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Radiofrequency and Mössbauer Spectra of a Paramaghetic Ion in the Presence of Hyperfine Interactions and of Tunnel Effect

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Radiofrequency and Mössbauer Spectra of a Paramaghetic Ion in the Presence of Hyperfine

Interactions and of Tunnel Effect

Françoise Hartmann-Boutron

To cite this version:

Françoise Hartmann-Boutron. Radiofrequency and Mössbauer Spectra of a Paramaghetic Ion in the

Presence of Hyperfine Interactions and of Tunnel Effect. Journal de Physique I, EDP Sciences, 1996,

6 (1), pp.137-147. �10.1051/jp1:1996133�. �jpa-00247173�

(2)

Radiofrequency and Môssbauer Spectra of

a

Paramagnetic Ion in the Presence of Hyperfine Interactions and of Tunnel Elfect

Françoise

Hartmann-Boutron

Laboratoire de

Spectrométrie Physique(*),

Université J. Fourier Grenoble I, B-P. 87,

38402 Saint Martin d'Hères

Cedex,

France

(Received

13

July1995,

revised in final form and accepted 2 October

1995)

Abstract. The influence of a coherent tunnel elfect on the magnetic

hyperfine

structure of

a diluted

paramagnetic

ion, with

an electronic

ground

state

[S;

= +S >

(S

>

)),

is studied under the

assurnptions

of zero

longitudinal rnagnetic

field and slow electronic relaxation. It is shown that the

radiofrequency

and Môssbauer spectra should be

altered,

with a

change

in the number and intensities of the hnes. When the

tunnelling

parameter, r, is

large compared

to the

hyperfine

structure, the

magnetic hyperfine

structure

sphtting

should be

strongly

reduced and

it should vanish for r - cc~.

Tunnelhng

elfects have already been observed in EPR expenrnents

on Tb~+ diluted in diamagnetic matrices. The cases of NMR with f

=

3/2

and of Môssbauer

spectroscopy for a transition le

=

3/2

fg =

1/2

are considered.

PACS. 76.20+q General

theory

of

resonances and relaxations.

PACS. 75.60Jp

Fine-partiale

systerns.

PACS. 73.40Gk

Tunnehng.

1. Introduction

The

tunneling properties

oi a

large quantum

electronic

spin

S have been

recently

studied in reierences

il-Si-

A

large

spin may

correspond

to the resultant spin oi a small ferro or

ferrimagnetic particle,

or to the resultant spin oi a well defined cluster oi 10-20 transition ions in the core oi a

big

organic

molecule;

such organic molecules can be

prepared

in

single crystal iorm,

with very weak interactions between different dusters

[6-8j.

The smallest

possible

such duster is a

single paramagnetic

ion diluted in a

diamagnetic

matrix. This case is

interesting

because it has been shown:

1) that the coherent

tunneling splitting

decreases

exponentially

with the number N oi atoms oi the duster

[1-4j,

and con be

expected

to be very small even for a iew atoms

(<

Hz for

"Mn12" (4, Si),

ii)

that the

couphng

oi the giant spin with a

large

number oi nuclear spins has a deletenous effect on

tunneling phenomena

[9j

[10]

[SI. In a

single paramagnetic ion,

the electronic

spin

is

appreciably coupled only

with its own nudear

spin

and these

problems

should not be

important.

(*) UJF-CNRS,

UA 08

g

Les

Éditions

de

Physique

1996

(3)

Note that the situation considered here differs somewhat irom that oi a small

antiierromagnetic particle,

where the

tunneling splitting

involves different mechanisms and is

distinctly larger iii il [12],

also [13] for the effect oi nuclear

spins).

Let us now retum to the

problem

oi interest here and [et us assume that the electronic

spin

is well described

by

a main axial Hamiltonian:

lis

"

-D'S) il)

with D' > 0.

(Note:

for Rare Earth

ions,

S should be

replaced by J.)

