Absorption intensity analysis of Pr3+: Y3Al5O12

Absorption intensity analysis of Pr3+: Y3Al5O12

Solid State Communications, Printed in Great Britain. ABSORPTION Vol. 74, No. 1, INTENSITY pp. 17-20, ANALYSIS 1990. OF 00x3-1098/90$3.00+...

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Solid State Communications, Printed in Great Britain.

ABSORPTION

Vol.

74,

No.

1,

INTENSITY

pp.

17-20,

ANALYSIS

1990.

OF

00x3-1098/90$3.00+.00 Pergamon Press

plc

Pr3+: Y3A15012

M.Malinowski, R.Wolski and W.Woliieki Institute of Microelectronics and Optoelectronics ul. Koszykora 75, (Received19 The

intensity

00-662 Warsaw,

Poland

December 1989 by M.Balkanski) studies

of

the

optical

absorption

spectra of Pr3+ ions in Y3A15012 crystal are presented. Oscillator

strengths

of

f-f

Pr3+ transitions,

radiative lifetimes, fluorescence branching ratios, and Ot

intensity parameters

have been

calculated

and the

obtained results are compared witch the data reported for other host materials.

I .T.M.E. the Czochraleki method at room laboratory in Warsaw. The temperature abeorption epectrum, over 13 mm optical path length in the crystal, wa6 recorded by a Beckman WV 5270 spectrophotometer. Hmieeion epectra to the experimental leading the branching ratio0 determonation of ion laser argon were recorded under excitation at X - 488 run. The room temperature abeorption epectrum of the Pr3+: YAG have been agalyeed using the treatment of Judd and 0felt.7 of the etatic In this model coupling between the radiation field and the electronic charge dietribution of ligands, the oecillator etrength f of the electric dipole f-f traneltion of RE3+ is expreesed aa a eum of phenomenological inteneity parametere Rt and reduced matrix 8 lemente of tensor operators Ut of a rank t of the form

Trivalent rare earth lone (RE3+l doped yttrium aluminum garnet, Y3A15012 (YAG) have been exteneively studied during the last decade. Because Nd3+: YAG ie the meet ;uccesful solid &ate it attracted moet laser material attention and much lees ie known about f luoreecence of other RE3+ ions in thie cryetal. The optical spectrum of 2Pr3+: YAG hae been studied since 1963 but only recently a good deal of physical and spectroscopic data of thie magef;ijl are reported in the literature ’ ’ . However, to our knowledge, there has never been a complete of the analysis absorption line intensity of Pr3+: YAG, although eimllar calculations baeed on Judd-Ofelt approach 6D7 been have reporte; gf;t; praaeodymlum In other ho&e. ’ ’ In this study. we have presented calculations absorption inteneity leading to determination of the ot parameter8 that occur in the Judd-Ofelt radiative theory, the excited etate lifetime6 and branching ratios. We found also Interesting to compare our concerning other reeul:e Pr thoae with containing hoets with relation to the structure and point different crystal RH3+ ion. Thie ie ale0 symaetry of 1aser important because of potential applications of Pr3+: YAG cry&ale. crystal of A good quality single Y3A15012: 0.12 at.% Pr3+ was obtained by

f(aJ,bJ’l

8B2mcX - 3(2J+l)h

&1<4f”[dSL]JI t

1 x ’

lUtl 14fn[d’S’L’lJ’>12

(1)

where 5 is the average wavelength of the local field transition and I! ie the correction which for electric dipole transitions ie approximated by (n(h) 2t2) 2/9n(S1 . The spontaneoue emieeion probabilitiee A 17

18

ABSORPTION INTENSITY ANALYSIS OF Pr3+: Y3A150,2

in terms of above oscillator are calculated from

A(aJ,bJ’l

-

gl12Xe2n2

-zX-

f (aJ,bJ’l

strengths

(21

Since the details of this theory, its been precision and draw ;a,ckfo have analysed elsewhere * ’ we have presented here only essential the formulas. Because the 41 wave functions, due to the shielding by the outlying 5s and SP shells, retain much of their free ion character the
Table 1. Measured strengths

and for

calculated Pr

manif old

osci 1 lator

: YAQ

x

SLJ

Vol. 74, No. 1

f

f talc

exp

x 106

tnml

x 106 A

27.56

8.28

470

15.58

12.85

13.6

488

6.83

8.79

9.08

600

6.35

2.46

2.30

1030

0.50

0.69

0.58

1400

5.68

7.81

6.79

1500

14.91

14.88

13.72

1850

5.63

6.45

6.51

2315

1.

A: RMS dev-7.7 10-20cm2,

10

10B6

Q6-9.20

B: RMS dev-2.4

-20,,2

B

452

1.36 R2-0.

Q4-

11.78

“4’

12.20

10-20cm2

10e6

n2-0.

, R6-8. 27 10-20cm2

with the measured fluorescence lifetimes which are; xf - 8.8 CIS for 3Pl, 7f - 8.4 ps for

3Po and ~~ -

180 vs for

‘D2 state

In 1% Pr3+: YAG at 300 K. The nonradiative transition probabilities to the next lower lying levelT4are governed by the energy gap law, euggeeting thus more eff lclent nonradiative deexcltation in the case of YAG then LiYP4 crystal. This is probabely also the main reason of the great differences in the observed fluorescence lifetimes in thie two materials. Room temperature emission of Pr3+ ions in YAG , after c.w. 1aser argon excitation at X - 488 nm, is dominated by the very strong fluorescence from the state to the sound 3H4 lD2 excited state. The 3Po emission line intensities were too weak to perform precise measurementa. The experimental values of branching ratios for transitions from the excited ‘D2 state are presented in Table 2 together with the calculated values. observed that It could be

Vol. lh, No. 1

ABSORPTION INTENSITY ANALYSIS OF Pr3+: Y3A150,*

Table

2.

