Observation of a Large Atomic Parity Violation Effect in Ytterbium

  • K. Tsigutkin, D. Dounas-Frazer, A. Family, J. E. Stalnaker, V. V. Yashchuk, and D. Budker, Department of Physics, University of California at Berkeley, Berkeley, California 94720-7300, USA, Advanced Light Source Division, Lawrence Berkeley National Laboratory, Berkeley California 94720, USA, and Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA
Phys. Rev. Lett. 103, 071601
Low-lying energy eigenstates of Yb and transitions relevant to the APV experiment.

Atomic parity violation (APV) experiments are a powerful tool in the study of electroweak interactions (see, for example, review [1]). The electroweak parameter of utmost importance in APV experiments is the weak charge QW, associated with the exchange of the Z0 boson between an atomic electron and the nucleus. The most accurate APV experiments were performed using Cs atomic beam and yielded a value of the QW for Cs with experimental and theoretical uncertainties of 0.35% [2] and 0.27% [3], respectively, providing a stringent test of the standard model (SM) at low momentum transfer ( MeV/c). However, it has not yet been possible to test an important prediction of the SM concerning the variation of QW along a chain of isotopes. It has been suggested [4] that rare-earth atoms may be good candidates for APV experiments because they have chains of stable isotopes, and the APV effects may be enhanced due to the proximity of opposite-parity levels. While the accuracy of atomic calculations is unlikely to ever approach that achieved for atoms with a single valence electron, ratios of PV amplitudes between different isotopes should provide ratios of weak charges, without involving, to first approximation, any atomic-structure calculations.

The present experiment is inspired by the prediction [5] supported by further theoretical work of [6,7], that the PV amplitude in the chosen transition is 100 times larger than that in Cs. The motivation for PV experiments in Yb is probing low-energy nuclear physics by comparing PV effects on either a chain of naturally occurring Yb isotopes, or in different hyperfine components for the same odd-neutron-number isotope. The ratio of PV amplitudes for two isotopes of the same element is sensitive to the neutron distributions within the nucleus [8]. The difference between PV amplitudes measured on two different hyperfine lines belonging to the same transition is a manifestation of nuclear-spin-dependent APV, which is sensitive to the nuclear anapole moments (see, for example, reviews [9,10]) that arise from weak interactions between the nucleons. As the precision of the experiment increases, a sensitive test of the standard model may also become possible [11].

Here we report on experimental verification of the predicted PV-amplitude enhancement in Yb using a measurement of the APV amplitude for Yb174.

Orientation of fields for PV-Stark interference experiment and schematic of the present APV apparatus. Not shown is the vacuum chamber containing all the depicted elements, except the photomultiplier (PMT) and the photodiode (PD). PBC-power buildup cavity. Light is applied collinearly with x.Orientation of fields for PV-Stark interference experiment and schematic of the present APV apparatus. Not shown is the vacuum chamber containing all the depicted elements, except the photomultiplier (PMT) and the photodiode (PD). PBC-power buildup c... Show more

The idea of the experiment is to excite the forbidden 408-nm transition (Fig. 1) with resonant laser light in the presence of a quasistatic electric field. The PV amplitude of this transition arises due to PV mixing of the 5d6sD13 and 6s6pP11 states. The purpose of the electric field is to provide a reference transition amplitude due to Stark mixing of the same states, interfering with the PV amplitude. In such interference method [12,13], one is measuring the part of the transition probability that is linear in both the reference Stark-induced amplitude and the PV amplitude. In addition to enhancing the PV-dependent signal, employing the Stark-PV-interference technique provides for all-important reversals allowing one to separate the PV effects from various systematics.

The configuration which is used for the Stark-interference experiment is shown in Fig. 2. The electric field E is applied collinearly with the propagation axis ( x) of the linearly polarized resonant light beam, while the magnetic field B is directed along z. The pseudoscalar quantity which manifests PV is

where E is the electric field of the light. The APV effect vanishes when the angle θ between the light polarization and the magnetic field approaches a value which is a multiple of π/2.

Discrimination of the PV effect by E-field modulation under static magnetic field.Discrimination of the PV effect by E-field modulation under static magnetic field. Show more

This field arrangement is such that the M1 transition amplitude and Stark-induced amplitudes are out of phase [14]. Thus, the M1 Stark interference is suppressed. Additional suppression is provided by the use of a power-build-up cavity. The M1 transition amplitude proportional to k×E vanishes to the degree that the field in the cavity is a standing wave, and the net wave vector k is suppressed.

