國 立 交 通 大 學
光 電 工 程 研 究 所
碩 士 論 文
硒化鎵晶體中兆赫波光參數放大之研究
The study of terahertz optical parametric
amplification in ε-GaSe crystals
研 究 生:許哲睿
指 導 老 師:潘犀靈 教授
硒化鎵晶體中兆赫波光參數放大之研究
The study of terahertz optical parametric
amplification in ε-GaSe crystals
研 究 生:許哲睿 Student:Che-Jui Hsu
指導老師:潘犀靈 教授 Advisor:Prof. Ci-Ling Pan
國立交通大學
光電工程研究所
碩士論文
A Dissertation
Submitted to Department of Photonics and
Institute of Electro-Optical Engineering
College of Electrical Engineering and Computer Science
National Chiao Tung University
In partial Fulfillment of the Requirements
For the Degree of
Master of Engineering
In
Electro-Optical Engineering
July 2007
Hsinchu, Taiwan, Republic of China
硒化鎵晶體中兆赫波光參數放大之研究
研究生:許哲睿 指導教授:潘犀靈 教授
國立交通大學光電工程研究所
摘 要
以兆赫波時域光譜技術測量純的及掺鉺的硒化鎵晶體在兆赫波段的光學性質,我們 發現二者的折射率在0.2-1.2THz 波段約為 3.2,純硒化鎵晶體的吸收係數平均為 5 1 cm− , 掺鉺的硒化鎵晶體的吸收係數平均為55 1 cm− ,二者在0.589 THz 處都有一聲子吸收峯。 利用 Lorentz-Drude model 計算其導電率並以理論擬合可得知此二晶體的弛緩率及平均 碰撞時間,我們進一步推算其載子遷移率分別為μ=81cm Vs2 及μ =39cm Vs2 。 我們也架設了一套由高功率飛秒雷射聚焦游離空氣產生電漿,以空氣的三階非線性 係數滿足四波混頻的兆赫波產生源。改變雷射基頻(800 nm)及二倍頻(400 nm)間的相位 差、偏振方向夾角及強度,量測其產生的兆赫波的特性。並利用此光源來作硒化鎵晶體 中兆赫波光參數放大的研究,初步結果顯示在1THz 此光參數放大器有 150% 的增益。The study of terahertz optical parametric
amplification in ε-GaSe crystals
Student: Che-Jui Hsu Advisor: Prof. Ci-Ling Pan
Institute of Electro-Optical Engineering
College of Electrical Engineering and Computer Science
National Chiao Tung University
Abstract
Optical constants of pure and 0.2% Er:GaSe in 0.2 – 1.2 THz region are determined by THz-TDS. The refractive indexes for both crystals are 3.2 and absorption coefficients are 5 and 55 , respectively. A phonon vibration is observed at 0.589 THz for both crystals. By use of Lorentz – Drude model, the conductivity can be further calculated from experimental measurement. The parameters such as relaxation rate and momentum relaxation time are also derived. The mobility
1
cm− cm−1
2
81cm Vs
μ= for pure GaSe andμ=39cm Vs2 for
Er:GaSe are also proposed.
Femtosecond Laser induced plasma based on the third order nonlinearity is successfully utilized to construct the THz-TDS. The properties of the THz radiation from this configuration is characterized by altering the phase difference, the angle of polarization and intensity between fundamental beam (800nm) and second harmonic beam (400nm). Terahertz enhancement/amplification is preliminarily performed in our studies. The gain could be as high as 150% under the phase matching condition around 1THz.
Acknowledgement
首先誠摯的感謝指導教授潘犀靈老師,老師提供良好的實驗環境及細心的指導,使 我在求學的過程中學到不少專業知識及研究方法。 在實驗上耐心教導我的陳晉瑋學長,學長淵博的學識以及實驗嚴謹的精神,對我的 研究態度有了很大的影響;感謝王怡超學長在雷射系統的維護及調整,讓我有穩定的雷 射光源進行實驗;謝卓帆學長及黎宇泰學長在系統使用上的教導及建議。 此外感謝這二年來一起奮鬥的同學昀浦、韋文、彥毓、宜貞、君豪,不僅在課業及 實驗上的幫助,也給予我不少生活的美好回憶。學弟妹,育賢、介暐、孟桓、松輝、綿 綿、峻維的加入,也為生活增添了不少歡樂。 最後我要感謝我的家人,總是在背後默默的支持,沒有你們的栽培就沒有今日的我。Table of Contents
Abstract
...i.
Acknowledgements
...iii.
Table of Contents
...iv.
List of Figures
...vi.
List of Tables
...ix.
Chapter 1 Overview of Terahertz Radiation
1.
