New Physics: Sae Mulli,
Vol. 65, No. 9, September 2015, pp. 868∼872
DOI: 10.3938/NPSM.65.868
Formation and Photoluminescence of BaO2 -TiO2 -Strontium nitrate:Eu3+
Powders Fabricated by Using Mechanical Alloying
Hyun-Goo Kim∗
Department of Physics Education, Chosun University, Gwangju 61452, Korea
(Received 18 June 2015 : revised 22 July 2015 : accepted 28 July 2015)
BaO2 -TiO2 -Strontium nitrate:Eu3+ powders were synthesized by using the planetary ball mill
(PBM) method, and their structural and photoluminescent characteristics were investigated by
using X-ray diffractometry (XRD), thermogravimetric/differential thermal analyses (TG/DTA),
and an Ocean Optics USB2000 spectrometer. The crystallite size of the resultant powder milled
for 600 minutes (min) by using the Willaimson-Hall method, was approximately 74.1 nm with a
strain of 6.01 × 10−3 . The maximum dissolution temperature, the transition temperature, and the
total percent weight reduction of the sample powders were 604.1 ◦ C, about 525.7 ◦ C, and 29.22%,
respectively. Furthermore, the photoluminescence peaks of the powder mixtures were detected
near 578 nm, 591 nm, 615.5 nm, and 666 nm, respectively. The highest luminescence intensity of
the powder mixture was observed for the samples with Eu = 10 mole%. Peaks of Sr2 TiO4 and
(Ba1.5 Sr0.5 )TiO4 were observed in samples annealed at a temperature of 800 ◦ C for 1 h.
PACS numbers: 81.20.Ev
Keywords: Planetary ball mill, BaO2 -TiO2 -Strontium nitrate:Eu3+ , Williamson-Hall method, Scherrer
method
4
M
X
Ä
ì
¥
¶
?0
£
É;
n
c8
ý
¢ BaO2 -TiO2 -Strontium nitrate: Eu3+ ¶
X
¥V
ËÄ
R
Ø
Z
o8
ý]
ùV
k
Ëõ
R
Í
m
Ñ®
Ë
°
o°
Ñ
Ë
¤V
Ë
R
»g̀
@¦
∗
¸
@
/
Æ
<
§ Ó
to
ü
§¹
¤õ
¢
, F
gÅ
Ò 61452
(2015¸
6
4 18{
Z
~
9
Î6
Ã
§, 2015¸
£
7
4 22{
Z
Ã
9
º&
ñ
r~
:
Î6
Ã
§, 2015¸
£
7
4 28{
Z
>
9
F
S
&
X
)
ñ
BaO2 -TiO2 -Strontium nitrate: Eu3+ ½
Ë$
+
ì
í
rú́
`
¦ PBM ~
ÓZ
½
`
O
¦s
6
x
#
©
r\
:
"
f]
j
%
Ü
i
¼9,
¨
½
¸
9F
x
gµ
ÏF
1
g:
¤$
£
`
í
¦
¸
l
0
AK
X-ray diffractometry (XRD), thermogravimetric/differential
thermal analysis (TG/DTA), Õ
ªo
¦ Ocean Optics USB2000 spectrometer\
¦s
6
x
%
i
. 600ì
rx
9
Aô
a
Ç
r«
Ñì
rú́
`
¦ Williamson-Hall ~
ÓZ
½
`
O
¦s
6
x
#
½
¨ô
Ç
&
ß
ñ
¼l
H
74.1 nm,
+
AÖ
þ
¦
r
É
6.01
× 10−3 s
%
3
. þ
j@
/ì
rK
r
:
¸
H 604.1 ◦ C,
s
r
r
:
¸
H
525.7 ◦ Ce
`
¦·
Ã
ú
ºe
%
Ü
3
¼9, 8
xÁ
ú
º
>
y
èÖ
¦
r 29.22%s
É
%
3
.
