase noise, phase coherence with the reference signal - fine PC-controlled frequency tuning, PC-controlled amplitude (P~ -60dBm) - give access to « Zeeman » transitions - reduced microwave leakage The power spectral density of the fractional frequency fluctuations of the synthesized signal is written lineshape lineshape calculation calculation Initial hypothesis: - external motion is described by a classical trajectory r(t) - the two clock levels are spectrally resolved => 2 level atom - any process causing relaxation is neglected Hamiltonian: (magnetic dipole interaction, gI, ge-2 neglected) (purely stationary field) We neglect non-resonant terms (rotating wave approximation) We then rewrite the Hamiltonian in a new representation Atomic Atomic evolution evolution using using the the Bloch Bloch vector vector Hamiltonian in the new representation detuning Atomic observables are also transformed to the same representation The Hamiltonian can be written as Pauli matrices We define the Bloch vector (or fictitious spin) as Equation of evolution for the Bloch vector We used Heisenberg’s equations for sigma Atomic observables and Rabi Rabi oscillations oscillations The Bloch vector evolves according to The motion is an instantaneous rotation around Example: Rabi oscillation on resonance (δ=0) π/2 pulses: Final state 3π/2 pulses: Ramsey Ramsey interrogation interrogation Time 1st interaction free flight 2nd interaction The final state depends mostly on the accumulated phase during the free flight between the microwave field (ω) and oscillating atomic coherence (ωef): As long as δ<<Ω0: Ramsey fringes One big advantage: most of the time, atoms evolve without being coupled to the exciting field Ramsey Ramsey fringes fringes in in atomic atomic fountain fountain 1.0 1.0 0.8 transition probability P 0.6 0.4 0.8 0.94 Hz 0.2 0.0 -1.0 -0.5 0.0 0.5 1.0 0.6 0.4 NO AVERAGING ONE POINT = ONE MEASUREMENT OF P 0.2 0.0 -100 -50 0 50 100 detuning (Hz) We alternate measurements on bothe sides of the central fringe to generate an error signal, which is used to servo-control the microwave source Fluctuations of the transition probability: Sensitivity Sensitivity function function Goal: to calculate the effect of temporal frequency fluctuations of the interrogation oscillator (to first order) Definition of the sensitivity function It can be computed (and measured) by looking at the effect of a phase step during the interaction The sensitivity function can be used (with care) to calculate the effect of a perturbation of the atomic frequency The sensitivity function depends on the interaction scheme. It gives simple way to estimate frequency shifts or the effect of the noise of the interrogation even for complex cases (time dependent frequency shifts, non-square pulses...). Important remark: In true life, the sensitivity function is not exactly the same for all atomic trajectories. In some cases, this must be accounted for. Shape Shape of of the the sensitivity sensitivity function function For a single centered trajectory and in the limit δ<<Ω0, this is possible to derive an analytical expression. For an optimized Ramsey interrogation, we have: Sensitivity function in atomic fountains for two different field amplitudes Ω0 In a fountain : TE011 mode The The sensitivity sensitivity function function and and frequency frequency shifts shifts The equilibrium condition of the loop is developed to first order using g(t) The fractional frequency shift is then given by Slightly modified if we account for actual individual atomic trajectories Frequency Frequency noise noise of of the the microwave microwave source source Equation of the servo loop: Sensitivity