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Optical characterization of Er3+and Yb3+ co-doped barium ...

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furnace at 750 1C for 2 h in platinum crucible and the molten glass<br />

was stirred intermittently to achieve homogeneity. The melt was<br />

then cast onto a preheated (250 1C) carbon mold. The glass disks<br />

thus obtained were annealed at 250 1C for 12 h to avoid undesirable<br />

thermal stresses. The samples were then polished to optical<br />

quality and only bubble and streak free samples <strong>of</strong> thickness<br />

0.2 cm were taken for optical measurements.<br />

The density <strong>of</strong> the sample was measured by Archimedes’s<br />

principle and found to be 5.679 g/cm 3 and the calculated number<br />

density <strong>of</strong> the Er 3 þ ion in the glass were found to be 4.02<br />

10 20 ions/cm 3 .<br />

2.2. <strong>Optical</strong> measurements<br />

The refractive index were measured at five different wavelengths<br />

(473 nm, 532 nm, 632.8 nm, 1060 nm and 1552 nm) on<br />

Metri<strong>co</strong>n M2010 Prism Coupler equipped with respective laser<br />

sources and the obtained values were fitted to Sellmeier’s<br />

dispersion equation to obtain wavelength dependent refractive<br />

index. The absorption spectra were measured in the 300–1700 nm<br />

range using a spectrophotometer (Cary, Model 14R) in the<br />

transmission mode. The NIR emission spectra and fluorescence<br />

decay kinetics <strong>of</strong> the samples were re<strong>co</strong>rded on spectr<strong>of</strong>luorimeter<br />

(Model: Quantum Master enhanced NIR, PTI, USA) fitted<br />

with double monochromators on both excitation and emission<br />

channels. The instrument was equipped with liquid N 2 <strong>co</strong>oled<br />

gated NIR photo-multiplier tube (Model: NIR-PMT-R 1.7, Hamamatsu)<br />

as detector for acquiring both steady state spectra and<br />

phosphorescence decay. For decay measurements, a 60 W Xenon<br />

flash lamp was employed as an excitation source. The up<strong>co</strong>nversion<br />

luminescence spectra <strong>of</strong> the glass were re<strong>co</strong>rded in the above<br />

mentioned spectr<strong>of</strong>luorimeter using a 980 nm fiber pig-tailed<br />

diode laser with variable output power up to a maximum <strong>of</strong><br />

200 mW (Thorlab, USA) as an excitation source. For quantum<br />

yield measurements, the emission spectra <strong>of</strong> the samples were<br />

re<strong>co</strong>rded by exciting the sample with 980 nm band <strong>of</strong> a Ti–S laser<br />

(Spectra Physics, Model 3900S) pumped by an Nd:YAG laser<br />

(Spectra Physics, Model Millennia) and 488 nm band <strong>of</strong> an<br />

Ar-ion laser (Spectra Physics, Model 2500). The up<strong>co</strong>nversion<br />

and the visible emission from the sample were focused onto a<br />

photo multiplier tube (Model 1911, Horiba) and scanned using a<br />

1200 grooves/mm diffraction grating blazed at 0.5 mm, with a<br />

spectral resolution <strong>of</strong> 0.01 nm. The detector signal was processed<br />

in a PC <strong>co</strong>upled to the data acquisition system through a lock in<br />

amplifier (Stanford Research System, Model SR510). The entire<br />

system was <strong>co</strong>ntrolled through the data acquisition s<strong>of</strong>tware<br />

Snerjy (Origin Lab, and Jobin Yvon). All the emissions and decay<br />

time measurements were performed at room temperature. The<br />

FTIR vibrational spectrum was measured on the solid sample in<br />

the transmission mode using the FTIR spectrometer (Bruker,<br />

Model vector 22).<br />

3. Results<br />

3.1. Judd–Ofelt (JO) parameters<br />

The room temperature UV–vis–NIR absorption spectra <strong>of</strong> the<br />

sample are shown in Fig. 1(a) and (b) with their spectral band<br />

assignments. In calculating the absorption <strong>co</strong>efficients, the scattering<br />

losses have been subtracted in all absorption measurements.<br />

The broadening <strong>of</strong> the absorption bands is a <strong>co</strong>nsequence<br />

