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Hyperfine structure of 14NIII 2p 2P3/2 by quantum beats after ion surface interaction at grazing incidence

A. Schirmacher, H. Winter, H.J. Andrä, Y. Ouerdane, J. Désesquelles, G.

Docao, A. Denis

To cite this version:

A. Schirmacher, H. Winter, H.J. Andrä, Y. Ouerdane, J. Désesquelles, et al.. Hyperfine structure of 14NIII 2p 2P3/2 by quantum beats after ion surface interaction at grazing incidence. Journal de Physique, 1987, 48 (6), pp.905-909. �10.1051/jphys:01987004806090500�. �jpa-00210519�

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HYPERFINE STRUCTURE OF 14NIII 2p

2P3/2

BY QUANTUM BEATS AFTER ION

SURFACE INTERACTION AT GRAZING INCIDENCE

A.

Schirmacher,

H.

Winter,

H.J. Andrä, Y.

Ouerdane+,

J.

Désesquelles+,

G. DoCao+ and A. Denis+

Institut für

Kernphysik

der Universitât

Münster, Domagkstr.

71, D-4400 Münster, F.R.G.

+Laboratoire de Spectrométrie Ionique et

Moléculaire,

43 Bd. du 11 novembre 1918, 69622

Villeurbanne,

France

(Reçu

le 12 fivrier 198?’, accepte le !4 mars

1987)

Résumé.- Nous avons mesuré, par une éthode de battements quantiques, les écarts de structure hyperfine

de 14NIII 2p

2P3/203BD3/2,5/2

=

(252,0 ± 1, 1)

MHz et 03BD1/2,3/2 =

(126,2 ± 0,4)

MHz. De ces fréquences

on déduit le moment quadrupolaire électrique du noyau Q

(14N) = (19,4 ± 0,9)

mb et la constante de

couplage

quadrupolaire

pour l’électron 2p de 14NIII

1s22s22p 2P3/2 :

e Q qat =

-(16,6 ± 0,6)

MHz.

Abstract.- Applying a modified quantum beat method, the hyperfine splittings of 14NIII 2p

2P3/2

are

determined to 03BD3/2,5/2 =

(252.0 ± 1.1)

MHz and 03BD1/2,3/2 =

(126.2

±

0.4)

MHz. From the frequencies we

deduce the nuclear electric quadrupole moment of

14N Q (14N) = (19.4 ± 0.9)

mb and the

quadrupole

coupling constant for the 2p-electron in 14NIII

1s22s22p 2P3/2 :

e Q

qat = - (16-6 ± 0.6)

MHz.

Classification

Physics Abstracts

34.50 H ,- 35.20 S- 21.10 K

Measurements of hyperfine

(hf) -

splittings in sta-

ble and excited terms in ionized 14N allow to deduce the electric nuclear

quadrupole

moment of

14 N [1]

and

the

quadrupole coupling

constant of the 14NI

2pS -con-

figuration which is a relevant quantity in mol-ecular spectroscopy. Since the quadrupole interaction is neg-

ligible in the

14NI-atom,

the coupling constant has

been deduced from molecular spectra with some un- certainty

[2].

We pursue the concept to deduce this

constant by an extrapolation from coupling constants

for the 14 NII

2p2-

and the 14 NIII 2p-configurations.

In this paper we will concentrate our description on

measurements in the 14NIII 2p

2P3/2-term

to get the

quadrupole coupling constant for this configuration and

the nuclear electric quadrupole moment of

14 N Q (14N) .

For determining the hf-splittings of 14NIII 2p

2P3/2

we apply the ground term hf-quantum beat technique

[3]

after the interaction of fast ions with a solid sur-

face at grazing incidence. These collisions result in a

large orientation in the distribution of electronic or-

bital angular momenta

[4]

which is partly transferred to the nuclear spins via hf-interaction. Since ground

and metastable terms in 14N are dominantly popu- lated after ion-surface scattering, the transient transfer of anisotropy between electronic shell and nucleus re-

flects the hf-frequencies of those terms.

To apply the fast beam quantum beat technique

in ground and metastable terms, we observe after ion- surface scattering the transient nuclear spin orienta-

tion. This is accomplished by the interaction of the scattered ions with a thin foil which rearranges

(and excites)

the electronic shell, but preserves the nuclear orientation. The observation of the circular polariza-

tion of foil excited light given by the Stoke’s parameter

S/1 = (1 ((1-) - 1 ((1+)) / (I (a-) + I (a+)) (I ((7:1:) =

intensity of light with negative and positive helicity,

respectively)

is a direct measure of the nuclear orien-

tation

[5].