function: Slope of Ramsey fringes How the frequency fluctuations of the source are sampled and averaged: Fractional frequency instability (for N>>1) G. Dick, in Proc. PTTI, Redondo Beach, 1987, pp. 133–147. G. Santarelli et al., IEEE Trans. UFFC 45, 887 (1998). =>Limitation at the level of σy(τ)~10-13×τ -1/2 when microwave synthesis is based on a very good quartz oscillator. Independent on the atom number. Frequency -maser Frequency stability: stability: Fountain Fountain vs vs H H-maser Rb fountain vs. H-maser fractional frequency instability Limiting term: phase noise of the quartz oscillator integration time τ(s) maser autotuning Typically, when using a very good quartz oscillator: Frequency Frequency stability: stability: Fountain Fountain vs vs Fountain Fountain « Loose synchronization » (within a few seconds to a few minutes) Cycle by cycle synchronization with matched sensitivity functions: cancellation of the high frequency noise of the interrogation oscillator Cryogenic Cryogenic oscillator oscillator Sapphire cryogenic oscillator from the University of Western Australia High quality factor sapphire resonator (Q ~ 4×109) at 12 GHz Turning point of temperature sensibility: dν/dT = 0 near T=6K SCO has extremely good short term stability (measured at UWA against a second SCO) SCO signal is converted to 9.2 GHz A. Luiten, M. Tobar et al. Quantum Quantum projection projection noise noise For a single atom: - transition probability P: - Variance of quantum fluctuations of P: For an ensemble of Ndet uncorrelated atoms: Itano et al. PRA 47, 3554 (1993) Spin squeezing: Itano, Polzik, Mölmer… Contribution of the quantum projection noise to the frequency instability: Contribution of the photon shot noise (an other quantum noise): nph : number of detected photons per atom Practically, nph ~ 100 and this contribution is a small (negligible) fraction of the quantum projection noise Quantum Quantum projection projection noise noise -2 σy(τ) Qatπ(τ/Tc) Quantum Limited Operation of a Cs Fountain up to Nat∼ 6 105 1/2 10 0.91 N -1/2 at -3 10 4 10 5 10 Nat For Nat∼ 6 105 atoms, the frequency stability is σy(τ) ~ 4 10-14 τ-1/2 G.Santarelli et al. PRL,82,4619 (1999) 6 10 Frequency Frequency stability stability with with aa cryogenic cryogenic Oscillator Oscillator With a cryogenic sapphire oscillator, low noise microwave synthesis (~ 3×10-15 @ 1s) FO2 frequency stability This stability is close to the quantum limit. A resolution of 10-16 is obtained after 6 hours of integration. With Cs the frequency shift is then close to 10-13! Frequency Frequency comparisons comparisons between between fountains fountains 1E-14 -14 stabilité de fréquence 4.13 10 -14 2.83 10 1E-15 FO1 FO2 Difference -14 5.01 10 1E-16 100 1000 10000 temps (s) Fountain Fountain Accuracy Accuracy Fountain (BNM-SYRTE) Effect FO2(Cs) FO2(Rb) FO1 Shift and uncertainty (10-16) second order Zeeman 1927.3(.3) 3207.0(4.7) 1199.7(4.5) -168.2(2.5) -127.0(2.1) -162.8(2.5) -357.5(2) 0.0(1.0) -197.9(2.4) Residual Doppler effect 0.0(3.0) 0.0(3.0) 0.0(3.0) Recoil 0.0(1.4) 0.0(1.4) 0.0(1.4) Neighbouring transitions. 0.0(1.0) 0.0(1.0) 0.0(1.0) -4.3(3.3) 0.0(2.0) -3.3(3.3) 0.0(1.0) 0.0(1.0) 0.0(1.0) 6.5 7 7.5 Blackbody radiation Collisions + cavity pulling Microwave leaks, spectral purity, synchronous perturbations. Collisions with residual gaz. Total Frequency difference between FO1 and FO2: 3 10-16 Cold Cold collisions: collisions: orders orders of of magnitude magnitude Inter-atomic potential curves (87Rb) 1000 3 -long range: Van Der Waals interaction Typical inter-atomic distance: Typical De Broglie wavelength: 0 potential energy (K) -size of the « molecular » region: triplet state Σu -1000 