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8/11/2019 Phasematched Secondharmonic Generation in Periodically Poled Optical Fibers
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Phasematched secondharmonic generation in periodically poled optical fibers
Raman Kashyap
Citation: Applied Physics Letters 58, 1233 (1991); doi: 10.1063/1.104372
View online: http://dx.doi.org/10.1063/1.104372
View Table of Contents: http://scitation.aip.org/content/aip/journal/apl/58/12?ver=pdfcov
Published by the AIP Publishing
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http://scitation.aip.org/search?value1=Raman+Kashyap&option1=authorhttp://scitation.aip.org/content/aip/journal/apl?ver=pdfcovhttp://dx.doi.org/10.1063/1.104372http://scitation.aip.org/content/aip/journal/apl/58/12?ver=pdfcovhttp://scitation.aip.org/content/aip?ver=pdfcovhttp://scitation.aip.org/content/aip/journal/apl/91/9/10.1063/1.2776876?ver=pdfcovhttp://scitation.aip.org/content/aip/journal/apl/91/9/10.1063/1.2776876?ver=pdfcovhttp://scitation.aip.org/content/aip/journal/jap/95/7/10.1063/1.1667271?ver=pdfcovhttp://scitation.aip.org/content/aip/journal/apl/64/11/10.1063/1.111925?ver=pdfcovhttp://scitation.aip.org/content/aip/journal/apl/63/11/10.1063/1.109656?ver=pdfcovhttp://scitation.aip.org/content/aip/journal/apl/60/23/10.1063/1.106845?ver=pdfcovhttp://scitation.aip.org/content/aip/journal/apl/60/23/10.1063/1.106845?ver=pdfcovhttp://scitation.aip.org/content/aip/journal/apl/63/11/10.1063/1.109656?ver=pdfcovhttp://scitation.aip.org/content/aip/journal/apl/64/11/10.1063/1.111925?ver=pdfcovhttp://scitation.aip.org/content/aip/journal/jap/95/7/10.1063/1.1667271?ver=pdfcovhttp://scitation.aip.org/content/aip/journal/apl/91/9/10.1063/1.2776876?ver=pdfcovhttp://scitation.aip.org/content/aip/journal/apl/91/9/10.1063/1.2776876?ver=pdfcovhttp://scitation.aip.org/content/aip?ver=pdfcovhttp://scitation.aip.org/content/aip/journal/apl/58/12?ver=pdfcovhttp://dx.doi.org/10.1063/1.104372http://scitation.aip.org/content/aip/journal/apl?ver=pdfcovhttp://scitation.aip.org/search?value1=Raman+Kashyap&option1=authorhttp://oasc12039.247realmedia.com/RealMedia/ads/click_lx.ads/www.aip.org/pt/adcenter/pdfcover_test/L-37/454711315/x01/AIP-PT/COMSOL_APLArticleDL_060414/COMSOL_banner_US_IEEE-Supplement-2014_1640x440.png/5532386d4f314a53757a6b4144615953?xhttp://scitation.aip.org/content/aip/journal/apl?ver=pdfcov8/11/2019 Phasematched Secondharmonic Generation in Periodically Poled Optical Fibers
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second-harmonic generation in periodically poled optical
Raman Kashyap
British Telecom ResearchLaboratories, Martlesham Heath, Ipswich IP5 7RE, United Kingdom
(Received 1 October 1990; accepted for publication 18 December 1990)
Phase-matched second-harmonic generation is reported in periodically poled optical fibers for
the first time. A periodic x was induced in optical fibers during phase-matched
periodic-electric field-induced second-harmonic generation at a fundamental wavelength of
1064 nm. Further, it is shown that periodic poling can be achieved by photo excitation
with radiation of 514.5 nm wavelength while applying a spatially periodic static field. In both
cases, the mode interaction HEyi
-*HE:? is quasi-phase matched at 1064 nm. Seeding is
observed in fibers beyond the poled region. A photoinduced index change has been measured
using electric field induced second-harmonic generation.