The lowest

eigenstate

oi

lis

is the doublet

[Sz

= +S >. In zero

longitudinal field,

and in the presence of tunnel

effect,

the

degeneracy

oi the doublet is

liited, giving

rise to a

symmetric

state

~~

and an

antisymmetric

state

~~:

separated by

an energy 2r

(the "tunnelling splitting"). Expressions

of 2r

corresponding

to

crystalline perturbations

with varions

symmetries (orthorhombic, tetragonal, etc.)

or to a

transverse

magnetic

field have been derived in references

[il

[3] [4]

[Si.

~~

and

~~

are

diamagnetic

states, but <

il~[Sz[~~ >#

0. Therefore EPR between

~~

and

~~

should be observable

by applying

a

radiofrequency

field

parallel

to Oz. Such

experiments

have been carried out

recently by

Awschalom et ai.

[14]

on

antiferromagnetic ferritin,

which is

a

large

molecule with a small

uncompensated

moment c~

@,

and for

which, apparently,

2r m

a few MHz

([14j, Fig. 3). However, tunnelling splittings

A e 2r m 10 30 GHz have

already

been observed in the

past

on the much

simpler

case of a terbium ion

(Tb~+,

J

=

6,

1=

3/2),

diluted in a

diamagnetic

matrix such as

yttrium ethylsulfate [4].

Because of the nuclear

spin I,

the EPR

signal

in zero external field is in fact

composed

of two lines

corresponding respectively

to

Iz

= M

=

+3/2

and

+1/2.

Formulas

corresponding

to the line

frequencies

and

intensities,

as well as data relative to the relaxation

times,

can be found in the book

by Abragam

and

Bleaney [15] (§5.3, §5.6, Fig. 10.5).

In the present

work,

this

analysis

is extended to the case of NMR and Môssbauer

techniques.

A few formulas valid for H

#

0

(H

m

r)

are first derived. It is then assumed for

simplicity

that H

=

0,

1e. that the nuclear

spin

is

only

submitted to a

magnetic hyperfine coupling:

7ii,f

=

Ajjlzsz (to

which a

lattice-type quadrupole coupling

q

(Ij @@j,

insensitive to the tunnel

effect,

may be added if

desired). Indeed,

if S

# 1/2,

as assumed

here, magnetic hyperfine

terms of the form

(Ai /2) (1+S-

+

I-S+)

have no matrix elements inside + S >.

In what

iollows,

we will therefore use the notation A instead of

Ai

j.

The formulas

previously

obtained are then used for

computing

the

irequencies

and line intensities

corresponding

to EPR and NMR

spectra

when 1

=

3/2,

and to a

simple

Môssbauer

~ transition

le

=

3/2

-

Ig

=

1/2.

Such transitions exist, for

example,

in

5~Fe

or

~~~Tm [16].

2. General Formulas

Let us start irom the Hamiltonian:

7i =

g~IBHSz

+

AI=Sz

+

r[S

><

-Si

+

ri

S ><

Si (3)

in which r is the

(usually

non

adjustable)

tunnel

parameter.

Let us assume that

Iz

= M. The

eigenvalue equation

Ieads to two energy Ievels:

EM

=

+/(g~IBHS

+

AMS)2

+ r2.

(4)

(4)

The

tunnelhng splitting:

2/(g~IBHS

+

AMS)2

+ r2

=

/(2g~IBHS

+

2AMS)2

+ A2

(5)

is in

agreement

with

equation (5.56)

oi

Abragam

and

Bleaney [15]

for an effective

spin

S

=

1/2,

and reduces to A e 2r when A

= H

= 0 as

expected.

Let us define:

~~~~~~~ (g~IBH/+ AMS)

~~~

in

which,

for

simplicity,

both numerator and denominator will be assumed to be

positive (see

Addendum at the end oi the

paper),

with:

cos(2ÙM

"

~~~~~

~ ~~~

sin(2ÙM)

" ~

(7)

~/(g~IBHS

+

AMS)2

+ r2

/(g~IBHS

+

AMS)2

+ r2

There are two

eigen

vectors

titi(M) ~2(M)

=

COS(ÙM)lS,

M > +

Sin(ÙM)1 S,

M > j~~

=

sin(ÙM)(S,

M > +

cos(ÙM)( S,

M >

The first one

corresponds

to E = +

/7

and the second one to E

=

fi

in

equation (4).