1 singlet state Σg -2000 0.2 2+2 0.0 -0.2 -3000 1+2 -0.4 -4000 1+1 -0.6 -0.8 -5000 -1.0 1.5 2.0 2.5 3.0 3.5 4.0 4.5 5.0 5.5 -6000 0.4 0.6 0.8 1.0 inter-nuclear distance (nm) 1.2 In general, collisions tend to be dominated by s-waves: This is the case for 87Rb at 1µK. Collisions are then characterized by a single parameter for each atomic state, the scattering length in the s-wave channel: 133Cs is more complicated. At 1µK, d-waves must be taken into account due to low energy molecular resonances (Feshbach resonances). Collisional properties become independent on temperature only below 0.1nK Typical phase space density: far from quantum degeneracy Mean -field energy Mean-field energy and and collisional collisional shift shift Total mean-field interaction energy as a function of scattering length aff, atomic density n, atom number Nat and atomic mass m: Energy conservation before/after the interaction (with only the clock states populated and assuming 100% transfer efficiency) Resulting clock shift: In general (other states populated), the instantaneous frequency shift of the atomic resonance is given by: In the fountain, the time variation of the atomic density must be taken into account with the sensitivity function Collisional Collisional shift shift :: 87Rb 87Rb vs vs 133Cs 133Cs Differential measurements (interrogation oscillator H-maser) SYRTE In a MOT Cavity pulling is taken into account and subtracted YALE Th. Atomic density changed by changing the trapping light intensity (40% uncertainty) The shift in 87Rb is much (~50 to 100 times) smaller than in 133Cs SYRTE Y. Sortais et al. , PRL, 85, 3117 (2000) Th.1 = -11.7×10-23/ (at.cm-3) (S. Kokkelmans et. al., PRA 56, R4389 (1997)) Th.2 = -7.2×10-23/ (at.cm-3) (C.Williams et al.) YALE -5.6 ( ± 3.3)×10-23/ (at.cm-3); (C.Fertig and K.Gibble, PRL, 85, 1622 (2000)) Pushing 5 6 Detuning (kHz) Rabi Frequency (kHz) Collisional Collisional shift shift measurement measurement 4 2 0 -5 0 100% 0 1 2 3 Time (ms) 4 0 1 2 3 Time (ms) 4 50% Sweeping Launching By performing the internal state selection with adiabatic passage, we vary the atomic density by a factor of 2 without changing velocity and position distribution |4,n-1> |+> |3,n> |3,n> |-> |4,n-1> ¾Cold collisions then only depend on the atomic number To measure the cold collision shift in quasi real time ¾ We alternate measurements with full or interrupted adiabatic passage (produces n or n/2) F. Pereira Dos Santos et al., PRL 89,233004 (2002) δ The The “adiabatic “adiabatic passage passage method”: method”: Experiments Experiments The value and the stability of the ratio between 50% and 100% configurations is monitored during each measurement. We find: ME A S UR ED We have a practical realization of two atomic samples with a density ratio precisely equal to 1/2 Extrapolation of the collisional shift: Adiabatic Adiabatic passage passage method method limitation limitation One of the possible limitation of the adiabatic passage method: off-resonant optical pumping due to the pushing beam Measured atom number ratios with adiabatic passage The effect of spurious mF states is studied by populating them purposely and selectively With adiabatic passage and differential measurement, the measured quantity is the ratio between contributions of mF=0 states and the other mF state ⇒the atomic density cancels out ⇒possibility of precise comparison with theory Effect 0 states Effect of of the the m mFF≠≠0 states Differential method with 3 different configurations (period 60 cycles): 1. Full density on (0-0) 2. half density on (0-0) 3. Full density on (0-0) and on (mF - mF), (additional synthesizer for m F ≠ 0) Ratio between the shift per atom