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LASER COOLED, STORED ION EXPERIMENTS AT NBS AND POSSIBLE APPLICATIONS TO

MICROWAVE AND OPTICAL FREQUENCY STANDARDS

D. Wineland, J. Bergquist, R. Drullinger, H. Hemmati, W. Itano, F. Walls

To cite this version:

D. Wineland, J. Bergquist, R. Drullinger, H. Hemmati, W. Itano, et al.. LASER COOLED, STORED ION EXPERIMENTS AT NBS AND POSSIBLE APPLICATIONS TO MICROWAVE AND OPTI- CAL FREQUENCY STANDARDS. Journal de Physique Colloques, 1981, 42 (C8), pp.C8-307-C8-313.

�10.1051/jphyscol:1981838�. �jpa-00221734�

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JOURNAL DE PHYSIQUE

CoZZoque C8, suppl~ment au n012, Tome 4 2 , ddcembre 1981 page C8-307

LASER COOLED, STORED ION EXPERIMENTS AT NBS AND POSSIBLE APPLICATIONS TO MICROWAVE AND OPTICAL FREQUENCY STANDARDS

D.J. Wineland, J.C. Bergquist, R.E. Drullinger, H. Hemmati, W.M. Itano and F.L. Walls

Frequency and Mme Standards Group, Time and Frequency Division, National Bureau o f Standards, Boulder, Colorado 80303, U. S. A.

Abstract.

-

Research on s t o r e d i o n frequency standards a t t h e U n i t e d States N a t i o n a l Bureau o f Standards i s b r i e f 1 y discussed. We summarize p a s t work and i n d i c a t e d i r e c t i o n s o f f u t u r e research.

I n t r o d u c t i o n . - The purpose o f t h i s paper i s t o b r i e f l y summarize t h e work a t t h e N a t i o n a l Bureau o f Standards (NBS) which has been d i r e c t e d towards r e a l i z i n g a frequency standard based on s t o r e d i o n s . The s i m i l a r work o f o t h e r groups [I] i s n o t discussed here. T h i s summary b r i e f l y describes p a s t work and i n d i c a t e s f u t u r e d i r e c t i o n s o f research a t NBS.

The s t o r e d i o n work a t NBS was i n i t i a t e d i n t h e F a l l o f 1977. The goal o f t h i s work has been t o devise a technique f o r r e a l i z i n g a frequency standard whose accuracy would be s i g n i f i c a n t l y b e t t e r t h a n t h a t o f t h e Cs atomic beam frequency standard. W i t h t h i s i n mind, t h e i o n storage method [2] was pursued because i t can p r o v i d e l o n g confinement times w i t h o u t t h e usual p e r t u r b a t i o n s associated w i t h confinement (e.g., t h e w a l l s h i f t i n t h e H-maser).

The i n i t i a l work was d i r e c t e d toward r e a l i z i n g l a s e r c o o l i n g o f i o n s 131, s i n c e t h i s would p r o v i d e a way t o s u b s t a n t i a l l y suppress t h e frequency s h i f t due t o t h e second-order Doppler o r t i m e - d i l a t i o n e f f e c t . For these i n i t i a l e x p e r i - ments, Mg+ i o n s were s t o r e d i n a Penning trap. Mg+ i o n s were chosen, s i n c e t h e e l e c t r o n i c s t r u c t u r e i s f a i r l y simple ( i . e . , l i k e t h a t o f n e u t r a l a l k a l i atoms) and r e q u i r e d a l a s e r source a t 280 nm. The Penning t r a p was chosen because t h e r e s i d u a l h e a t i n g mechanisms ( a t l e a s t f o r a c l o u d o f ions) a r e l e s s than f o r t h e rf t r a p .

I n t h e f i r s t experiments [4], t h e temperature o f t h e i o n s was monitored d i r e c t l y by t h e b o l o m e t r i c technique 151. F i g u r e 1 shows t h e Mg+ i o n temperature vs. time f o r a f i x e d l a s e r d e t u n i n g o f about -2 GHz from t h e 3s 25% (MJ = -$) +

3p 2P,,2 (MJ = - 3 / 2 ) t r a n s i t i o n frequency. The s e n s i t i v i t y o f these temperature measurments was l i m i t e d by n o i s e i n t h e e l e c t r o n i c d e t e c t i o n . Therefore, subse- quent measurements d e t e c t e d t h e temperature by observing t h e fluorescence l i g h t s c a t t e r e d by t h e ions and measuring t h e Doppler w i d t h s o f t h e o p t i c a l 1 in e s [6].