Optical fibers have been poled by the application of
electric fields in the presence of high-intensity
phase-matched and non-phase-matched fibers.2
fibers by quasi-phase matching3 using spatially pe-
dc electric fields in the presence of (a) 1064 nm
or (b) argon ion laser 514.5 nm radiation. It is
d that after poling of the fiber for the interac-
-+ HE:;, it subsequently
the same mode interaction when
1064 nm radiation alone. The fiber beyond the
region seeds4 in the presence of 1064 nm radiation
competition in second-harmonic generation (SHG)
and poled regions of the fiber is thought to
The fiber device used for poling is similar to the one
in Ref. 5. Two half-coupler blocks (HCB) as used in
tric field induced second-harmonic gen-
in optical fibers were made using two
(core radius 1.19 pm) and B (core radius 1.52
Both fibers had a core-cladding index difference of
o that the fiber cladding was partially removed in
lo-mm-long region in the middle of the HCB. The edge
ore was estimated5 to be approximately 6 pm below
urface for fiber A and 2 pm for fiber B. A chromium
electrode structure, manufactured on a glass
placed on the surface of the HCB with a
spacer to separate the periodic electrode f rom the
etter, seeding refers to the situation
the presence of the fundamental and second-
wavelengths alone in the fiber induces prepara-
al poling as reported by Stolen and Tom,4
self-seeding refers to preparation in the absence of
external second-harmonic seed.
Before beginning the poling experiments, the-electrode
rotated while 1064 nm radiation was present in the
to achieve phase-matched periodic-EFISH generation
HEY, *HE:; interaction. The angle 8 of the elec-
= A/(2 cos 6), where A is the period of the in-
electrodes. For both wavelengths, the electrode
was left in position at the phase-matching angle during
poling so that the poled fiber would be phase matched for
the same mode interaction.
In the poling experiments with 1064 nm radiation, ini-
tially, 130 mW of 150 ns Q-switched 1064 nm radiation at
a repetition rate of 1 kHz was launched into fiber A to
ensure that no self-preparation was taking place. There was
little change in the background signal over a period of an
hour. A pulsed dc field of 10 ps pulse width was then
applied. Poling was performed on a device using fibre A
with a 4 ,um Mylar spacer. Phase-matched SHG was ob-
served at 8 = 10.8. With A = 32 ,um the coherence length
Z, was calculated to be 16.29 pm. The maximum average
field in the core was calculated5 to be 1.95 x lo6 V m - t
(120 V across electrodes). After poling, and in the pres-
ence of the electric field, there are three factors that con-
tribute to the SHG signal-EFISH generation, SHG from
the poled region and SHG from any seeded region. The
poled region should have a grating rr/2 out of phase with
the grating created by the EFISH generated seeding signal
(proportional to x
3&,) as is the case in normally seeded
fibers. After poling for 10 min, the SHG signal with 150
mW of infrared power was monitored, as the spatially pe-
riodic static potential is varied from 120 to 0 V and back up
to 120 V (shown in Fig. 1). The x axis shows arbitrary
time taken to ramp the voltage manually . The top curve
shows that at first the SHG signal decreases with decreas-
ing field (bottom curve). The SHG signal does not reach
zero showing that there is an increase in the background
SHG level which is believed to be as a result of EFISH
generation acting as the seeding radiation. As the dc-field
induced nonlinearity x
(3)Edc becomes smaller by further
reducing Ed0 the second-harmonic signal increases indicat-
ing that the poled nonlinearity is of the opposite sign to the
EFISH nonlinearity (i.e., out of phase by Z- radians). At
zero field, the poled signal is slightly less than the EFISH
signal. Increasing the static field returns the SHG to the
EFISH level by retracing the curve. By cutting back the
fiber it was ascertained that only the length of fiber beyond
the poled region had seeded; it might be concluded that the
fiber had not self seeded but that had undergone EFISH
generation-assisted seeding.