527.0 ◦ C\
"
f
626.5 ◦ C
t
_
Á
º>
y
èÖ
¦s
^
y
èÖ
¦_
83.2%
Ð
ß
©
¼>
z
`
¦·
Ã
ú
ºe
3
%
. Eu\
¦ 10 mol% '
Ù
¡`
þ
¦
Ä
â
ºµ
ÏF
1
gy
©
¸
Z
©
}6
§`
£
¦
º
ú
·
Ãe
%
Ü
3
¼9, @
/^
&
Ü
h
¼
Ð 578 nm, 591 nm, 615.5 nm, 666 nm, Õ
ªo
¦ 698 nm
н
¨$
÷
í
&%
3
. 800
◦
C\
"
f1h1
xî
l
\
ß
%
P
o
ô
Çr
«
Ñ[
t\
þ
"
f
H Sr2 TiO4 ü
< (Ba1.5 Sr0.5 )TiO4 x
ß
¼[
ts
þ
8
¤&
£
÷
ñ
&%
3
.
This is an Open Access article distributed under the terms of the Creative Commons Attribution Non-Commercial License
(http://creativecommons.org/licenses/by-nc/3.0) which permits unrestricted non-commercial use, distribution, and reproduction in
any medium, provided the original work is properly cited.
Formation and Photoluminescence of BaO2 -TiO2 -Strontium nitrate:Eu3+ Powders Fabricated by · · · – Hyun-Goo Kim
869
PACS numbers: 81.20.Ev
Keywords: Ä
»
+
A^
þ
¦x
, BaO2 -TiO2 -Strontium nitrate:Eu3+ , Williamson-Hall ~
9
ÓZ
½
, Scherrer ~
O
ÓZ
½
O
I. "
eÂ
Ø
]
>
l
&
h
½
ËF
+
K (mechanical alloying) [1–3] ~
ÓZ
½
O
r É
H
í
ºô
Ã
Ç
&
ì
ñ
rú́
`
¦¶
"
é
H
¸$
õ
í
¸ß
¼l
_
&
x
ñ
q
9
|
ñ
&
F
9
K5
q½
Å
ËF
+
K1
xÜ
p
¼
н
Ë$
+
í
HD
h
Ðî
rl
Õ
t
ü
Ð+
Koch
x [4]\
p
1
_
K
Ni60 Nb40 F
K5
qÄ
Å
»o
_
]
j
\
6
x6
£
x÷
&%
3
.
AF
þ
+
g^
(luminescent material)
H#
Q:
¤&
£
+
ñ
AI
þ
_
\
-t
\
¦ f
¨Ã
º
#
\
4
P
¤
l
4
¤
Ð \
-t
\
¦ ~
Ó
½
¦
Ø
HÓ
t|
ü
s
9
9, +
AF
þ
g^
\
_
K
~
ÓØ
½
¦
a
)
l
4
¤
II. ÷
ÇM
m
ö
]
BaO2 -TiO2 -Strontium nitrate:Eu3+ ì
rú́
r
«
Ñ_
]
j
¦0
`
AK
Junsei
_
TiO2 , BaO2 , Sr(NO3 )2 \
¦
6
x
%
i
¼9,
Ü
¥½
D
ËÓ
+
t
ü
r y
É
y
_
$
ì
í
r
¦
` r
ì
q
1:1:1s
&
÷
¸2
¤
¸$
í
#
}
µ
Ï
1
Ð 10ì
r &
ñ
¸ °
ú
ï
r Ê
ê PBM ~
ÓZ
½
O
¦ `
6
xK
"
f
©
r\
:
"
f x
a
9
A
%
i
. x
a
9
A
¸|
Ü
¼
Ð
H 80
ml ^
&
_
h
t
Ø
Ô
ï³
u 6
o
xl
\
"
f ^
¦õ
r
«
Ñ_
Á
º>
q
30:1s
÷
&
¸2
¤ ì
rú́
õ
t
Ø
Ô
ï³
u ½
o
¨ (zirconia ball, f
â
15 mm)\
¦
6
x
#
500 rpm_
r
5
q
Å
¸
Ðz
´+
>
«
%
i
.