due to the 0 states (ν00) and to the mF state (νmFmF) The contribution of m F ≠ 0 states are at most 1/3 of the contribution of the clock states In the usual clock configuration: 3×10-3 residual populations in mF states contributes to less than 1×10-3 ¾The cold collisional shift can be controlled at 10-3 of its value Clock shifts due to |mF| = 3 are not equal … Feshbach Feshbach resonances resonances at at low low magnetic magnetic field field (Cs) (Cs) Ratio of frequency shift due to |mF| = 1; 2; 3 over clock states frequency shift plotted as functions of the magnetic field. Observation of the amplitude (all mF) and the width (|mF| = 3) of Feshbach resonances. Calibration of the relative contribution of the remaining mF ≠ 0 atoms on the clock shift with respect to the B field H. Marion et al. to be published Black Black body body radiation radiation shift shift Spectral density of blackbody radiation Cs D1 and D2 lines 894 and 852 nm Peak:1.7×1013 Hz (λ~17µm) E. Simon et al. PRA 1997 Resulting frequency shift: most of the effect is the AC Stark shift Sensitivity to temperature fluctuations (Cs): -2.3×10-16 K-1 Magnetic Magnetic field field A static B field is applied on purpose to spectrally resolve de mF=0 to mF=0 transition: (Earth field ~300mG) sensitivity to field fluctuations: 9.3 10-16.nT-1 The B field is measured and made homogeneous using the mF=+1 to mF=+1 transition Zero crossings must be avoided along the cloud trajectory to prevent Majorana transitions Systematic Systematic effects/evaluation effects/evaluation methods methods Cold collisions + cavity pulling -real-time measurement and extrapolation with adiabatic passage method Black body radiation -static polarizability, calculations, stabilization and measurement of T Second order Zeeman effect -proper shielding and homogeneity, spectroscopy of the “Zeeman” transitions Microwave leaks -careful design, characterization of synthesizers, π/2-3π/2-… Microwave spectrum (spurious side bands, synchronous phase modulation,…) -careful design and characterization of synthesizers, π/2-3π/2… measurements, change timing and synchronization Residual first Doppler effect (due to phase gradients in the Ramsey cavity) -careful design of the cavity, sym.-assym., π/2-3π/2-…, change clock tilt angle Ramsey pulling, Rabi pulling, Majorana transitions -careful design and characterization of the B field, calculations Background gas collisions -earlier measurements Recoil effect -calculations Second order Doppler effect -order of magnitude => negligible PHARAO: PHARAO: aa Transportable Transportable Fountain Fountain Measurement of 1S-2S transition of Hydrogen at Max Planck Institut für Quantenoptik in Garching cryostat atomic hydrogen chopper Faraday cage 2S detector vacuum chamber x 2 243 nm time resolved photon counting dye laser f dye x4/7 486 nm ν1S-2S = 2 466 061 413 187 103 (46) Hz Accuracy : 1.8 10-14 M. Niering et al, PRL 845, 5496 (2000) x1/2 4/7 x f dye 1/2 x f dye microwave interaction I λ 70 fs Ti:sapphire mode locked laser 9.2 GHz cold atom source detection Measurement of the Ry, test of QED, fundamental constants stability. Long Long distance distance comparison comparison between between PTB PTB and and NIST NIST Cesium Cesium Fountains Fountains Frequency Comparison NIST F1 - CSF1 (period of overlap, date of measurement) PTB: A. Bauch, S. Weyers NIST: S. Jefferts BIPM circular T data base of clock comparisons using GPS or TWSTFT (15 days, August 2000) 2 0 -2 10 15 x y(F1 - CSF1) 4 -4 (20 days, November 2001) (10 days, July 2001) -6 0 1 2 3 Number of Measurement 4 Atomic Atomic fountains fountains:: summary summary Microwave frequencies • Cs 9.192 631 770 GHz • 87Rb 6.834 682 610… GHz Magneto-optical trap or molasses. 