For an isotope with zero nuclear spin I, there are three Zeeman-split components of the transition. A Stark-induced transition amplitude is generally expressed in terms of real scalar ( α), vector ( β), and tensor ( γ) transition polarizabilities [12,15]; however, for the case of a J=0J=1 transition, only the vector transition polarizability contributes. Assuming that the magnetic field is strong enough to resolve the Zeeman components of the transition and selecting the quantization axis along the magnetic field, we obtain the following transition rates:

where I is the light intensity. Here ζ characterizes the PV-induced electric-dipole transition amplitude between states with total angular momenta and projections F, M and F, M:

A profile of the B-field-split 408-nm spectral line of Yb174 recorded at 1st and 2nd harmonic of the modulation. Also a simulated PV contribution is shown for clarity. E˜=5kV/cm; dc offset=40V/cm; θ=π/4; an effective integration time is 10 s per point.A profile of the B-field-split 408-nm spectral line of Yb174 recorded at 1st and 2nd harmonic of the modulation. Also a simulated PV contribution is shown for clarity. E˜=5kV/cm; dc offset=40V/cm; θ=π/4; an effective integration time is 10 s per ... Show more

where q=M-M labels the spherical component and F,M,1,-q|F,M is a Clebsch-Gordan coefficient. In expressions (2) and (3), we neglect the term quadratic in PV mixing. Using the theoretical value of ζ10-9ea0 [6] combined with the measured |β|=2.24-0.12+0.07×10-8ea0/(V/cm) [15,16], the expected relative strength of the PV effect, 2ζ/βE, is 10-4, for θ=π/4 and E=1kV/cm.

The transition rates (2) and (3), are detected by measuring the population of the 6s6pP03 state, where 65% of the atoms excited to the 5d6sD13 state decay spontaneously (Fig. 1). This is done by resonantly exciting the atoms with 649-nm light to the 6s7sS13 state downstream from the main interaction region and collecting the fluorescence resulting from the decay of this state back to 6s6pP03 state, and also to 6s6pP13 and 6s6pP23 states. As long as the 408-nm transition is not saturated, the fluorescence intensity measured in the probe region is proportional to the rate of that transition.

In order to isolate the Stark-PV interference term in the transition rate from the dominant Stark-induced transition rate, we harmonically modulate the applied electric field. The dominant Stark-induced rate has a static component and a component oscillating at twice the modulation frequency, while the Stark-PV interference term oscillates at the first harmonic. The frequency discrimination is performed using lock-in amplifiers. For an arbitrary angle of the light polarization θ, there are generally three Zeeman components of the transition present while scanning over the profile as shown in Fig. 3(a). The first-harmonic signal due to Stark-PV interference has a characteristic signature: the sign of the phase of the modulation of the two extreme components of the transition is opposite to that of the central component. The second-harmonic signal provides a reference for the line shape since it is free from interference effects linear in E [Fig. 3(b)]. If, in addition to the oscillating electric field, there is also a dc component present in the applied field, a signature identical to that in the second harmonic will also appear in the first harmonic, Fig. 3(c). The latter can be used to increase the first-harmonic signal above the noise, which makes the profile analysis more reliable.

The PV-interference parameter ζ/β. Mean value: 39(4)stat(5)systmV/cm, |ζ|=8.7±1.4×1010ea0. The 68% confidence band includes both the statistical and the systematic uncertainties.The PV-interference parameter ζ/β. Mean value: 39(4)stat(5)systmV/cm, |ζ|=8.7±1.4×1010ea0. The 68% confidence band includes both the statistical and the systematic uncertainties. Show more

A schematic of the Yb-APV apparatus is shown in Fig. 2. A beam of Yb atoms is produced (inside of a vacuum chamber with a residual pressure of 3×10-6Torr) with an effusive source, which is a stainless-steel oven loaded with Yb metal, operating at 500°C. The oven is outfitted with a multislit nozzle, and there is an external vane collimator reducing the spread of the atomic beam in the horizontal direction. The resulting Doppler width of the 408-nm transition is 12MHz [16].