r
É
ü
@
(ultraviolet, UV)s
&
ü
h
@
ò
%%
@
i
/
¸
rF
>
a
9
x
Ar
ç
(milling time, tm )
ß
r 300ì
É
rõ
600ì
rÜ
¼
Ð
%
Ü
i
¼
t
ë
@
ß
/Â
Òì
r r
F
g
%
%
ò
\
i
e
. :
¤y
£
100¸
s
©
9, /
L
å
ô
Ç
r
:
¸
5
©
x
p
¦
`}
l
0
AK
15ì
rx
a
9
AÊ
ê 30ì
r&
ñ
¸A
a
)
½
¨%
i
\
¦ t
¦e
HÁ
ºl
(inorganic) +
AF
þ
g^
r
t
v
Hõ
&
`
ñ
¦>
5
qì
Å
Í4
ø
¤Ù
¡
þ
. x
a
9
Aô
Çr
«
Ñ
H 800 ◦ C
H+
AF
þ
g1
x`
p
¦
í
Ê
<
#
, cathod ray tube (CRT), X-ray "
\
f 1r
ç
\
ß
%
P
o
%
i
.
|ó
Í, F
ø
g
¦6
x
Ð×
¼, plasma display panel (PDP),
j
]
aì
)
rú́
_
©
I
\
¦
¸
l
0
A
#
XRD (PANa-
light emitting diode (LED) 1
x\
p
6
x÷
&#
QÄ
ºo
Ò
t
q
Ö̧\
lytical, X’pert PRO MPD)\
¦
6
x
%
i
. X-
"
¶
é
ré
É
ß
X
9
x
]y
aº
'
÷
&#
Qe
Ü
¼9,
ÓÊ
¾
ê_
Æ,
<
Ðî
1
ß
x
p
ç
s
ß
&
ñ
Ð\
¦%
3
¦
H
¸
Hì
r
\
V
o
,
Ö̧6
x
a
)
.
1966¸
GaN '
A
õ
o
Ò LED
6
©
x
o
as
)
A
Ñ
Ò
þ
o LED\
Ø
s
Ôl
t
ú́
§
r µ
É
Ï
1
`
¦ s
À
Ò%
Ü
3
¼
f
|
&
9
>
h
h
`
¦
Aô
0
Çõ
]
j
Hí
&
ß
K
h
e
H
I
©
s
. &
Ò
h
oþ
A
+F
g^
H
ü
@
o CuKα
Ò
(λ = 1.5406 Å)`
¦
6
x
%
Ü
i
¼9, 5
q
Å
·
õ
ú
À
Ó
Hy
y
40 kVü
< 30 mAs
%
3
. 2θ_
8
¤&
£
3
ñ
#0
A
H 10
∼90◦ t
Ð %
Ü
i
¼9, Å
Ò
5
q
Å
¸
H 1 sec/0.03 stepÜ
¼
Ð
%
i
. TG
H{
&
9
ô
ñ
Ç5
q
Å
¸
Ð
r
:
¸\
¦
or
(
`
¦M
:Å
Ò
Q
#
r
ç
1
ß
xî
l
r
ß
«
Ñ_
Á
º>
o\
¦l
2
¤ô
Ç
כ
s9, DTA
Hr
«
Ñ\
¦{
ñ
9
&ô
Ç5
q
Å
¸
Ð \
<
P
Ê
rÍ
É
ty
r
(
`
¦M
:Õ
ª
r
:
Ü
¼
ÐÂ
Ò'
&
ü
h
@
t
_
\
-t
s
#
_
Ä
â
º
Ð
¸#
_
3
ß
î\
"
f
H\
&
P
:
h
¤$
£
_
í
o \
O
Hl
ï
rÓ
t|
ü
õ
9
8&
"
fZ
}
r ò́Ö
É
¦_
+
AF
þ
g^
\
¦%
l
3
B
Ä
º#
Q§
>
.