108 atomes, T ~1µK Resonance width ~1Hz Frequency stability: 1 10-14 τ -1/2 Frequency accuracy : 7 10 -16 Ultimate accuracy~10-16 Can we go further ? Two Two possible possible ways ways atomic resonance macroscopic oscillator 1 correction atoms interrogation 0 atomic quality factor -as high as possible -low natural width -Fourier limit, long interaction time -low oscillator spectral width -Large atom number -low noise detection scheme -low noise oscillator + transition should be insensitive to external perturbations Atomic transition in the optical domain A clock in space Optical Optical frequency frequency standards standards ?? Frequency stability : Increase (x 105) Optical fountain at the quantum limit !!!!!!!!! Frequency accuracy: most of the shifts (expressed in absolute values) don't depend on the frequency of the transition (Collisions, Zeeman...). -Ability to compare frequencies (no fast enough electronics ) Three major difficulties -Recoil and first order Doppler effect -Interrogation oscillator noise conversion (Dick effect). The best optical clocks so far exhibit frequency stabilities in the 10-15 τ -1/2 range together with an accuracy around 10-14. Optical Optical frequency frequency measurements measurements No electronics is fast enough to measure the phase of signals @ frequencies > ~100 GHz Harmonic frequency chains: -A set (about 13) of non linear stages, each of them performing a basic operation (frequency multiplication by 2 or3, addition, difference). -Uncomfortable regions of the spectrum (THz, MIR): alcohol lasers… -1 apparatus for one particular transition (to within a few 10's GHz). -very heavy and complex systems (need for secondary standards). divide by 3 system Only a few systems have been fully operated (JILA, PTB, SYRTE, NRC). Only one achieved phase coherent comparison visible-RF Schnatz H. et al. PRL 76 18 (1996) Femto -second frequency Femto-second frequency chain chain • temporal domain E(t) ∆φ 2∆φ t τr.t = 1/fr • frequency domain I(f) x2 x f 0 All optical frequencies of the comb are known in terms of RF frequencies J. Reichert et al. PRL 84, 3232 (2000), S. Diddams et al. PRL 84,5102 (2000) Femtosecond Femtosecond Laser Laser Kerr effect mode locked Ti-Sa laser (25fs) 450 mW output Spectral broadening using a photonic crystal fiber (up to 270 mw output) Self referenced frequency comb 40µm Locking Locking scheme scheme 40 MHz Cryo or H Maser RF Synth Synth. Repetition rate phase locked to H maser or Cryo 9 GHz + 200 MHz or 9.19 GHz Rep. lock 11. har. Offset frequency detected, not locked Output to OFS fs laser 840 MHz PCF measurements KTP Off. freq. Noise of the frequency comparisons (optical-optical or optical-microwave) ~ 10-15t-1/2 Accuracy of frequency ratios ~ 10-19 Ma et al. Science 303, 1843 (2004), Telle et al. PRL 2002 Bauch and Telle, Rep. Prog. Phys. 65, 789, 2002 and references therein Recoil Recoil effect effect Overlap of the wave packets after 1s of free flight would imply temperatures ~ 1 fK Ramsey-Bordé interferometer Experimental realisation: PTB, NIST (Ca atoms) C. Bordé et al. PRA 30 1836 (1984) G. Wilpers et al., PRL 89 230801 (2002) C. W. Oates et al. Opt. Lett. 25, 1603 (2000). Ca Ca optical optical clock clock First order Doppler effect (wavefront curvature, beam misalignement). Ca Vs Maser Ca Vs cavity Ca Vs Hg+ Dick effect (very low duty cycle) Trapped -Dicke regime) Trapped particles particles (Lamb (Lamb-Dicke regime) classical picture To first order, no effect of the atomic motion quantum picture Momentum conservation if the atom is confined to well below λ, is a broad function of p The atomic transition is not shifted