Appl. Phys. Lett. 58 (12), 25 March 1991
0003-6951/91 /I 21233-03 02.00
@ 1991 American Institute of Physics
1233
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8/11/2019 Phasematched Secondharmonic Generation in Periodically Poled Optical Fibers
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Time (Minutes)
FIG. 1. Top curve shows SHG signal from a poled fiber. Bottom curve is
the corresponding voltage applied to the periodic electrodes. The hori-
zontal axis shows the time over which the measurement was performed as
the voltage is varied manu ally between 120 and 0 V.
A second device made with fiber B was also electrically
poled using the same infrared power. The voltage applied
across the electrodes was between 50 and 100 V (average
dc field in the core of between 1.84~ lo5 and 3.68~ lo5
V m - ). Phase-matched periodic EFISH generation ob-
served at an angle of 18.8 corresponds to a coherence
length t, of 16.90 pm. The conversion efficiency for EFISH
generation was measured to
be
6.08 X 10 - 6%. The poling
field was applied for 200 min and the growth of the poling-
induced second-harmonic signal (shown in Fig. 2) mea-
sured by occasionally switching off the dc-electric field.
The final poled SHG signal was approximately 190 x the
initial background SHG signal, giving
a
conversion effi-
ciency of 3.85 X 10 - 6%. A linear growth in the SHG sig-
nal with time of application of the field was seen and no
saturation was observed. Once the poling field was
switched off, the SHG signal was monitored continuously
over a period of 600 min at the same input infrared power.
The data are shown in Fig. 3. Immediately after poling the
4
El
t
cl
g
2
El
a
?
II
lo
fn 1
El
El
l3
a
I 1
I
0
100
200
Field application time (minutes)
FIG. 2. Growth in the SHG signal from a poled fiber as a function of
poling time.
+self
seeding
- IOOIM
z
- 1000
competitionwith
170 mW QS 1064nm
% 100
a
I., ,
. , .
,
0 100 200 300 400 500
time (minutes)
600
FIG. 3. SHG si gnal after poling as a function of time. Initially the signal
decreases slowly. Note that at 1 20 min, the i nfrared power was raised
from 130 to 170 mW.
SHG signal slowly decayed, During this measurement, the
infrared power was raised to 170 mW after 120 min caus-
ing the SHG signal to increase slightly before continuing to
decay. After 220 min, the SHG signal began to increase
and this was attributed to the beginning of seeding of the
fiber beyond the poled region. The decrease in SHG is not
believed to be due to self erasure, since the decrease after
poling is followed by a steady growth in self-seeded har-
monic radiation. Our preliminary experiments indicate
that competition between the SHG from the poled and
seeded regions is the cause of the SHG signal decaying
with time immediately after poling.
The observation of poling in optical fibers with 1064
nm radiation on application of the periodic static field is of
practical interest but also intriguing. Bergot et af. have
reported poling in the presence of infrared light bu t they
gave no reasons for their observation. We believe that pol-
ing is assisted by Four-photon absorption from 1064 nm. In
previous experiments,6 we observed erasure of self-seeded
gratings with infrared radiation alone and recently, the
erasure has been shown to be proportional to the fourth
power of the infrared intensity. The intensity of the infra-
red in the core was approximately 14 GW cm - f 140
W pm - 1, similar to that used in Ref. 7. A possible ex-
planation is that: carriers are generated through four-
photon absorption which are then organized by external
electric fields. With the external field off, the internal
charge distribution remains, creating an internal poling
field.
Electric field poling was also tried with 514.5 nm ra-
diation. At first irradiation of Fiber B with 250 mW of
514.5 nm radiation for 30 min completely erased the pre-
viously poled fiber so that subsequentl y only the back-
ground SHG signal was observed when probed with 1064
nm radiation. Not wi thstanding the use of different fibers,
this observation is contrary to the work of Bergot et al.
who noted that the poled nonlinearity did not erase with
blue-green light irradiation. After e rasure, the EFISH gen-
eration phase-matching angle 8 at 1064 nm had to be al-
tered to 18, indicating a photoinduced change in the mode
indices had occurred. The magnitude of the change in the
index mismatch of the modes A(n - nb) before and af-
ter erasure was calculated to be 7.3~ 10 - * (equivalent to
a change in the core cladding index difference at both fre-
1234 Appl. Phys. Lett., Vol. 58, No. 12, 25 March 1991
Raman Kashyap
1234
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8/11/2019 Phasematched Secondharmonic Generation in Periodically Poled Optical Fibers
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d 2w, of approximately 8 X 10 - 5). Detail ed
be published elsewhere.