«
r
Ñ<
ü_
r
:
¸
∆T\
¦
r
:
¸_
ÊÃ
<
º
Ðl
2
¤ô
Ç
Ü
כ
¼
Ð 50
Liu 1
x
p
r [5]
É
r É
o
Æ 6
<
xÓ
o 7
x
£
ÌZ
Ã
\
O
_
K
]
j
a
)
Ba0.7 Sr0.3 TiO3 :Eu3+ ~
Ì}
Ã
_
½
¨
¸ü
< F
gµ
ÏF
1
g :
¤$
£
, Õ
í
ªo
∼ 1000 ◦ C
r
:
¸½
¨ç
\
ß
"
f \
5
P
q
Å
¸\
¦ 10 ◦ C/min
Ð8
¤&
£
ñ
%
i
.
¦ Ä
»
:
¤$
£
\
í
@
/K
½
¨Ù
¡Ü
þ
¼9, Pazik 1
x [6]
p
r #
É
Q
Eu\
¦ 6.0, 8.0, Õ
ªo
¦ 10 mol%\
¦y
y
'
ô
Çr
«
Ñì
r
t
~
ÓZ
½
Ü
O
¼
Ð ]
j
a Bax Sr1−x TiO3 (BST):Eu3+ ì
)
rú́
_
ú́
F
gµ
ÏF
1
g$
Û
í
¼&
à
7
Ô!
3
r Ocean Optics USB2000 specÉ
t_
þ
[
½
¨
¸ x
þ
9
A
+F
g :
¤$
£
`
í
¦
½
¨Ù
¡
þ
. ¢̧ô
Ç Samantaray
x [7]
p
1
r Eu\
É
¦
¸i
ô
ç
Ç barium strontium titanate (Ba,
Sr) TiO3 [
j
b
[
t\
þ
@
/K
BaTiO3 , SrTiO3 , Õ
ªo
¦
Eu2 O3 _
¸$
q
í
\
¦
Ø
Ô>
]
j
ô
ÇÊ
êF
gµ
ÏF
1
g:
¤$
£
`
í
¦
¨Ù
½
¡
þ
.
r
:
Hë
7
H
r PBM ~
É
ÓZ
½
\
O
_
K
Eu3+ \
¦ 6 mol%, 8 mol%,
trometer\
¦
6
x
#
¸
%
i
. F
g#
l
HF
g3
$Ä
Ȁ
»
¸
u
©
Â
Ò
Ì
Ã
a LEDF
)
g"
¶`
é
¦
6
x
#
s
À
Ò#
Q&
Ü
¼9 È
Ò
y
¸
H 45◦ s
%
3
. s
M
: /
N$
B
z
í
´o
HÜ
B
¼
ÐÂ
Ò'
µ
ÏF
1
g
ay
)
C
n
r 90◦ 0
É
Au
\
e
H CCD detector\
aF
)
g$
Ä
3
»
Ð Ã
º|
÷
9
&%
3
. CCD detector_
Ã
ºF
g
%
©
%
ò
i
r 400
É
nm\
"
fÂ
Ò'
900 nm
t
s
%
3
.
ªo
Õ
¦ 10 mol%
¸i
r
ç
BaO2 -TiO2 -Strontium nitrate
rú́
ì
`
¦½
Ë$
+
í
%
Ü
i
¼9, ½
Ëí
+
$
aì
)
rú́
_
½
¨
¸&
:
h
¤$
£
õ
í
F
g
III. +
ÇÊ
s
Ýõ
ÍÀ
m
Ø8
X
ý
ÏF
1
µ
g:
¤$
£
í
r XRD, TG/DTA, Õ
É
ªo
¦ Ocean Optics USB
2000 spectrometer\
¦
6
x
#
8
¤&
£
ñ
%
i
.