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:1981838

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JOURNAL DE PHYSIQUE

LASER ON

)c 5.6 m i n 4 IONS REMOVED 7

1. I o n temperature vs. t i m e when l a s e r c o o l i n g i s a p p l i e d f o r f i x e d l a s e r de- t u n i n g o f -2 GHz. The i o n s were i n i t i a l l y heated above e q u i l i b r i u m tempera- t u r e w i t h t h e l a s e r . Laser c o o l i n g was then a p p l i e d on t h e 3s 2S% (MJ = -%)

+ 3p 2P3/2 (MJ = - 3 / 2 ) t r a n s i t i o n f o r a f i x e d t i m e u n t i l a temperature approaching 0 K (< 40 K) was achieved. A f t e r t h e l a s e r i s t u r n e d o f f , t h e i o n s r e t h e r m a l i z e t o t h e ambient temperature.

\

Mg II RESONANCE TRANSITIONS ( ~ S ~ S , / ~ , m, = -b 1-

2. Spectra o f one Zeeman component o f l a s e r cooled 24,25,26~g+. The room temperature Doppler w i d t h o f these l i n e s i s about 3 GHz. Only t h e 2 4 ~ g i i s d i r e c t l y l a s e r cooled. The 2 5 ~ g + h y p e r f i n e s t r u c t u r e has been o p t i c a l l y pumped r e s u l t i n g i n t h e o b s e r v a t i o n o f o n l y t h e (MJ = -5, MI = -s/,)++

(MJ =

-

3 / 2 , MI = - 5 / 2 ) component.

F i g u r e 2 shows t h e fluorescence l i g h t from a "low" power l a s e r which i s swept i n frequency across t h e 3s 2$ (MJ = -5) -t 3p 2P3/2 (MJ = - 3 / 2 ) o p t i c a l t r a n s i t i o n s o f t h e t h r e e n a t u r a l l y o c c u r i n g M ~ + isotopes. A t t h e same time, a h i g h e r power (approximate1 y 10 times h i g h e r power) f ixed-frequency l a s e r i s tuned t o t h e low frequency s i d e of t h e 2 4 ~ g + t r a n s i t i o n t o keep t h e sample cold. (Note t h a t t h e 2 5 ~ g + and 2 6 ~ g + isotopes a r e n o t d i r e c t l y l a s e r coo?ed, b u t a r e cooled by Coulomb c o l l i s i o n s w i t h t h e coaled 2 4 ~ g + . )

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Lowest temperatures have so f a r been obtained f o r s i n g l e i o n s 171 where cyclotron-magnetron "temperatures" o f approximately 0.05 K have been obtained f o r a s i n g l e 2 4 ~ g + ion. F i g u r e 3 shows t h e double-resonance d e t e c t i o n o f t h e (MJ = -4) + 2P3/, (MJ = -%) o p t i c a l t r a n s i t i o n i n a s i n g l e 2 4 ~ g + i o n . Our theore- 2S4

W

s

3 Y

r

BACKGROUND LEVEL

RELATIVE LASER FREQUENCY (MHz)

3 . Double-resonance curve o f a s i n g l e 2 4 ~ g + i o n . On t h e v e r t i c a l a x i s i s t h e

fluorescence from a fixed-frequency l a s e r (power approximately 5 yW) tuned t o t h e (2P3/,, MJ = -3/2)+(2S4, M = -5) t r a n s i t i o n . Each p o i n t represents

J

a 10 s i n t e g r a t i o n ; t h e connecting l i n e s a r e o n l y f o r c l a r i t y . The h o r i - z o n t a l a x i s i s t h e frequency o f t h e low-power (<< 5 yW) l a s e r which i s c o n t i n u o u s l y scanned across t h e (2P3,,, MJ = -+)+(PS+, MJ = -5) t r a n s i t i o n . The dashed curves a r e s i m u l a t i o n s o f fluorescence a t T = 0 K and 100 mK (no added noise). The s o l i d curve i s experimental data. From these data, we conclude T = 50 f 30 mK.

t i c a l p r e d i c t i o n s [8, a l s o I t a n o , Wayne M., and Wineland, D. J., t o be published]

i n d i c a t e d t h a t lower temperatures should be obtained; p o s s i b l e l i m i t a t i o n s may be caused by t h e presence o f i m p u r i t y i o n s i n t h e t r a p . F u t u r e experimental inves- t i g a t i o n s a r e planned; a new apparatus w i t h improved fluorescence c o l l e c t i o n e f f i c i e n c y i s b e i n g constructed.