The

quantum-beat

technique for stable terms by

Andri and Winter

[3]

is successfully applied by Schir-

macher

[7]

in most of the stable terms in 14NI and

14 NIL At the high energy end of the accelerator used in the studies of reference

[7] (Emax=

350

keV)

the quan-

tum beat spectra

yield

an indication of a frequency component which is estimated to stem from a hf-split- ting in 14NIII 2p

2 P3/2.

The experiments reported here

are motivated by the fact that an increase in energy of the projectiles will also increase the fraction of the

N2+-component

in the surface scattered beam so that hf-measurements in 14NIII are feasible.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01987004806090500

(3)

906

Experiment

A sketch of our

experimental

setup is shown in fig-

ure 1. The experiments are performed at the 2.5 MeV

van de Graaff accelerator of the Institut de

Physique

Nucl6aire

(Lyon, France). Nt-ions (0.8 -

1.8

MeV)

are used instead of N+-ions because of reasons of beam intensity. The ion-beam is bent by electric field plates onto a highly

polished

silicon surface of lenghts ranging from 2.5 to 5 mm at a scattering angle of

about 0.5°. In some runs the surface scattered ions

are selected with respect to charge states by electric

field

plates

and slit systems close behind the target.

All these components are mounted on a common block which is moved

by

stepmotor drive with respect to a carbon foil about 5

jig/CM 2

thick and its surface nor-

mal

parallel

to the beam.

The circular polarization of the light emitted from foil excited atoms is detected by a lens system, quarter

wave plate, beam splitter polarizer, and two indepen-

dent

photomultiplier

channels. This detection scheme

provides a simultaneous measurement of

I(a-)

and

I(a+)

which cancels the effects due to fluctuations of the beam intensity on the data.

For the optical detection of nuclear orientation transitions from terms with large transfer factors be- tween nuclear and electronic orientation should spec-

troscopically be selected

[5].

In these experiments, however, the

intensity

of

light

is rather low so that we

relinquish an interference line filter and simultaneously

observe all transitions within the spectral response of the detector

("white light detection").

This causes

some reduction in the detected polarization

(and

quan-

tum beat

amplitudes)

in comparison to the selection of

favourable lines, but this drawback is overcompensated by the significant win in intensity. The same argu- ment holds with respect to the use of

N+-molecular

ions instead of

N+ -ions,

where some reduction in col-

lision induced orientation after ion-surface scattering

and

dissociation

of molecules in comparison to pure ions is observed

[6].

Data sets are taken by varying the distance be-

tween solid surface and foil via microcomputer-control

in equidistant steps and recording

1(0’-)

and

1(0’+).

Due to the mechanical

design

the minimum in ap-

proach of surface and foil is about 65 mm.

Results

In a number of experiments with 14

N+

-projecti-

les at energies between 0.8 and 1.8 MeV we resolve quantum beat pattern as shown in

figure

2 at an en-

ergy of 870 keV. Figure 3 shows in the upper part a Fourier-transform of the data in

figure

2 and in the

lower part of data at an energy of 1.57 MeV. Whereas the transform of the data in figure 2 shows components of terms in NI-III

(for

detailed discussion see

Ref.[7]),

the transform of the data at 1.57 MeV

(lower curve)

shows two prominent

frequencies

which dominate the

spectrum and can be ascribed to the

hf-splitting

in 14NIII 2p

2P3/2.

Figure 4

displays

the data where the

N2+-component

of the reflected beam at an energy of 1.1 MeV is selected

by

electric field

plates

and slits be- hind the target. The data show a simple beat structure

which is

generated

by two

frequencies

of the

splittings

in 14 NIII 2p

2P3/2 (see

Fourier transform in

Fig. 5).

The quantitative analysis of the hf-splittings of

Fig.l.-Experimental

setup

(4)

Fig.2.-Quantum beat pattern after the interaction of 870 keV -

N2 -

molecular ions with a solid Si-surface at

an angle of incidence of about o.3° . The plot shows the variation of the circular polarization fraction

8/1 of

foil

emitted light in dependence on the distance between surface and foil.

Fig.3.-Fourier-transform of the data in figure 2

(upper curve)

and of data at 1.57 MeV

(lower curve).

Details

with respect to the identification of charge states in

the Fourier-spectrum will be given in reference

[7].

14 NIII

2p2P3/2

is based on known frequencies in 14NI

[8]

14NII

[7]

which are simultaneously observed as

shown in the Fourier spectra in figure 3. By this cal-

ibration

procedure

of the frequency scale we find for 14 NIII

2p 2pS/2 :

From these frequencies we derive the A-factor

A3/2 - (96.6

z

0.4)

MHz and the B-factor

r83/2

=

(8.32 ±0.30)

MHz, respectively.

In previous investigations of hf-structures in ion- ized 14N

[1]

good agreement of the experimental data

with single configuration Hartree-Fock calculation

[9]

is found. For 14NIII 2p

ZP3/2

we compute

(r-S)2P

=

4.677

ao 3 (see

also Ref.