Fig. 1
r PBM ~
É
ÓZ
½
\
O
_
K
0ì
r, 300ì
r, Õ
ª
o
¦ 600ì
r
xî
l
1
x
ß
a
9
Aô
Ç Eu3+ -doped BaO2 -TiO2 -Strontium nitrate
rú́
ì
_
X-
r]
X
¸
_
ª
o\
¦
pÕ
·
ªa
>
Ë
s
. x
a
9
A
∗ E-mail:
[email protected]
t
·
§
ú
¤`
¦ M
:<
ü q
§K
"
f 300ì
r x
a
9
A
%
`
i
¦ Ä
â
º {
9
870
New Physics: Sae Mulli, Vol. 65, No. 9, September 2015
Fig. 1. (Color online) XRD patterns of Eu-doped BaO2 TiO2 -Strontium nitrate powders by Planetary Ball Mill.
Ò x
Â
ß
¼[
t
þ
r ¢
É
a
y
\
#
O
Qt
<
Ê
r
É
{
©
y
©
y
èH
d`
¦
Fig. 2. (Color online) (a) Williamson-Hall plot showing
β cos θ/λ vs. 2sin θ/λ for the powders after 600 min of
milling. (b) Crystallite size obtained by applying the
Scherrer formula to different peaks of the XRD patterns
for the powders with 600 min of milling.
¦Ã
^
ºe
%
3
. :
¤y
£
300ì
rs
x
©
a
9
A
%
`
i
¦
Ä
â
º TiO2 ,
BaO2 , Sr(NO3 )2 ü
@\
¸ Ba(NO3 )2 x
ß
¼[
ts
þ
z
`
¦
·
t
§
ú
r?
É
/Â
Ò
+
A\
þ
aº
'
a(
)
f
&
³
`
©
¦ Williamson-Hall
º
ú
·
Ãe
%
Ü
3
¼9, 600ì
rx
a
9
A
%
`
i
¦
Ä
â
º\
H Ba(NO3 )2
ÓZ
½
~
\
O
"
f
H
¦
9Ù
¡l
þ
M
:ë
H
כ
Ü
¼
ÐÒ
ty
q
a
)
. Scherrer
ß
x
¼[
t
þ
¸ y
è÷
&
x
ß
¼[
ts
þ
e
%
6
3
§`
£
¦ ·
Ã
ú
º
Nd
B
/
`
¦s
6
x
#
>
í
ß
Ç
ô î̈
ç
H
&
ß
ñ
¼l
\
¦ tm Z
>
Ðq
§
%
e
3
. s
ü
<°
ú
r
É
³
&
©
r BaO2 x
É
a
9
A\
r\
É
\
P
-
K
Ð
Fig. 2(b)\
¶
{
ú
9
a
)
rÕ
É
ªa
>\
Ë
"
f^
¦º
Ãe
1
ws
p
1
t
xõ
p
°
ú
rz
É
´+
>8̈
«
\
â
_
K
8̈
"
¶÷
é
&
¦ Sr(NO3 )2
Hì
r
300ì
r1
xî
l
x
ß
a
9
Aô
Çr
«
Ñì
rú́
_
î̈
ç
H
&
ß
ñ
¼l
H
32.4
&
K
÷#
Q Ba(NO3 )2 Ò
tí
q
$
a
)
Ü
כ
¼
ÐÆ
Ò&
ñ
a
)
.
nm
Ð 600ì
r1
xî
l
x
ß
a
9
Aô
Çr
«
Ñì
rú́
_
î̈
ç
H
&
ß
ñ
¼l
Ð
Fig. 2
Hr
«
Ñì
rú́
_
{
9
ß
¼l
<
ü?