I n t h e Penning t r a p , i o n s a r e unstable w i t h r e s p e c t t o c o l l i s i o n s w i t h background gas; t h a t i s , c o l l i s i o n s cause t h e magnetron o r b i t s t o increase i n s i z e and t h i s leads t o i o n l o s s . T h i s process can be reversed by a technique which i s f o r m a l l y e q u i v a l e n t t o t h e usual l a s e r c o o l i n g [4,6, a l s o I t a n o , Wayne M., and Wineland, D. J., t o be published]; s p e c i f i c a l l y , t h e magnetron energy i s

increased and t h e o r b i t s i z e reduced by l a s e r s c a t t e r i n g by s p a t i a l l y t a i l o r i n g t h e l a s e r beam. The r e s u l t i s t h a t i n f i n i t e confinement times a r e i n p r i n c i p l e p o s s i b l e i n t h e Penning t r a p .

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C8-3 1 0 JOURNAL DE PHYSIQUE

The ground-state s t r u c t u r e o f M ~ + i o n s has been measured by double-resonance schemes where changes i n t h e l a s e r fluorescence can be used t o monitor ground- s t a t e rf and microwave t r a n s i t i o n s [9,10]. T h i s has l e d t o a measurement o f t h e ground-state h y p e r f in e constant (A = -596.254 376(54) MHz) and gI/gJ (= 9.299 484(25) x i n 2 s ~ g + . For t h i s i o n , t h e d e r i v a t i v e o f t h e ground- s t a t e (MI, MJ) = ( - 3 / 2 , %) t o (-%, %) t r a n s i t i o n w i t h r e s p e c t t o magnetic f i e l d 6, goes t o zero a t Bo z 1.24 T. The corresponding resonance (u Z 292 MHz) was ob- served a t t h i s f i e l d w i t h l i n e w i d t h s as small as 0.012 Hz (Q z 2.4 x loi0) by im- plementing t h e Ramsey i n t e r f e r e n c e method w i t h two coherent rf pulses separated i n t i m e by 41.4 s (see f i g u r e 4). We expect t h a t such narrow resonance l i n e s (and even narrower l i n e s ) can be observed i n o t h e r i o n s (e.g., H ~ + ) w i t h h i g h e r ground- s t a t e t r a n s i t i o n frequencies. T h i s c o u l d t h e n y i e l d extremely h i g h Q (> l o z 2 ) i n microwave t r a n s i t i o n s which would be v a l u a b l e f o r frequency standard a p p l i c a t i o n s .

RF Frequency - 291 996 250 (Hz )

4. R f resonance curve f o r t h e (inI, mJ) = (-3/2, 4) t o (-%, 4) ground-state h y p e r f i n e t r a n s i t i o n i n 2 5 ~ g + . Each c i r c l e represents t h e average of f o u r measurements ( t o t a l d e t e c t i o n fluorescence i n t e g r a t i o n time o f 16 s). The o s c i l l a t o r y lineshape r e s u l t s from t h e use o f t h e Ramsey method t o d r i v e t h e t r a n s i t i o n . Two coherent rf pulses o f d u r a t i o n r: = 1.02 s separated by T = 41.4 s were applied. The v e r t i c a l arrow marks t h e c e n t r a l minimum, which corresponds t o t h e resonance frequency.