When

(g~IBHS

+

AM) SP,

2ÙM -

~,

and:

2

l~i(M) ~2(M)

-

[~~

>

[M

>, with

E~,M

" +r

-

[~~

>

[M

>, with

E~,M

" -r.

When

(g~IBHS

+

AM)

»

r,

2ÙM -

0,

and:

l~i(M) ~2(M)

-

[S,

M > with

Es,M

"

+g~IBHS

+ AMS

-

S,

M > with

E-s,M

"

-gIIBHS

AMS.

Finally

<

i~i(M)lszli~iim)

>

= <

1~21M)lSz14Î2(M)

>=

Scos(2ÙM) 19)

<iii(M)jSzj~2iM)>

=

-Ssinj2ÙM). (10j

From now on, it wiII assumed that H

= 0 and M > 0. Then

EM

"

E-M

"

+~ (ll)

tg(2ÙM)

"

~

,

cos(2ÙM)

" ~~~

,

sin(2ÙM)

= ~

(12)

AMS

~ ~'

There are two

degenerate

states with energy:

+~

~iimj

=

cosjÙmjis,

M > +

sin(Ùmjj S,

M >

iljj-Mj

~~~~

=

sinjÙmjjs,

-M > +

cosjÙm)j S,

-M >

and two

degenerate

states with energy:

-/r2

+

(AMS)2)

IÎÎÎÎ~Î)

=

ÎÎÎÎÎÎÎÎÎ ~ÎÎ~Î~ÎÎÎÎ)[ ~),~ÎÎÎ~

>

~~~~

It what

iollows,

it wiII be assumed that the

(irreversible)

relaxation rates between aII the

states of the

problem

are small

compared

to r and A. This is

obviously

necessary for the

observation of the

magnetic hyperfine

structure.

(5)

3.

Application

to EPR and NMR when 1=

3/2

It is assumed that the

hyperfine

Hamiltonian has the form:

~ ~~ ~

~~ iii

+

)j

hf =

z z + q

z ~

and that S

(or

J for

R-E-)

is

larger

than

1/2 (for example,

J

= 6 for

Tb~+ ).

For I

=

(,

the four

lowest electronuclear states are four doublets with the

following energies

and wave functions:

~

~

~ ~

4/i ((

= Cos

lÙ~/~) s,

+ sm

lô~/~) s,

~~~ ~~~~

~

~~ Î~

~~~ ~~~/~~

~'

~ ~°~ ~~~/~~

~'

~

~ 4/i ())

= Cos

lÙi/~) s, ))

+ sin

(ôi/~) s, ))

~~~ ~ ~' ~~~~

4/[ (-j)

= sin

lÙi/~) s, -))

+ Cos

(ôi/~) s, -))

~

~ 4/2 ())

= sin

lÙi/~) s, ))

+ Cos

(ôi/~) s, ))

~~~~ ~ ~~~~

~ ~~

~Î (~jj

COS

~~l/2) ~,

Sl~

(Ù1/2) ~,

~

~~

4/2

(~)

= sin

lÙ~/~) s, ()

+ Cos

(ô~/~)

s,

()

~~~~ ~ ~' ~~~~

4/i (- ()

= Cos

lÙ~/~) s,

sin

lô~/~) s,

3.1. E-P-R- SPECTRUM. It can be observed with an RF field

parallel

to Dz:

~RF

=

gpBHisz Cos(~Jt).

The hne intensities are

proportional

to

[sin(2ÙM

)]~

Line I

Transitions:

~2 ())

-

~i (() ~[ (-))

-

~[ (-)).

Intensity: II

~c

[sm

(2Ù~

/~)]~,

increases from 0 to 1 when r increases from 0 to cc.

Fi.equency: huI

=

2~,

increases from 3AS to 2r +

~

~~~~.