/Â
Ò
þ
A
+Ö
¦_
o
¸F
K
8(
6
§
£
¦
`·
Ã
ú
ºe
%
3
. ¢̧ô
Ç 2θ_
o
\
r
É
¦ Williamson-Hall [8–10] ~
\
ÓZ
½
Ü
O
¼
н
¨
%
Ü
i
¼9, Scher-
&
ß
ñ
¼l
\
¦q
§K
Ð
, 300ì
r1
xî
l
x
ß
a
9
Aô
Ç
r«
Ñ_
â
rer ~
ÓZ
½
[11]`
O
¦ 6
x
#
½
¨ô
Ç r
«
Ñì
rú́
_
{
9
ß
¼l
º
Ä
H 2θ @
/|
Ì 40◦ Ä
t
&
ß
ñ
¼l
7
x
£
Õ
ªÊ
ê
¦ \
q
§
%
i
. Fig. 2(a)
H 600ì
r x
a
9
Aô
Ç r
«
Ñ ì
rú́
`
¦
/^
@
&
Ü
h
¼
Ðy
è
H
â
Ó`
¾
¦
Ð%
Ü
i
¼
, 600ì
r1
xî
l
x
ß
a
9
A
Williamson-Hall ~
ÓZ
½
`
O
¦ s
6
x
#
Õ
ª
; Õ
2
ªa
>Ü
Ë
¼
Ð î̈
ç
H
Çr
ô
«
Ñ_
Ä
â
º\
H 2θ 50◦ &
ñ
¸
t
&
¼
ñ
ßl
@
/
&
ß
ñ
¼l
H
74.1 nms
%
Ü
3
¼9,
+
AÖ
þ
¦
¦
`_
p
Hf
&
^
Ü
h
¼
Ð{
ñ
9
&
Ê`
<
¦^
¦Ã
ºe
%
3
.
−3
%
s
3
. ¢̧ô
Ç Scherrer /
N
B
Fig. 3
r r
É
«
Ñ ì
rú́
`
¦ 600ì
r x
a
9
Aô
Ç ê
Ê 8
¤&
£
ô
ñ
Ç
`
d
¦s
6
x
#
1
x{
l
ô
9
Çr
ç
1
ß
xî
l
x
ß
a
9
Aô
Çr
«
Ñì
rú́
_
î̈
TG/DTA Õ
ªa
>s
Ë
. 8
xÁ
ú
º>
y
èÖ
¦
r 29.22%s
É
%
Ü
3
¼9,
H
ç
&
ß
ñ
¼l
H
29.1 nm s
%
3
[Fig. 2(b)]. s
<
ü°
s
ú
j@
þ
/ì
rK
r
:
¸
H 604.1 ◦ C,
s
r
r
:
¸
H
525.7 ◦ C
Williamson-Hall ~
ÓZ
½
\
O
_
K
>
í
ß
a
)
ñ
&ß
¼l
Scher-
`
e
¦·
Ã
ú
ºe
%
3
.
527.0 ◦ C\
"
f
626.5 ◦ C
t
_
rer ~
ÓZ
½
\
O
_
K
>
í
ß
a )
&
ß
ñ
¼l
\
q
K
8 Z
}
r É
`
כ
¦
º>
Á
y
èÖ
¦s
^
y
èÖ
¦_
83.2%
Ð
ß
©
¼>
¦Ã
^
ºe
%
3
HX
<, s
s
H Scherrer ~
ÓZ
½
\
O
"
f
HÒ
ty
q
z
`
¦·
Ã
ú
ºe
%
3
.
_
l
Ö
¦l
H
6.01 × 10
Formation and Photoluminescence of BaO2 -TiO2 -Strontium nitrate:Eu3+ Powders Fabricated by · · · – Hyun-Goo Kim
871
Fig. 4. (Color online) Eu concentration dependence of
PL emission spectra from the BaO2 -TiO2 -Strontium nitrate: Eu3+ mixtures after 600 min of milling.
Fig. 3. TG/DTA patterns of the BaO2 -TiO2 -Strontium
nitrate: Eu3+ mixture after 600 min of milling.