[10])

and with pi= 0.4037

JJB

me jmp [11]

where 3B is the Bohr magneton, me

and mp are the masses of electron and proton, respec-

tively, we have for the 2p-electron :

and

A3/2= 8/15

a2p= 96.05 MHz. This is in excellent agreement with our experiment and confirms earlier findings that single configuration Hartree-Fock calcu- lations provide

(r- 3)

-integrals for an adequate de- scription of hf-splittings in ionized 14N.

From the B-factor we deduce the electric

quadru-

pole moment of

14 N Q (14N)

and the quadrupole cou- pling constant e Q gat with the electric field gradi-

ent

qat= a2v /az2

at the nucleus. From measured

A3/2

we get

(r-3)2P

=

(4.707 :f:: 0.015) uo 3

and by

neglecting magnetic shielding one deduces from

b2p=

e2 Q (r -3 )2p, b2p

=

5/2 B3/2

=

(20.B:f:: 08)

MHz and

for the "experimental quadrupole moment"

(18.8 ± 0.7)

mb. By

applying

the Sternheimer correction

[12]

with

(1-R)-1 =

1.03 from calculations by Sen and Weiss

(5)

908

Fig.4.-Quantum beat pattern after the interaction of 1.1 MeV -

N2+

-molecular ions with a solid Si-surface. The

N2+-component

of the surface scattered ions is selected by means of electric field plates and slits.

[10],

we finally obtain Q

(14N) = (19.4 ± 0.9) mb.

For the 14NIII 2p

ZP3/2-term

we get for the coupling

constant of the single

2p-electron

e Q qat= -2

Bs/2=

- (16.6 ± 0.6)

MHz.

Fig.S.-Fourier-transform

of the data in figure 4. The

two

frequencies

are ascribed to the

hf-splittings

of 14NIII 2p

2P3/2-

Conclusion

In this paper we report on the application of the ground term quantum beat technique for the measure-

ment of the hf-splittings in 14NIII

2p 2P3/2.

The exper-

imental A-factor is well reproduced by a theoretical ap-

proach based on single configuration Hartree-Fock cal- culations. From the B-factor we deduce an electric nu-

clear quadrupole moment Q

( 14 N) = (19.4 ± 0.9)

mb.

This result supports the results of a former experiment

[1]

where Q

(14N) = (19.3 ± 0.8)

mb is found, and can

be considered as an independent test for the evaluation

of this quantity.

In addition we determined the electric quadrupole coupling constant for the 14NIII 2p-configuration. In

molecular spectroscopy the coupling constant for the single 2p-electron in the neutral 14NI

2p3-configura-

tion is of importance to deduce structures and orbital

populations in molecules containing 14N from mea-

sured hf-splittings. Since the quadrupole interaction in 14NI is too small, the constant has been estimated from molecular data with a high degree of uncertainty

[2].

There is good hope that an extrapolation based on

experimental

data in 14NII and 14NIII

(reported here)

will provide a more accurate determination of this con-

stant. Details of corresponding measurements in 14 NII and the analysis to determine the coupling constant in 14NI will be given elsewhere

[7].

Acknowledgements

The

hospitality during

the runs at the Labora-

(6)

toire de Spectrometrie Ionique et Moléculaire is grate- fully acknowledged. We thank M. Champlovier

(Lyon)

for his assistance in running the accelerator, U. Linke

(KFA J31ich)

and Fa. Wacker-Chemie

(Burghausen)

for providing us with the Si-target, and B.

Hippert (Bochum)

and H. Baumeister

(Mfnster)

for the pro-

duction of the carbon foils. We also acknowledge the support of H.W.

Ortjohann

during the

preparations

of

the experiments. This work is supported by the Son-

derforschungsbereich

216

Bielefeld/ Miins ter.

References

[1]

WINTER H. and ANDRA H.J., Phys. Rev. A21

(1980)

581.

[2]

TOWNES C.H. and DAILEY B.P., J. Chem. Phys.

17

(1949)

782.

[3]

ANDRA H.J. and WINTER H., Hyp. Int. 5

(1978)

403.

[4]

ANDRA H.J., Phys. Lett. 54A

(1975)

315 ; TOLK

N.H.,

TULLY J.C., KRAUS J.S., HEILAND W. and

NEFF

S.H.,

Phys. Rev. Lett. 41

(1978)

643.

[5]

ANDRA H.J., PLOHN H.J., FROHLING R. and

GAUPP A., Z. Physik A281

(1977)

15.

[6]

FROHLING R., Dissertation,

(Freie

Universität,

Berlin)

1983, unpublished.

[7]

SCHIRMACHER A. et al., to be published.

[8]

RADFORD H.E. and EVENSON K.M., Phys. Rev.

168

(1968)

71.

[9]

FROESE-FISCHER C., Comp. Phys. Commun. 4

(1972)

107.

[10]

SEN K.D. and WEISS A., Phys. Rev. A20

(1979)

1323.

[11]

TING Y. and WILLIAMS B., Phys. Rev. 89

(1953)

595.

[12]

STERNHEIMER

R.M.,

Phys. Rev. 84

(1951)

244.

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