4 4 r

Line II

Transitions:

~2 ())

- lYi

())1 ~[ (-))

-

~[ (-)).

Intensity: III

c~

[sm (2Ùi /~)]~,

increases from 0 to 1 with r.

Frequency:

hVII

=

2~,

increases from AS to 2r +

~~~~

4 4 r

These two EPR fines haire been observed on

Tb~+

in

Y.E.S.,

as descnbed

by Abragam

and

Bleaney

[15]

(Section 5.3,

Section

5.6, Fig. 10.5).

The

experimental

EPR

frequencies

are:

huI

" 14.932

GHz, huII

= 12.018

GHz, correspond-

ing to a

tunnelhng splitting

A

= 2r

= 0.387 cm~l. The relaxation rate is the same for the two fines within the

experiniental

precision, and at the lowest measurement temperature K.

the relaxation time is about 25 ms.

(6)

3.2. NMR SPECTRUM. It can

only

be observed with a R-F- field

perpendicular

to Dz:

~RF

"

~"~"~~

(I+e~~~/~

+

I-e~~/~).

The fine intensities are

proportional

to the square of 2

the matrix element

of1+ (3

for -

~

,

4 for

- - +

).

2 2 2 2

Line 1:

Transitions:

~i (Î)

-

i~i (Î)liÎÎ (~')

~

~i (~Î).

Intensity:

~

~ ~ ~~~~ ~~~~~ ~~~~~~~ ~ ~

~2 +

~~~~~~~

1 ~2 s2

~

~~~~~

4 4

Vfhatever

r/AS,

this

quantity

never

departs

very much from 3.

Frequency:

hui

"

~-

A2S2 +

2q. (19b)

~2 s2

It varies from AS +

2q

to +

2q

when r increases from 0 to cc.

r Line 2:

Transitions:

q/ij 1j_q/ (lj~~~q/ jlj_q/ij 1j

21 § 2 § 1 ~à'

Intensity:

Ajs2

~~~~~

12 Cc 4 [COS

(2Ù1/2)1~

4 ~

~2 +

A(S~

It decreases from 4 to 0 when r increases from 0 to cc.

Frequency:

hu2

" 2 A2S2.

(20b)

It varies from AS to m 2r when r increases from 0 to cc.

Line 3:

Transitions:

~2 (Îj

~

~2 (1)

~~~

~~ ~~~)

~

~~ (~Îl'

Intensity:

same as that of fine 1.

Its

frequency

derives from

hui by

the

change: +2q

-

-2q.

~ÎOnCÎU310nT

. For r

=

0,

there are three fines with:

hui

" AS +

2q, hu2

"

AS, hu3

" AS

2q

and

intensities 3:4:3

(7)

. When r - cc,

hv2

C3

2r,

with

vamshing intensity,

and there remains

only

fines and

~2 s2 3,

with

intensity

3 and hu

= +

2q.

Line 2 and the

magnetic hyperfine

structure r

(h.f.s.)

of fines 1 and 3 are

suppressed by

the tunnel elfect.

4.

Application

to a Môssbauer Transition

3/2

-

1/2

The ~y transition is assumed to occur between an excited nuclear state

I~

= 3

/2

with a

hyperfine

Hamiltonian

~hf

"

AI]Sz

and a

ground

nuclear state

Ig

=

1/2

with

~hf

"

-BIfSz ii-e-

trie

order of trie levels in trie

ground

state is

inverted,

as in

5~Fe).

Trie energies and

eigenfunctions

of trie excited state with 1=

3/2

bave been

given

m trie

preceding

section. It will be assumed for

simplicity

that q

= 0. Let us define