Fig. 4
H BaO2 -TiO2 -Strontium nitrate ì
rú́
\
Eu3+ \
¦
6 mol%, 8 mol%, Õ
ªo
¦ 10 mol%m
'
ô
Ç
6
§, PBM
£
ÓZ
½
~
Ü
O
¼
Ð 600ì
rx
a
9
A
#
800 ◦ C
Ð 1r
ç
m
ß
\
%
P
o
ô
Ç
«
r
Ñ[
t_
þ
µ
ÏF
1
gy
©
¸\
¦q
§ô
ÇÕ
ªa
>s
Ë
. Eu\
¦ 6 mol%,
8 mol% '
ô
Çr
«
Ñ[
t_
þ
1
Ï
µF
gy
©
¸
Ð
Eu\
¦ 10 mol%
ô
'
Ç r
«
Ñ_
1
Ï
µF
g y
©
¸
Z
©
}6
§
£
¦
` ·
Ã
ú
º e
%
Ü
3
¼
9, Eu\
¦ 6 mol%ü
< 8 mol% '
ô
Çr
«
Ñ[
t_
þ
1
Ï
µF
gy
©
¸
H@
/^
&
Ü
h
¼
Ðq
5
w
p
Ê`
<
¦·
Ã
ú
ºe
%
3
. 8
¤&
£
ñ
ar
)
«
Ñì
rú́
1
_
Ï
µF
gx
ß
¼[
t
þ
r@
É
/^
&
Ü
h
¼
Ð 578 nm (5 Do → 7 F0 ), 591
nm (5 Do → 7 F1 ), 615.5 nm (5 Do → 7 F2 ), 666 nm (5 Do
→ 7 F3 ), Õ
ªo
¦ 698 nm (5 Do → 7 F4 )
н
¨$
÷
í
&%
Ü
3
¼9,
¤y
£
:
×
æd
Â
Ò
H\
0
Au
ô
Ç 591 nmü
< 615.5 nm_
1
Ï
µF
gx
¼
ß
Hr
«
Ñ[
ts
þ
¸E
t
$
-&
Ò
h
oµ
ÏF
1
g`
¦
?
/
H
Ü
כ
¼
ÐÒ
t
q
y
a
)
[5].
Fig. 5
H 300ì
rõ
600ì
r 1
xî
l
x
ß
a
9
Aô
Ç BaO2 -TiO2 Strontium nitrate:Eu r
«
Ñ ì
rú́
`
¦ 800 ◦ C\
"
f 1 h 1
x
l
Fig. 5. (Color online) XRD patterns of Eu-doped BaO2 TiO2 -Strontium nitrate powders after annealing at 800
◦
C for 1 h.
\
ß
î
%
P
o
ô
Ç X-
r]
X
¸
_
ª
o\
¦
pÕ
·
ªa
>s
Ë
.
300ì
rõ
600ì
rx
9
a
Aô
Çr
«
Ñ
¸¿
º\
"
f Sr2 TiO4 x
ß
¼[
tõ
þ
IV. +
ÇÂ
s
Ø
]
(Ba1.5 Sr0.5 )TiO4 x
ß
¼[
ts
þ
8
¤&
£
÷
ñ
&%
3
. Õ
ª
Q
300ì
rx
9
Aô
a
Çr
«
Ñ\
¦\
%
P
o
ô
Çâ
Ä
º\
H Sr2 TiO4 x
ß
¼[
ts
þ
Å
Ò
Ð
600ì
rx
a
9
Aô
Çr
«
Ñì
rú́
`
¦ Williamson-Hall ~
ÓZ
½
`
O
¦s
¤&
£
8
÷
ñ
&%
Ü
3
¼9 {
9
Â
Ò (Ba1.5 Sr0.5 )TiO4 x
ß
¼[
ts
þ
8
¤&
£
÷
ñ
&%
3
x
6
#
½
¨ô
Ç ñ
&ß
¼l
H
74.1 nm,
þ
A
+Ö
¦
r
É
6.01
¦, 600ì
rx
9
a
Aô
Çr
«
Ñì
rú́
_
Ä
â
º
H (Ba1.5 Sr0.5 )TiO4
× 10−3 s
%
Ü
3
¼9, þ
j@
/ ì
rK
r
:
¸
H 604.1 ◦ C,
s
r
ß
x
¼[
ts
þ
Å
Ò
Ð8
¤&
£
÷
ñ
&%
Ü
3
¼9 {
Â
9
Ò Sr2 TiO4 x
ß
¼[
ts
þ
8
¤
£
r
:
¸
H
525.7 ◦ Ce
`
¦ ·
Ã
ú
º e
%
3
. 8
x Á
ú
º
> y
èÖ
¦
H
ñ
&
d`
¦S
X
½
ÉÃ
+
ºe
%
3
.