I n some double-resonance schemes, i t i s p o s s i b l e t o s c a t t e r many photons f o r each microwave o r o p t i c a l llclockll photon absorbed. ( I n Ref. 10, a f a c t o r o f about l o 6 was achieved.) This "quantum m ~ l t i p l i c a t i o n ~ ~ should a l l o w t h e s i g n a l - t o - n o i s e r a t i o i n double-resonance d e t e c t i o n schemes t o be l i m i t e d o n l y by t h e s t a t i s t i c a l n o i s e i n t h e number o f i o n s t h a t have made t h e "clock1' t r a n s i t i o n [9,11]. T h i s w i l l be extremely i m p o r t a n t f o r frequency standards based on ions where t h e number o f i o n s i s n e c e s s a r i l y r a t h e r small.

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Because o f t h e above r e s u l t s , we have i n i t i a t e d work a t NBS t o r e a l i z e microwave [ll] and o p t i c a l [11,12] frequency standards based on ttg+ i o n s s t o r e d i n a Penning t r a p .

The proposed microwave frequency standard i s based on t h e (F, MF) = (1,l) ++

(2,l) ground-state h y p e r f i n e t r a n s i t i o n i n 2 0 1 ~ g + , which i s field-independent t o f i r s t order a t Bo r 0.534 T, w i t h frequency z 25.9 GHz (see f i g u r e 5). I f Bo can be c o n t r o l l e d t o s l i g h t l y b e t t e r t h a n 0.1 ppm over t h e i o n cloud, t h e f r a c t i o n a l frequency s h i f t can be k e p t below 10-15. ( A t t h e I'f ield-independent1' p o i n t Av/vO = (AB/B0)'/6). The v e l o c i t y i n t h e magnetron motion w i l l g i v e a second- o r d e r Doppler s h i f t ; i t should be c o n t r o l l a b l e t o 1 0 - l 5 (see below). A l l o t h e r systematic s h i f t s , such as those due t o c o l l i s i o n s , t h e t r a p e l e c t r i c f i e l d s , o r thermal r a d i a t i o n appear t o be l e s s t h a n 1 0 - l 5 [Ill. I t should be p o s s i b l e t o observe t h e t r a n s i t i o n w i t h a Q o f 2.6 x 1012 o r b e t t e r , by u s i n g o p t i c a l pumping and d e t e c t i o n techniques s i m i l a r t o those demonstrated w i t h 2 5 ~ g + . The accuracy o f t h i s standard c o u l d be b e t t e r than 10-15.

5. Ground-state h y p e r f i n e energy l e v e l s o f 2 0 1 ~ g + VS. magnetic f i e l d . States a r e designated by t h e (F, MF) representation. Three t r a n s i t i o n s a r e i n d i - c a t e d a t t h e f i e l d s where t h e t r a n s i t i o n frequencies a r e independent o f magnetic f i e l d t o f i r s t order.

The proposed o p t i c a l frequency standard [11,12] i s based on t h e two-photon- allowed 5d1° 6s 2S54

-

5d9 6s2 2D,,2 Hg* t r a n s i t i o n , which has a n a t u r a l Q o f 7.4 x 1014. The f i r s t - o r d e r Doppler e f f e c t can be e l i m a t e d by d r i v i n g t h e t r a n s i -

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C8-3 1 2 JOURNAL DE PHYSIQUE

t i o n w i t h counter-propagating 563.2 nm l a s e r beams. Hyperfine-Zeeman components, whose magnetic f i e l d d e r i v a t i v e s vanish a t p a r t i c u l a r values o f Bo, e x i s t i n

1 9 9 ~ g + and 201~g+. The two-photon t r a n s i t i o n can be detected w i t h high e f f i c i e n c y by using the 194.2 nm fluorescence i n t e n s i t y as a probe o f the ground-state population. Taking f u l l advantage o f the high Q t r a n s i t i o n would r e q u i r e a l a s e r w i t h l i n e w i d t h less than 1 Hz, which does n o t e x i s t a t present. However, l i n e - widths 5 100 Hz appear f e a s i b l e and could be used f o r i n i t i a l experiments. I f t h e l a s e r l i n e w i d t h i s l e s s than the natural linewidth, then the ac Stark s h i f t i s about 2 x 1 0 - l 5 near saturation. A l l other systematic s h i f t s appear t o be l e s s than 10-Is. We note t h a t t h e ac Stark s h i f t can be made n e g l i g i b l y small by d r i v i n g the s i n g l e photon 2S4 + 2D5,2 quadrupole t r a n s i t i o n . I n t h i s case, i t w i l l be desirable t o use a s i n g l e i o n t h a t can be confined t o approximately r e a l - i z e the Dicke c r i t e r i o n i n order t o suppress f i r s t - o r d e r Doppler e f f e c t s .