~~~~~~~ BÎ~S' ~°~~~~~

r2

ÎÎÎMS)2

'

~~~~~~~ ~

~~~~

The nuclear

ground

state

gives

rise to trie two doublets:

~ ~

~ *2 1))

=

sin1~7i/~) s,

+ Cos

l~Ji/~) s,

~~~~ ~ ~~~~

~

~Î (~ jj

COS

(§~1/2) ~,

Sl~

~~'l/2) ~, ~j

~

~ ~i (j)

= Cos

1~7i/~) s,

+ sin

(~Ji/~) s,

~~~~ ~ ~

~[ (- j)

= sin

(~Ji/~) s, -j

~~~~

+ Cos

(~Ji/~) s, -)

For a

magnetic dipole

nuclear transition between two states a and

b,

and for a

powder,

trie

intensity

is:

Iab

ce

j<

a

§ >j~

+ < a

§

b

>

j~+ j< ai

Ml~ jb

>j~ 124)

where Ml is trie

magnetic dipole operator.

It is well known that for transitions between

eigenstates

of

I(

and

If,

trie intensities of trie allowed transitions are

proportional

to

3(3/2

-

1/2),2(1/2

-

1/2)

and

ii-1/2

-

1/2).

Here we will

only

consider trie transitions between trie vanous excited states and trie lowest

ground

state

Ah, 4l[ (first

half of trie

spectrum).

Trie second half of trie

spectrum

is

easily

deduced from it.

4.1. ASPECT OF THE

(HALF)

SPECTRUM

Line a

~~~~~~~~~~

4Îl (Î~

~

~1 (Î~' ~~ Î~

~

~~ Î~

Intensity:

~~~~~

~~~~~

~~~~~

~

~

~2~~ ~2~~~~2

+

~2 2~

~~~~~

(8)

It varies from 3 to 0 when r increases from 0 to cc.

Frequency:

h~ =

r2 + ~~2 s2 +

~(25b)

~

~

4

It varies from

)AS

+

)BS

to 2r +

) ~j~~

+

) ~j~~

Line b

~~~~~~~~~~

fl~~

())

-

~l (Î)Î

4~~

~~Îj

~

~~ ~~Î~'

Intensity:

(àCOS (Ùl

/2 §~l

/2)j

~

" Î + ~~

~~~ ~~~ ~~

l. (~~~)

~~~~ ~~ ~

Î~~~~

It varies from 2 to 0.

~~~~~~~~~

hub

"

~

~

~

~~~~~

~ ~

~~~~~~ ~~~~ ~s +

)

~S tO 2r +

) ~~~

~

Î ~é

Line ~y

~~~~~

4Îl (Î~

~

~~ ~~Î~' ~~ Î~

~

~l ~~Î~

Intensity:

~~~~~~~~~ ~ ~~~~~~

~

~2

~~~2~Î~~

~2 s2

l~~~~~

4

~

Always

near zero.

It varies from

)AS

+

)BS

to 2r +

) ~j~~

+

) ~i~~.

Line c

Transitions:

~l (~)

~

~~ ~~Îl' ~~ ~~Î~

~

~l ~~Î~'

Intensity:

[Cos

iôi/~

+

~Ji/~ii

2 = +

~~

l) j[ j)~ )[ [j~~~1.

128ai

~ ~

(9)

Always

near 1.

~~~~~~~~~

hUC "

~~~ ~

~~~~~

It varies from

-)AS

+

1BS

to

-1~~s2

~ i B2s2

Line

fl

Transitions:

~

jlj

_q/

jlj,~ij lj_q/ij lj

ii 2 à' 1~à 2

Intensity:

il

S1n (Ù1/2 ~71/2

Ii

~

" Î

l~

~~

~~ )~~~ ~

~

j

(~~~)

~ ~ ~ ~ ~ ~ ~i ~

4 4

It varies from 0 to 2.