r 29.22%s
É
%
Ü
3
¼9,
527.0 ◦ C\
"
f
626.5 ◦ C
t
_
872
New Physics: Sae Mulli, Vol. 65, No. 9, September 2015
Á>
º
y
èÖ
¦s
^
y
èÖ
¦_
83.2%
Ð
ß
©
¼>
z
`
¦·
Ã
ú
ºe
%
3
. Eu\
¦ 10 mol% '
Ù
¡`
þ
¦
Ä
â
ºµ
Ï
1
gx
F
ß
¼_
©
y
¸
Z
©
}6
§`
£
¦·
Ã
ú
ºe
%
Ü
3
¼9, @
/^
&
h
5
7
¼
Ü
Ð 578 nm ( Do → F0 ),
¸E
t
$
-&
Ò
h
o µ
ÏF
1
g`
¦ ?
/
H 591 nm (5 Do →7 F1 )ü
< 615.5 nm (5 Do →7 F2 ), Õ
ªo
¦ 666 nm (5 Do →7 F3 ), Õ
ªo
¦ 698 nm (5 Do →7 F4 )
Ð
¨$
½
÷
í
&%
3
. 300ì
rõ
600ì
r1
xî
l
x
ß
a
9
Aô
Çr
«
Ñì
rú́
[
t`
þ
¦
◦
800 C\
"
f1h1
xî
l
\
ß
%
P
o
ô
Çr
«
Ñ[
t\
þ
"
f
H Sr2 TiO4 ü
<
(Ba1.5 Sr0.5 )TiO4 x
ß
¼[
ts
þ
8
¤&
£
÷
ñ
&%
3
.
[3] C. Kursun and M. Gogebakan, J. Alloys Compd.
619, 138 (2015).
[4] C. C. Koch, O. B. Cavin, C. G. McKamey and J. O.
Scarbrough, Appl. Phys. Lett. 43, 1017 (1973).
[5] L. Liu, N. Qin and D. Bao, Curr. Phys. 15, 748
(2015).
[6] R. Pazik, D. Hreniak, W. Strek, A. Speghini and M.
Bettinelli, Opt. Mater. 28, 1284 (2006).
[7] C. B. Samantaray, M. L. Nanda Goswami, D. Bhat-
ACKNOWLEDGEMENTS
tacharya, S. K. Ray and H. N. Acharya, Matter.
Lett. 58, 2299 (2004).
This study was supported by research fund from
Chosun University, 2015.
[8] G. K. Williamson and W. H. Hall, Acta Metall. 1,
22 (1953).
[9] M. E. Rabanal, A. Vorez, B. Levenfeld and J.
REFERENCES
M. Torralba, J. Mater. Process. Technol. 143, 470
(2003).
[1] S. Kumaran, T. Sasikumar, R. Arockiakumar and
T. S. Rao, Powder Technol. 185, 124 (2008).
[2] M. Slimi, M. Azabou, L. Escoda, J. J. Sunol and M.
Khitouni, Powder Technol. 266, 262 (2014).
[10] W. H. Hall, Proc. Phys. A 62, 741 (1949).
[11] B. D. Cullity,
Elements of X-ray Diffraction
(Addison-Wesley, Massachusetts, 1978), p. 284.
© Copyright 2026 Paperzz