or broadened (Recoil, Doppler) Very detailed calculations in Wineland, Itano PRA 20, 1521 (1979) For atoms, however, conservative traps require large trapping fields inducing large shifts of the levels ions can be trapped with much lower fields, but with only a few ions in the trap for a clock Single Single ion ion clock clock Hg+, NIST (Bergquist et al.) Other experiments: Yb+, PTB (Tamm, Peik...) NPL : Yb+, Sr+, NRC : Sr+, MPQ : In+… NIST NIST Hg+ Hg+ Clock Clock R. Rafac, B. Young, J. Beall, W. Itano, D. Wineland and J. Bergquist, PRL 85, 2462 (2000) Width 40 Hz 10 Hz Quality factor: Q = ν/∆ν=1.6 Highest Q ever achieved Current accuracy: 10-14 20 Hz 6 Hz 1014 ++ Clock accuracy NIST Hg NIST Hg Clock accuracy Effect Second order Zeeman effect @ B=2.7 G Black Body radiation shift @ T=300K Black Body radiation shift @ T=4K Second order Doppler secular motion Second order Doppler micromotion 4 Background collisions ( He) Quadrupole shift -2 @ ∇E=10 V.mm Correction Uncertainty 2.6 +1 386 +0.079 <0.08 0 0 <0.003 0.003 <0.1 0.1 0 0 <1 10 Quadratic sum 10 Hz At PTB sub Hz comparison of Yb+ single ion clocks (Tamm et al. Proc. ICOLS 2003, arXiv 0403120) Optical Optical clock clock with with trapped trapped atoms atoms • Trap ions: – Accuracy. Régime de Lamb-Dicke, Effects of traooing field – Stability limited by Nat : one or a few ions – Problem of the ultra-stable laser • Free atoms: – Stability Nat~106, fast response time – Accuracy limited by atomic motion: Doppler effect • Trapped atoms: – Combine the advantages of both methods – Trapping the atoms implies strong field ? – Maintain coherence ? AA future future optical optical standard standard with with trapped trapped Atoms Atoms 3S 1P 1 461 nm λtrap 1S 0 1 688 nm λtrap 679 nm 689 nm 698 nm (87Sr: 1 mHz) 3P 1 0 Combine advantages of single trapped ion and Free fall neutral atoms optical standards Katori, Proc. 6th Symp. Freq. Standards and Metrology (2002) Pal’chikov, Domnin and Novoselov J. Opt. B. 5 (2003) S131 Katori et al. PRL 91, 173005 (2003) Clock transition 1S0-3P0 transition (Γ =1mHz) 11S -33P transition Sr Sr S00- P00 transition MOT fluorescence (%) Free Falling atoms 100.0 99.8 ν1S0-3P0=429 228 004 235 (20) kHz 99.6 99.4 99.2 Courtillot et al., PRA 68, 030501 (2003). 99.0 -4 -3 -2 -1 0 1 2 3 4 698 nm laser detuning from resonance (MHz) Trapped atoms Takamoto et al. PRL 91, 223001 (2003) Magic wavelength measurement (813 nm) Very recently linewidth 50 Hz (Katori ICAP 2004) Other experiements (JILA, PTB, LENS, NIST…) Other atoms: Yb, Hg… Einstein Einstein Equivalence Equivalence Principle Principle and and the the stability stability of of fundamental fundamental constants constants In any free falling local reference frame, the result of a non gravitational measurement should not depend upon when it is performed and where it is performed. EEP ensures the universality of the definition of the second It implies the stability of fundamental constants: α=e2/hc, me, mp,… In particular: the ratio of the transition frequencies in different atoms and molecules should not vary with space and time The EEP can be tested by high resolution frequency measurements regardless of any theoretical assumption EEP revisited by modern theories: gµν ⇒ gµν,ϕ,… Fundamental constants depend upon local value of ϕ : α(ϕ), m(ϕ),… Violations of EEP are expected at some level !! For instance: T. Damour, G. Veneziano, PRL 2002 Does Does the the fine fine structure structure constant constant αα varies varies ?? Because of large relativistic corrections, the hyperfine energy of an alkali atom depends upon Z and α=e2/ħc Search method for α drift: Compare hyperfine energy of rubidium and cesium as function of time Present Present tests tests of of cosmological cosmological Variations Variations of of αα – Oklo test : geochemical analysis of the natural fossil fission reactor in Oklo (Gabon, 1.8×109 yr ago) : α now − α Oklo ≤ 1×10 −7 α& α ≤ 5 ×10−17 yr −1 Damour, Poliakov, Nucl. Phys. B 480, 37 (1996) – Absorption spectroscopy from quasars: ∆ α α = (− 0 . 