Frequency:

hvp

= A2S2 + B2S2

=

hu~. (29b)

It varies from

)AS

+

1BS

to -1 A2s~

~ i B2s2

Line o

Transitions:

~l~~')~~2~~Îl'~~~~')~~~~ Î~'

Intensity:

~~~~~

~~~~~

~~~~~

~

~2~~ ~2~~~2 ~~2 2~

~~~~~

It varies from 0 to 3.

Frequency:

h~ = r2 + ~~2 s2 + r2 + f~2 s2

(30bj

°

~ ~'

It varies irom ~ As +

)Es

to ~

~~~~

+

~~~~

4.2. DIscussIoN

. For

arbitrary r/AS

trie half spectrum is

composed

of six fines a,

b,

~y, c,

fl,

a.

. Trie sum of trie fine intensities is

always equal

to

6,

as

expected.

. When r

=

0,

trie half

spectrum

is

composed

of three fines a,

b,

c with

respective

ire-

quencies hv~

=

~

AS +

BS, hvb

" AS +

BS, hv~

= AS +

BS,

and

respective

2 2 2 2 2 2

mtensities

3, 2,

1

(this

is trie standard Zeeman

case).

(10)

. When r m

AS,

BS

ii-e- (r/h)

m 50 MHz for

5~Fe,

m

10~

10~ MHz for

R-E-).

there are three fines a,

b,

~y, with hu m 2r and

vanishing intensities,

there are three fines c,

fl,

a, with

respective frequencies hu~

=

hup

= ~ ~ +

~ ~ ~

~ ~ ~ ~

8

Î~

8

Î~

and

hua

=

-~

~ ~

+

~ ~

,

and with

respective

intensities

1, 2,

3. In

practice,

8 r 8 r

since uc

= up the

(half) spectrum

is

composed

of two

equal

fines with

intensity 3,

at

frequencies

u~ and va

(note

that if A m

B,

va <

0).

Upon turning

no~v to the whole

spectrum,

it appears that when r increases from 0 to cc, its

aspect changes

from the standard six fine

spectrum

: a,

b,

c,

c', b', a',

with fuit

magnetic hyperfine

structure and intensities 3 : 2 1 1 2

3,

to a four fine

spectrum (c+fl),

a,

a', (c'+fl')

with shrinked

magnetic hyperfine

structure and

equal

intensities 3.

In other

words,

the tunnel elfect suppresses the

magnetic

h-f-s-. Note in

passing

that in the presence of a lattice

type quadrupole coupling,

and whatever

r,

fines a,

a',

a, a' will be shifted

by

+q, and fines

b, b',

~y, ~y', c,

c', fl, fl' by

-q.

There exists a

simple explanation

for the suppression of the

magnetic

h-f-s-- Let us con- sider for

example

the case 1

=

3/2 (NMR

or excited Môssbauer

state).

ivhen r - cc, the

eight eigenstates

give rise to two electronuclear

quadruplets )~~

>

(M

> and

(~a

>

iii

>

(M

=

+), +)), separated by

2r. The electronic states

)~~

> and

)~a

>

being diamagnetic,

these

quadruplets

have no first order

magnetic hyperfine

structure. However there is a

magnetic hyperfine

contribution to second

order, giving

rise to foui- doublets:

)~~

> +

3/2

> :

E~

= r +

~

~/ (31)

~2 s2 )~~

> +

l/2

>

:

E(

= r +

(32)

1

~2 s2 )~a

>

+1/2

>

E[

= -r

(33)

)~a

> +

3/2

>

Ea

= -r ~ ~ ~

(34)

Since there exists no nuclear matrix elements between

)~~

> and

)~a

>, this enables to

explam

the NMR

spectra (disappearance

of one

hne) and,

after extension to the Môssbauer

ground

state, the presence of four Môssbauer fines with

equal

intensities. This last

phenomenon

has a little

analogy

with trie mechanism of the

pseudoquadrupole

interaction invoked for ex-

plaining

the

quadrupole

spectra

of169Tm

in

TmC13 6H20 ([16] §3.10

and

Fig. 3.9,

and ii. ii

).