The method c u r r e n t l y being investigated f o r generating t h e required 194.2 nm r a d i a t i o n f o r l a s e r cooling and o p t i c a l detection i s sum-frequency mixing i n a KB5 c r y s t a l o f the output o f a 792 nm single-mode cw r i n g dye l a s e r and the second harmonic, generated i n an ADP c r y s t a l , o f the output o f a 514 nm s t a b i l - ized, single-mode cw ~ r + laser.

For the microwave frequency standard, i t i s e s p e c i a l l y desirable t o use the l a r g e s t possible number o f ions i n order t o increase signal t o noise. Unfor- tunately, as the number o f ions i s increased, the second-order Doppler s h i f t due t o magnetron r o t a t i o n also increases, which w i l l , therefore, l i m i t the number o f ions t o about l o 5 o r less f o r 10-l5 accuracy [Ill. (A s i m i l a r problem e x i s t s f o r t h e rf t r a p due t o the k i n e t i c energy i n the micromotion 1131). Therefore, studies w i l l a l s o be devoted t o methods o f c o n t r o l l i n g the density and shape o f the i o n clouds.

We g r a t e f u l l y acknowledge the support o f the United States A i r Force O f f i c e o f S c i e n t i f i c Research and the O f f i c e o f Naval Research.

References.

[I] See f o r example the f o l l o w i n g references and other references therein:

Major, F. G., and Werth, G., Phys. Rev. 30 (1973) 1115; Dehmelt, H., Proc.

35th Ann. Symp. Freq. Control, Philadelphia, Pa., June 1981; McGuire, M.

D., Petsch, R., and Werth, G., Phys. Rev. A.

2

(1978) 1999; McGuire, M.

D., B u l l . Am. Phys. Sac.

3

(1981) 615; Jardino, M., Desaintfuscien, M., B a r i l l e t , R., Viennet, J., P e t i t , P., and Audoin, C., Appl. Phys.

24

(1981) 1. Neuhauser, W., Hohenstatt, M., Toschek, P. E., and Dehmelt, H., Phys. Rev. A22 (1980) 1137; Javanainen, J., and Stenholm, S., Appl. Phys.

24 (1981) 1 5 c

-

[ Z ] Dehmelt, H. G., Advances At. Mol. Phys. 3 (1967) 53 and

5

(1969) 109.

[3] Wineland, D. J., and Dehmelt, H. G., B u l l . Am. Phys. Soc.

20

(1975) 637;

Hansch, T. W., and Schawlow, A. L., Opt. Commun. 2 (1975) 68.

Wineland, D. J., D r u l l i n g e r , R. E., and Walls, F. L., Phys. Rev. Lett.

(1978) 1639.

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Dehmelt, H., and Walls, F. , Phys. Rev. L e t t . 21 (1968) 127. Wineland, D.

J., and Dehmelt, H. G., J. Appl. Phys.

9

(1975) 919.

D r u l l i n g e r , R. E., Wineland, D. J., Bergquist, J.

(1980) 365.

C., Appl. Phys.

Wineland, D. J., and Itano, Wayne M., Phys. L e t t .

82A

(1981) 75.

Wineland, D. J. , and Itano, Wayne M. , Phys. Rev. (1979) 1521.

Wineland, D. J., Bergquist, J. C., Itano, Wayne M., and D r u l l i n g e r , R. E., Opt. L e t t . 5 (1980) 245.

Itano, Wayne M., and Wineland, D. J., Phys. Rev. M , (1981) 1364.

Wineland, D. J. , Itano, Wayne M. , Bergquist, J. C., and Walls, F. L., Proc. 35th Ann. Symp. Freq. Control, Philadelphia, Pa., June, 1981.

Bender, P. L., H a l l , J. L., Garstang, R. H., Pichanick, F. M. J., Smith, W. W., Barger, R. L., and West, J. B . , B u l l . Am. Phys. Soc. 21 (1976) 599.

Wineland, D. J., Proc. Conf. on Prec. Meas. and Fundamental Constants, Gaithersburg, Md. June, 1981.

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