Poling of the fiber was then performed using 140 ps dc
and acousto-optically generated 100 ps pulses at
nm wavelength radiation at a repetition rate of 1
The poling field (average of 8.1 x lo5 V m - in the
was applied for a time longer than the optical pulses
avoid optical bleaching during the off period. 200 mW of
was used for a poling time of 205 min. After poling,
final SHG signal was 70.3~ the background when
130 mW of Q switched 1064 nm radiation.
conversion efficiency was approximately
x 10 - 6%, being limited by a photoinduced change in
The intensity of the 514.5 nm radiation while poling
approximately 10 MW cm - (0.1 W pm - 2), well be-
the 1 Wprnw2
threshold required for poling by Bergot
al. in their experiment. By our own experiments of
formation in optical fibers and those re-
recently by LaRochelle et ~f.,~ we believe that pho-
y by two-photon absorption (TPA), is
place at these intensities and the carriers so gener-
if two-photon excitation at 514.5 nm is assisting
process, then the question remains as to whether
532 nm light through EFISH generation is causing
With intensities five orders of
smaller at 532 nm than used in the 514.5 nm
experiment, it is expected that the poling time
be ten orders of magnitude greater, contrary to ob-
EFISH-generated signal on its own does
the poling process.
It has been shown that optical fibers can be poled to
create a spatially periodic nonlinearity by photoexcitation
at a wavelength of 1064 nm or 514.5 nm and simultaneous
application of a periodic static field. The poled nonlinearity
has the opposite sign to that of EFISH generation. A pos-
sible explanation is that electric field poling is assisted by
four-photon excitation from 1064 nm and two-photon ex-
citation from 5 14.5 nm. A photoinduced change in the core
cladding refractive index difference of the fiber after irra-
diation of the fiber with 514.5 nm light has been observed
and estimated to be approximately 8X lo- 5. With better
optimized devices, it should be possible to seed fibers effi-
ciently by using periodic EFISH generation. Periodic pol-
ing of fibers in connection with short wavelength radiation
should allow phase-matching at arbitrary wavelengths.
Frequency mixing from wavelengths at which the fiber is
not photosensitive should then be possible.
I would li ke to thank S. T. Davey, D. L. Williams, and
C. A. Millar for stimulating discussions and comments on
the manuscript.
M. V. Bergot, M. C. Farries, M. E. Fermann, L. Li, L. J. Poyntz-
Wright, P. St. J. Russell, and A. Smith son, Opt. Lett. 13, 592 (1988).
M. E. Fermann, L. Li, M. C. Farries, and D. N. Payne, IEE Conf. Proc.
292, 135 (1988).
3N. Bl oembergen and N. J. Sievers, Appl. Phys. Lett. 17, 483 ( 1970).
4R. H. Stolen and H. W. K. Tom, Opt. Lett. 12, 585 (1987).
5R. Kashyap, J. Opt. Sot. A m. B 6, 313 ( 1989).
J. Lucek, R. Kashyap, S. T. Davey, and D. L. Williams, J. Mod. Opt.
37, 533 (1990).
Y. Hibino, V. Mizrahi, and G. I. Stegeman, Appl. Phys. Lett. 57, 656
(1990).
R. Kashyap, in Proceedings of Topical Meeting on Nonlinear Guided
Wave Phenomenon: Physics and Applications, 1989 Technical Digest Se-
ries, Vol. 2 (Optical Society of American, Washington DC, 1989), pp.
255-258.
9S. LaRochelle, V. Mizrahi, G. I. Stegeman, Appl. Phys. Lett. 57, 747
(1990).
Appl. Phys. Lett., Vol. 58, No. 12, 25 March 1991
Raman Kashyap
1235
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