<strong>of</strong> the absence <strong>of</strong> long range order in the host producing changes<br />

in the micro-symmetry around the Er 3 þ ion. It was found that<br />

all absorption bands <strong>of</strong> Er 3 þ in fluorotellurite glass is similar<br />

to those <strong>of</strong> previously reported tellurite glass hosts [19–21].<br />

M. Pokhrel et al. / Journal <strong>of</strong> Luminescence 132 (2012) 1910–1916 1911<br />

Abs. Coeff. (cm -1 )<br />

Abs. Coeff. (cm -1 )<br />

6<br />

3<br />

0<br />

3.0<br />

1.5<br />

0.0<br />

4 G9/2+ 4 G 11/2<br />

4 F5/2<br />

4 F3/2<br />

2 G9/2<br />

4 F7/2<br />

2 H11/2<br />

4 S3/2<br />

4 F9/2<br />

400 450 500 550 600 650 700<br />

Wavelength (nm)<br />

4 I9/2<br />

4 I11/2 (Er 3+ )+ 2 F 5/2 (Yb 3+ )<br />

800 1000 1200 1400 1600<br />

Wavelength(nm)<br />

4 I13/2<br />

Fig. 1. Room temperature absorption spectra <strong>of</strong> Er 3þ in Er 3þ /Yb 3þ <strong>co</strong>-<strong>doped</strong><br />

glass, 1(a) ranging from 350 to 700 nm, 1(b) ranging from 700 to 1650 nm<br />

including Yb 3þ ( 2 F7/2- 2 F5/2) transition at 980 nm.<br />

Table 1<br />

Measured and calculated absorption line strengths <strong>of</strong> Er 3þ in Er 3 þ /Yb 3þ <strong>co</strong>-<strong>doped</strong><br />

(Ba,La)-tellurite glass at 300 K.<br />

4 I15/2- k (nm) S meas<br />

ed (10 –20 cm 2 ) S cal<br />

ed (10–20 cm 2 )<br />

4 I13/2 1532 2.0121 2.2836<br />

4 I9/2 800 0.2452 0.2978<br />

4 F9/2 654 1.4445 1.5151<br />

4 S3/2 546 0.2088 0.3049<br />

4 H11/2 522 5.2190 5.0589<br />

4 F7/2 490 0.6235 1.1052<br />

4 F5/2 452 0.1303 0.3078<br />

4 F3/2 444 0.0138 0.1754<br />

( 2 G, 4 F, 2 H)9/2 408 0.1603 0.3422<br />

4 G11/2 380 6.3243 6.5085<br />

Twelve absorption bands were identified in the room temperature<br />

absorption spectra between 300 and 1600 nm, shown in<br />

Fig. 1(a) and (b) and are tabulated in Table 1. These absorption<br />

bands were chosen to determine the phenomenological Judd–<br />

Ofelt parameters [22–26] for Er 3 þ in Er 3 þ /Yb 3 þ <strong>doped</strong> fluorotellurite<br />

glass. The JO parameters obtained for the Er 3þ in the present<br />

glassy system are O 2¼5.97 10 20 70.3 cm 2 , O 4¼1.64 10 –<br />

20 70.10 cm 2 ,andO6¼1.38 10 –20 70.067 cm 2 . These values are<br />

in excellent agreement with the values reported earlier for many<br />

tellurite glassy hosts [20,21,27,28] within the relative error <strong>of</strong> fit and<br />

falls at the lower end <strong>of</strong> the range 5–25%, as obtained by the<br />

application <strong>of</strong> the JO theory to other laser materials [22,23,29,30].<br />

Using these phenomenological JO parameters, the emission<br />

line strengths <strong>co</strong>rresponding to the transitions from the upper

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