1.1 Introduction
1
1.2 Terahertz Generation Methods
4
1.2-1 Generation by Optical rectification
4
1.2-2 Generation by Photoconductive Antenna
6
1.2-3 Generation by laser induced plasma
8
1.3 Terahertz Detection Methods
9
1.3-1 Detection by Photoconductive Antenna
9
1.3-2 Detection by electric Optical Sampling
10
1.4 Laser System Used
15
1.5 The chacacteristics of THz Generated by Laser Induced
Plasma by Four Wave Mixing
16
Reference 23
Chapter 2 Optical Constant of ε-GaSe crystal in THz regime
24.
2.1 Introduction to GaSe
24
2.1-1 GaSe properties
24
2.1-2 The growth of GaSe
28
2.2 Analysis Method
29
2.2-1 Analysis Method of Optical Constant from THz-TDS
29
2.2-2 Lorentz Model and simple Drude Model
32
2.3 Experimental setup
34
2.4 Experimental Results
35
2.4-1 Raman spectroscopy
35
Reference
43
Chapter 3
Study of Optical parametric Amplification
in Terahertz
44.
3.1 Introduction to Optical Parametric Amplification
44
3.2 Theory of OPA
46
3.2-1 Coupled Wave Equations
46
3.2-2 Pump non-depletion condition
48
3.2-3 Pump depletion condition
49
3.2-4 Group Velocity Mismatch
50
3.2-5 Effective length
52
3.2-6 Phase Matching and Phase Matching Bandwidth
53
3.2-7 Theoretical prediction of THz-OPA
55
3.3 Experimental Setup
60
3.3-1 Setup of THz-OPA
60
3.3-2 Indium-tin-oxide-coated glass(ITO)
62
3.4 Experimental Results
62
Reference 67
Chapter 4 Conclusions and Future Work 68.
4.1 Conclusions
68
List of Figures
1-1
Overview of frequency regions. 11-2
Illustration of terahertz radiation by optical rectification 51-3
Schematic of PC antenna 61-4
The scheme of EO sampling setup 111-5
Angles of the THz wave and probe beam polarization directions 131-6
The scheme of femtosecond laser system 151-7
Schematic of the laser induced plasma setup used for THz generation 171-8
The THz time domain waveform inset: its corresponding frequencydomain 18
1-9
Terahertz radiation from BBO versus its azimuthal angle 191-10
Terahertz radiation from plasma versus the azimuthal angle of BBO 191-11
THz amplitude versus the distance from BBO to focus point 201-12
THz amplitude versus laser pulse energy 212-1
The atomic configuration of ε-GaSe 252-2
Absorption spectra for e-ray in GaSe, CdSe, GaP, GaAs,LiTaO3,LiNbO3 272-3
The cleaved surface of GaSe 292-4
Schematic of multi-reflection structure of sample 292-6
Raman spectra of pure GaSe, 0.2% Er:GaSe, 0.5% Er:GaSe 362-7
The terahertz time domain waveform. Inset: The corresponding frequencyspectrum 37
2-8
The real part of refractive index of pure GaSe and 0.2% Er:GaSe 382-9
The imaginary part of refractive index of pure GaSe and 0.2% Er:GaSe 392-10
The absorption coefficient of pure GaSe and 0.2% Er:GaSe 392-11
The real part of conductivity of pure GaSe and 0.2% Er:GaSe 402-12
The imaginary part of conductivity of pure GaSe and its theoretical fitting 412-13
The imaginary part of conductivity of 0.2% Er:GaSe and its theoreticalfitting 41
3-1
Geometries of OPA 453-2
Schematics of group velocity mismatch of ultrashort optical pulse in themedium 50
3-3
Illustration of Aperture length 533-4
Signal wavelength versus corresponding external phase matching angle 563-5
GVM between signal and pump versus signal wavelength 573-6
GVM between idler and pump versus signal wavelength 583-7
Idler intensity versus to the crystal length 593-8
Calculated gain versus to the crystal length 593-9
Pump intensity versus to the crystal length 603-10
The experimental setup of THz-OPA 613-12
THz transmittance versus the pump intensity 633-13
Gain coefficient calculation 643-14
THz-OPA phase matching curve 653-15
Seeded and amplified THz time domain profile 65List of Tables
1.1
List of THz emitters and detectors and their advantage 21-2
The description of Tsunami and Spitfire 162-1
Properties of some common used crystals, GaSe, ,KDP, , 3 LiNbO 2 ZnGeP AgGaSe2 262-2
Fitting parameters 40Chapter 1
Overview of Terahertz Radiation
1.1
Introduction
After the rapid progress in ultrafast lasers and the successes in semiconductor technology and nonlinear optics, it has leaded the birth of a new area of applied physics known as optoelectronics or photonics in 1970s. One of the most promising photonic spectroscopic applications, is the terahertz time-domain spectroscopy (THz-TDS), is now barely 15 years old.