72 ± 0 . 18 )×10 −5 ( 0 . 5< z < 3 . 5 ) J. Webb et al., PRL 87, 091301 (2001) Laboratory Laboratory tests tests versus versus cosmological cosmological tests tests • • • • • • • • A priori loss of factor 1010 in sensitivity !! ~ 1 year versus 1010 years But: ultra-stable and accurate clocks: 10-15 Æ10-16 -10-17 repeatable measurements independent checks in various labs choice of hyperfine, fine and optical transitions See S. Karshenboim, Can. J. Phys 78 639, (2000), J.P. Uzan Rev. Mod. Phys., 75, 403 (2002) Test Test of of Local Local Position Position Invariance Invariance Stability Stability of of fundamental fundamental constants constants (1) (1) [Following the work of Prestage et al., PRL 74, 3511 (1995)] Frequency of hyperfine transitions as a function of fundamental constants (at lowest order): atomic unit of frequency nuclear g-factor purely numerical factor electron to proton mass ratio relativistic « correction » factor, function of the fine structure constant α Frequency of electronic transitions as a function of fundamental constants (at lowest order): Ratio between atomic frequencies: Sensitivity to variation of fundamental constants: Test Test of of Local Local Position Position Invariance Invariance Stability Stability of of fundamental fundamental constants constants (2) (2) g(i) [Following the work of V.V. Flambaum, ArXiv:physics/0302015 (2003)] and mp are not “fundamental” constants but they can be linked (at least in principle) to 2 fundamental parameters: mass scale of QCD: quark mass: Any clock comparison can be seen as testing the stability of 3 fundamental parameters: The K(i) are sensitivity coefficients: hfs: elec: molecular vibration: With 4 well chosen atomic clocks, we constrain the stability of 3 independent frequency ratios => independent constraint to the variation of With more than 4 well chosen atomic clocks, redundancy is achieved Test Test of of Local Local Position Position Invariance Invariance Stability Stability of of fundamental fundamental constants constants (3) (3) Comparisons between 87Rb and 133Cs hyperfine frequencies in atomic fountains over 5 years: early measurement with a fractional uncertainty one data point on this graph corresponds to 1.3×10-14. Improvement by 104 at the time. ~2 months of measurements, with many checks on systematic shifts latest measurements with a fractional uncertainty 1.3×10-15: Stability of fundamental constants: Marion et al. PRL 90, 150801 (2003) Other recent comparison 199Hg+(elec) vs. 133Cs(hfs) at NIST: Bize et al. PRL 90, 150802 (2003) Test Test of of Local Local Position Position Invariance Invariance Stability Stability of of fundamental fundamental constants constants (4) (4) Other Measurements with comparable accuracy (H, Yb+) Bize et al. PRL 90, 150802 (2003) Fischer et al. arXiv:physics 0311128 and 0312086, PRL 2004 Peik et al., arXiv:physics 0402132 (2004) AA FEW FEW REFERENCES REFERENCES Vannier, Audoin, "the quantum physics of atomic frequency standards" Adam Hilger (1989) A. Bauch, H. Telle,"frequency standards and frequency measurements" Rep. Prog. Phys. 65, 789, (2002) S. Cundiff and J. Ye "femtosecond optical frequency combs", Rev. Mod. Phys. 75, 325 (2003) Proc. 6th Symp. Freq. Standards and Metrology, World scientific, (2002) www.bipm.fr www.nist.gov www.ptb.de www.obspm.fr ….