Downstream from the collimator, the atoms enter the main interaction region where the Stark- and PV-induced transitions take place. Up to 80 mW of light at the transition wavelength of 408.345 nm in vacuum is produced by frequency doubling the output of a Ti:sapphire laser (Coherent 899).

The 408-nm light is coupled into a power buildup cavity (PBC) inside the vacuum chamber. The finesse and the circulating power of the PBC are measured to be up to F=9000 and P=8W, respectively. The laser is locked to the PBC using the FM-sideband technique [17]. In order to remove frequency excursions of the PBC in the acoustic range, the cavity is locked to a more stable confocal Fabry-Pérot étalon, once again using the FM-sideband technique. This stable scannable cavity provides the master frequency, with the power-build-up cavity serving as the secondary master for the laser.

The magnetic field is generated by a pair of rectangular coils designed to produce a uniform magnetic field up to 100 G: 1% nonuniformity over the volume with the dimensions of 1×1×1cm3 in the interaction region. Additional coils placed outside of the vacuum chamber compensate for the external magnetic fields down to 10 mG at the interaction region. The residual B field of this magnitude does not have an impact on the PV-effect measurements, since its contribution is measured using the field reversals (see below).

The electric field is generated with two wire-frame electrodes separated by 2 cm. The copper electrode frames support arrays of 0.2-mm diameter gold-plated wires. This design allows us to reduce the stray charges accumulated on the electrodes by minimizing the surface area facing the atomic beam, thus minimizing stray electric fields. ac voltage up to 10 kV at a frequency of 76.2 Hz is supplied to the E-field electrodes by a homebuilt high-voltage amplifier. An additional dc bias voltage up to 100 V can be added.

Light emitted from the interaction region at 556 nm is collected with a light guide and detected with a photomultiplier tube. This signal is used for initial selection of the atomic resonance and for monitoring purposes. Fluorescent light from the probe region is collected onto a light guide using two optically polished curved aluminum reflectors and registered with a cooled photodetector (PD). The PD consists of a large-area ( 1×1cm2) Hamamatsu photodiode connected to a 1-GΩ transimpedance preamplifier, both contained in a cooled housing (temperatures down to -15°C). The preamp’s bandwidth is 1 kHz and the output noise is 1mV (rms). The 649-nm excitation light is derived from a single-frequency diode laser (New Focus Vortex) producing 1.2mW of cw output, high enough to saturate the 6s6pP036s7sS13 transition. A drift of the laser frequency is eliminated by locking the diode laser to a transfer cavity, in turn locked to a frequency-stabilized He-Ne laser.

The signals from the PMT and PD are fed into lock-in amplifiers for frequency discrimination and averaging. The typical time of a single spectral profile acquisition is 20 s. The first- and second-harmonic signals are registered simultaneously, which reduces the influence of slow drifts, such as instabilities of the atomic-beam flux. The modulation frequency is limited by several factors. Thermal distribution of atomic velocities in the beam causes a spread (of 2ms) in the time of flight between the interaction region and the probe region. This, along with the finite bandwidth of the PD, leads to a reduction of the signal-modulation contrast. The choice of the modulation frequency of 76.2 Hz is a tradeoff between this contrast degradation and the requirement of lock-in detection over many modulation periods.

In Fig. 4 a profile of the B-field-split 408-nm spectral line of the Yb174 isotope is shown. The 649-nm light-induced fluorescence was recorded during a typical integration run. Statistical error bars are smaller than the size of the points in the figure. The peculiar asymmetric line shape of the Zeeman components is a result of the dynamic Stark effect [16]. The profiles are fit to an approximated analytic function. The fit amplitudes of the three peaks yield the fluorescence amplitudes for the different Zeeman components at 1st and 2nd harmonics of the modulation. Ideally, in the absence of apparatus imperfections and systematic effects, the following combination of amplitude ratios between the 1st and 2nd harmonics yields the PV-interference effect:

where A±1, A0 are the amplitudes of the respective Zeeman components and E˜ is the amplitude of modulating electric field.

The detailed analysis of an impact of the apparatus imperfections and systematic effects on the accuracy of the measurements will be presented elsewhere. Here we address briefly the principles of this analysis. The PV effect is discriminated from other effects by recording the spectral profiles for different combinations of the B field and the light polarization angle θ, and by isolating the part of the measured values of K that has a correct PV response upon the reversals. In addition we artificially impose exaggerated combinations of imperfections and measure their effect on K. Then, by scaling down these contributions we estimate the residual uncertainties in the PV measurements. Such experiments showed a negligibly small contribution of the imperfections compared to the present accuracy of the PV-effect determination (see below).