Note that conclusions similar to those of the

present

paper were derived a

long

time ago for

an

analogous problem Ii?i (valence quadrupolar

structure of Môssbauer spectra in the presence of Jahn-Teller

tunnelling

between two

wells).

At first

sight,

it does not seem very easy to find favorable cases for the Môssbauer obser- vation of the

shrinking

of the

magnetic hyperfine

structure due to

tunnelling

elfects.

~5~Tb

is

unfortunately

net a Môssbauer

isotope. 169Tm

is one, and

Tm~+

has J

= 6 as

Tb~+;

how~

ever, smce the second order Stevens coefficients

o j of

Tb~+

and

Tm~+

are opposite, whenever

Tb~+

has a

)Jz

= +6 >

ground

doublet

[4], Tm~+

will

probably

have a

singlet (or

at least

unfavorable) ground

state.

In orgamc or

biological compounds [18],

there exist

examples

of ferric ions

5~Fe~+ (S

=

5/2)

with

large

spm Hamiltonians ~

=

-D'S]

and

ground

state doublets

)Sz

=

+5/2

>.

(11)

However,

for Kramers ions

[4], tunnelling splittings

can

only

be induced

by application

of a

transverse

magnetic

field

Hi,

with r c~

HfS

c~

H[,

which is net very convenient. The same

remark

applies

to

~6~Dy~+,

J =

15/2,

whence r c~ H

(5

for the

ground

doublets

)Jz

=

+15/2

>

observed in some

compounds

[16] Tab.

17.8),

at least if trie level scheme is well

represented by ~o

=

-D'J],

which is seldom trie case in R-E-

compounds

[4]. This is

elfectively

net trie

case for

l~°Yb~+,

J

=

7/2,

in

yttrium ethylsulfate,

in which it bas a

ground

state doublet

)Jz

=

+3/2

>: for

predicting

trie variation of r with

Hi,

it will be necessary to use the exact

level scheme and wave functions

(which

are

fairly

well known

[19]).

In

Fe++

ions

(S

=

2),

there is an

important

orbital contribution to trie

magnetic hyperfine

structure

[20] [21].

In

addition,

relaxation between orbital states is

usually

very fast. There

are a few cases of slow

relaxation,

but

apparently

without

tunnelling splitting

in trie

ground

state

[22].

5. Conclusion

The elfect of a coherent tunnel elfect on trie

magnetic hyperfine

structure of a

single

ion,

observed

by EPR,

NMR and Môssbauer

spectroscopies

bas been studied in zero

longitudinal

field.

Explicit expressions

for trie fine

frequencies

and intensities bave been derived in the

case of EPR and NMR experiments

involving

a nuclear

spin

1 =

3/2,

and for a Môssbauer transition

Ie

=

3/2

-

Ig

=

1/2.

Predictions relative to EPR had

already

been made and checked a

long

time ago for

Tb~+

in

yttrium ethylsulfate, although

the name "tunnel elfect"

was not used at that time. The

present

paper

mainly

surveys the

opportunities provided by

Môssbauer

spectroscopy

for

observing

the

"shrinking"

of the

magnetic hyperfine

structure due to the coherent tunnel elfect.

A summary of these results has been

presented

as a post deadline poster at the International Conference on the

Applications

of the Môssbauer

Elfect,

I.C.A.M.E.

1995,

Rimini

(Italy), September

1995.

Acknowledgments

The author is indebted to Drs P. IMBERT and P. BONVILLE for useful discussions about

tunneling phenomena.