Calculated the

3P1,

ratios Final

radiative

transition

3P0 and ‘D2

P for

the

levels

probabilities

and calculated

Initial

etate

k [nml

3po

A[s%

17689

branching

state lD2

X[nml 0

X[nml

A[& _

-

Ah-‘1 _

P

talc

P

exp

-

2371

0

2739

0

-

lG4

904

1372

953

2373

1470

357

0.07

-

3P4

714

1336

745

14454

1023

146

0.03

0.02

3P3

689

10235

718

0

972

177

0.03

0.03

3P2

632

0

656

0

862

1232

0.24

0.15

3H6

611

6314

633

11709

823

1212

0.24

0.30

Rs

540

37790

557

0

700

62

0.01

0.05

3R4

485

26578

499

610

1854

0.37

0.45

parameter6

Qt

Us

69086 ZR- 10.2

[1O-2o

cm21

laser

crystals.

Pr3+

Material

of

Nd3+

‘2

‘4

‘6

‘2

‘4

‘6

YAL03 ”

2

6

7

1.3

4.7

5.9

LaP3 I3

0.12

1.77

4.78

0.35

2.57

2.5

4.88

8.55

5.25

2.9

8.07

7.32

1.9

2.7

5

12.20

8.27

0.

2.7

5

17.2

LiYF4B ’ ’ O0 YAG ’

YAG for

D2

some Pr3+ and Nd3+ doped

l3

Pr3+:

and measured

3P0

ZR- 11.9

‘2’3

A of

‘D2 emission.

3Pl

Table 3. Intensity

19

0 this

19.8

work

agreement between theory and experiment Thie could be explained in is poor. selective terms of the observed, under laser excitation, multieite luminescence from regular and perturbed Pr3+ ions characterised the different by transition probabilities. compares Table 3. parameters Gt

pe

TR- 198 ps

determined for several Pr3+ and Nd3+ laser hosts. As in the case of Nd3+ ion, the R4 and R6 in LiYP4 and YAG doped

have also similar values for Pr3+. The discrepancies observed for R2 in Nd3+ doped crystals are probabely due to different site synnnetry of Re3+ ion which is S4 in LiYP4 and D2 in YAG. In comparing the fit of Pr3+: YAG with those of other hosts it is seen that Q4 has relatively large value when R6 parameter ia in agreement with this of YA103, concentrated LiYP4 and praseodymium phosphates.” In conclusion, based on the absorption intensity analysis, we have pgsented several spectroscopic data on Pr : YAG. Thie can be useful in further studies of this interesting earth doped rare crystal which could be also an efficient laser material. We wish to thank Dr 2. Frukacz, ITME growing the crystal of Warsaw, for YAG:Pr3+. This work wa8 supported by the CPBR 8.14 program.

20

ABSORPTION INTENSITY ANALYSIS OF Pr3+: Y3A150,2

Vol. 74, No. 1

R8f@rMiCOB.

Danielmsysr in "Laser@" ed. Levine and A.J. DeMaria (Marcel Dekker, Inc. N.Y. and Baael 1976)

1. H.G. A.K.

P.1

2. E.Y. O.M.Stafsudd and Wow. D.R.Johnston. J.Chem.Phye. 39, 786 (1963). 3. E.Antic-Fidancev, M.Lemaitre-Blalee and P.Caro, Inorg.Chim. Acts 139, 281 (1987). 4 O.L.Malta, E.Antlc-Fidancev, M.Lemaitre-Blaiae, J.Dexpert-Ghye Chem.Phys.Lett. and B.Pirlou, 183, 557 (1986). 5. J.B.Gruber, M.E.Hills, R.M.Macfarlane C.A.Morrison and G.A.Turner, Chem.Phys. 139, 24 (1989). 6. B.R.Judd, Phys.Rev. 187, 750 (1962). 7. G.S.Ofelt, J.Chem.Phys. 37, 511 (1962) 8. C.A.Morrieon and R.P.Leavitt in "Handbook on the Physic6 and Chemistry of Rare Earth" vol 5.

ed. K.A.Gschneidner Jr and L,!Eyring (North-HollandPubl.Co 1982) e.461 9. M.Malinowski, R.Wolski and W.Wolifiski J.Lumln.35, 1 (1986). 10. J.L.Adam, W.A.Sibley, and D.R.Gabbe, J.Lumin.33, 391 (1985). 11. M.J.Weber, J.Chem.Phys. 48, 4774 (1968). 12. M.J.Wsber, T.E.Varltlmos and B.H. Matsinger, Phy8.Rev.B 9, 47 (1973). 13. W.F.Krupke, Phys.REv, 145, 325 (1966). Laser 14. H.P.Jenssen, "Phonon Assisted Transitions and Energy Transfer in RE Laser Cry&ale" Crystal Physics Lab. Tech.Rep. No 16, MIT, Cambridge, Mass. 1971 15. M.Mallnowskl, Proc. 1st Int.SymP. on Rare Earth Spectroscopy, WrocZaw. ed. B.Je*owska-Trzebiatowska, J.Legendziewicz and W.Str?k (World Scientific Publ.Co Singapore 1985) P.348