In Fig. 5, the PV-interference parameter ζ/β is shown as determined in 19 consecutive runs ( 60 h of integration). Its mean value is 39(4)stat(5)systmV/cm, which is in agreement with the theoretical predictions. Thus, |ζ|=8.7±1.4×10-10ea0, which is the largest APV amplitude observed so far. This confirms the predicted enhancement of the PV effect in Yb.

The present measurement accuracy is not yet sufficient to observe the isotopic and hyperfine differences in the PV amplitude. It must be better than 1% for PV amplitude in a single transition [11,18,19]. We found that the main factors limiting the present accuracy are fluctuations of the electric field in the interaction region (due to stray fields and HV-amplifier noises), and frequency excursions of the Fabry-Pérot étalon serving as a frequency reference for the optical system. A direct impact of these factors on the spectral profiles has been observed, thus leading to errors not only in the APV measurements, but also in the study of systematic effects and apparatus imperfections. This accounts for the relatively large systematic uncertainty of the PV parameter. In the course of the APV measurements, several improvements have been implemented targeting these noise sources. They have demonstrated a possibility to reduce the measurement errors substantially. This is seen in Fig. 5, where the last six measurements exhibit higher accuracy than the rest. An upgrade of the apparatus is under way aimed at eliminating the noise sources, which will open ways to the measurements of neutron distributions and anapole moments.


  1. J. Guena, M. Lintz, and M. A. Bouchiat, Mod. Phys. Lett. A 20, 375 (2005).
  2. C. S. Wood, S. C. Bennett, D. Cho, B. P. Masterson, J. L. Roberts, C. E. Tanner, and C. E. Wieman, Science 275, 1759 (1997).
  3. S. G. Porsev, K. Beloy, and A. Derevianko, Phys. Rev. Lett. 102, 181601 (2009).
  4. V. A. Dzuba, V. V. Flambaum, and I. B. Khriplovich, Z. Phys. D 1, 243 (1986).
  5. D. DeMille, Phys. Rev. Lett. 74, 4165 (1995).
  6. S. G. Porsev, G. Rakhlina Yu, and M. G. Kozlov, JETP Lett. 61, 459 (1995).
  7. B. P. Das, Phys. Rev. A 56, 1635 (1997).
  8. E. N. Fortson, Y. Pang, and L. Wilets, Phys. Rev. Lett. 65, 2857 (1990).
  9. J. S. M. Ginges and V. Flambaum, Phys. Rep. 397, 63 (2004).
  10. W. C. Haxton and C. E. Wieman, Annu. Rev. Nucl. Part. Sci. 51, 261 (2001).
  11. B. A. Brown, A. Derevianko, and V. V. Flambaum, Phys. Rev. C 79, 035501 (2009).
  12. M. A. Bouchiat and C. Bouchiat, J. Phys. II (France) 36, 493 (1975).
  13. R. Conti, P. Bucksbaum, S. Chu, E. D. Commins, and L. Hunter, Phys. Rev. Lett. 42, 343 (1979).
  14. P. S. Drell and E. D. Commins, Phys. Rev. A 32, 2196 (1985).
  15. C. J. Bowers, D. Budker, S. J. Freedman, G. Gwinner, J. E. Stalnaker, and D. DeMille, Phys. Rev. A 59, 3513 (1999).
  16. J. E. Stalnaker, D. Budker, S. J. Freedman, J. S. Guzman, S. M. Rochester, and V. V. Yashchuk, Phys. Rev. A 73, 043416 (2006).
  17. R. W. P. Drever, J. L. Hall, F. V. Kowalski, J. Hough, G. M. Ford, A. J. Munley, and H. Ward, Appl. Phys. B 31, 97 (1983).
  18. S. Porsev, M. Kozlov, and Y. Rakhlina, Hyperfine Interact. 127, 395 (2000).
  19. A. D. Singh and B. P. Das, J. Phys. B 32, 4905 (1999).

About the Authors

Image of K. Tsigutkin
Image of D. Dounas-Frazer
Image of A. Family
Image of J. E. Stalnaker
Image of V. V. Yashchuk
Image of D. Budker

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