Addendum

In reference [4] of the present paper, for orthorhombic

symmetry

and

integer S,

the

tunnehng splitting

2r is due to the term

~(S(

+

S~

e

2~(Sj S))

in

equation il

of [4]. r is given

by equation

là of [4] for even

S,

r is

always negative

and the

symmetric

state ~~~ ~

~~

~

~~

is

lowest;

for odd

S,

r has the

sign

of

~~

i-e- trie

sign

of ~. However when ~ < 0 trie easy axis in trie hard

plane

is

Dz,

but when ~ >

0,

the easy axis is

Oy;

if Dz is chosen as the easy axis

in the hard

plane,

one must take ~ <

0;

then r is

always negative

and the

symmetric

state is lowest whatever the

parity

of S.

Similarly,

in the

tetragonal

case, trie

tunnehng splitting

is due to trie term

u(S(

+

S~

in

equation (58)

of [4]; this term is trie

"operator equivalent"

of the classical

quantity 2u(S]

6SjS(

+

S().

For Dz or

Oy

to be easy axes m the hard

plane,

it is necessary to take u < 0.

If u >

0,

trie easy axes are

[l10][lÎ0].

r is

given by equation (59)

of [4]. When S =

4n,

r

(12)

is

negative

whatever trie

sign

of u. When S

= 4n + 2 and u <

0,

r is aise

negative

and the

symmetric

state is lowest in bath cases.

Similar discussions should also be carried out in the

trigonal

and

hexagonal

cases.

In the present paper, we have taken r > 0 for

simplifying

the

correspondence

between square root solutions such as

equation (4)

and their limits when A

= H

= 0. As shown

above,

this may

correspond

to

taking

for Dz the hard axis in the hard

plane. Anyhow,

whatever the

sign

of

r,

the

physics

and the conclusions are the same.

References

iii

Scharf

G.,

Wrezinski W-F- and Van Hemmen

J-L-,

J.

Phys.

A

(London)

Math. Gen. 20

(1987)

4309 and references therein.

[2]

Chudnovsky

E-M- and Di Vicenzo

E-P-, Phys.

Re~. B 48

(1993)

10548 and references therein.

[3] Politi

P.,

Rettori

A.,

Hartmann-Boutron F. and Villain

J., Phys.

Re~. Lett. 75

(1995)

537.

[4] Hartmann-Boutron

F.,

J.

Phys.

I France 5

(1995)

1281. In that paper, the R-H-S- of

equation (5)

should read:

~/~.

Additional

precisions

relative to this work

[5] artmann-Boutron F., Politi P. andVillain

J.,

Int.

lication).

[6]

I?i Sessoh R.,

Gatteschi D., aneschi A.

and

Novak

[8] Gatteschi

D.,

Caneschi

A.,

Pardi L. and Sessoli

R.,

Science 265

(1994)

1054.

[9] Garg

A.,

Phys. Re~. Lett. 70 (1993) 1541.

[loi Prokof'ev N-V-

and

Stamp P-C-E-, J.

Phys.

Condensed

il

ii Barbara B.

and

Chudnosky -M-,

Phys.

Lett. A

205.

12]rive I.V. and Zalavskii

O.B., J. Phys.

Condensed att.

2

(1990)

[13]

Garg A., Phys. Re~.

Lett.

74

(1995)

1458.

[14] Gider S.,

Awschalom D.D-, Douglas T.,

Mann

S.

77,

(7

April 1995),

and references

herein.

il 5]

Abragam

A.

and Bleaney B.,

on

ress,

Oxford

970).

[16] Greenwood N-N-

and

1971).

Il?I

[18]

Wickman H.H. and Wagner C.F., J.

Chem.

Phys.

[19]

Borely C., nzalez-Jimenez

F.,

Imbert P. and

Varret

F.,

J.

Phys.

605.

Borely C.,

Thesis Orsay 1974).

[20] artmann-Boutron

F.

and

Imbert P.,

[21]

Varret F., J. Phys. rance 37

Coll C6

(1976

)

437

[22]

Price D.C., ohnson

C.E.

and aartense I., J.

Phys.

. Soiid

State Phys. 10

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