Figure 1-1 : Overview of frequency regions. [1]
1 THz can be presented as: 1 THz = 1 ps = 300μm = 33 cm−1 = 4.1 = 47.6K.
Even though the terahertz (THz) region lies between microwave and infrared regions is relatively narrow (see Figure 1-1), it is important in condensed matter physics.
There are as many interesting phenomena falling right to this region, especially the soft lattice vibrations in dielectrics. The microwave wave region can be accessible via conventional radiofrequency methods, which cannot be extended as the frequency of synthesizers is limited. In the infrared region, the optical devices are used, however, while the frequency is lowered, the brightness of common infrared radiation sources practically vanishes.
The development and spread of THz sources and receiver advance the THz time-domain spectroscopy. Table 1-1 is the list of common use of THz emitter and detector. As the THz spectroscopy is a time-domain method, the pump-probe experiments can be easily performed. The sample can be excited by the optical pump beam, which is split from the femtosecond laser beam the pump beam is perfectly synchronized with the THz probe pulse and gating pulse. During last few years, the femtosecond optical amplifiers and parametric generators became commercially available. The regenerative amplified laser enabled us to generate a very intense excitation pulse and the latter to tune the excitation wavelength. This makes the THz time-domain spectroscopy very suitable for investigations of ultrafast dynamics on the subpicosecond time scale.
Table 1-1 : List of THz emitters and detectors and their advantage
Emitter Type Advantage
Free electron laser Highest THz power
Gunn oscillator Generate sub THz
Differential frequency generation Narrow linewidth CW possible
Photoconductive antenna High SNR
Semiconductor surfaces Higher THz power
Optical rectification broadband THz spectrum
Detector Type Advantage
Bolometer incoherent radiation, more sensitivity
Pyroelectric detector incoherent radiation
Photoconductive dipole antenna Higher SNR
Electro-optic crystal broadband THz spectrum
In recent years, THz spectroscopy systems have been applied to a variety of domains, such as material characterization, image and tomography, biomaterial application. The ability of THz-TDS to measure both real and imaginary components of the dielectric function in real time has made it a desired method to study the materials at THz frequencies. THz spectroscopy in chemistry and biology is another area of studies. Rotational, bending, and torsion dynamics of molecules can be probed by THz waves. In addition to the gas phase, the dynamics of molecules in condensed phases can be studied. Using subpicosecond waves one can study relaxation processes, and high THz fields can induce interionic motion or molecular orientational motion, changing the local structure. Imaging is also a very promising field of study and application. THz radiation can be applied to medical imaging of skin, teeth, etc. Unique biological
resonances are the basis for THz signature imaging employed to identify disease. Pharmacists can also benefit from THz spectroscopy. Drugs can be differentiated and identified using THz spectroscopy by different forms of the same compound with different pharmaceutical activities.
1.2 Terahertz Generation Methods
1.2.1
Generation by Optical rectification
The generation of terahertz by optical rectification method is only possible by pulsed laser. Optical rectification is the generation of DC polarization by the application of optical waves in a non-centrosymmetric medium with large second order susceptibility χ(2).
Assume a femtosecond pumping pulse propagates in z-direction, pulse durationτG
with Gaussian profile.
2 0
( ) ( ) exp( ( G ) 2)
I ω =I ω −τ ω (1)
When it propagates through the nonlinear optical crystal, there will be induced polarization in the crystal
(2)( , ) (2)( ) ( ) exp( ) g
P z ω =χ ω ωI −ωz v (2)
where v is the group velocity of pump pulse. g
By solving nonlinear Maxwell’s equations
2 (1) 2 (2)
2E 1 ∂ D 4π ∂ P
The locally generated terahertz electric field
2 (2)
( , ) ( ) ( 2)
THz THz
E z ω =ω χ ω zsinc kΔ z (4)
Then the generated terahertz is integral of local generation.
If these are no momentum mismatch, the output signal follows the intensity envelope of the pump laser pulse. For example, we use 100 fs pulses as the pump. The spectrum of the generated pulse peaks around a few terahertz.
Because the ultrafast pulses have large bandwidth, the frequency components are differentiated with each other and the produced signal have frequency component from 0 to the bandwidth of the pump ~ 1 ~ 10
G
THz
ω τ
Δ . The current record for THz
detection is 70THz [2]. Figure 1-2 illustrates the terahertz radiation generated by optical rectification.
Figure 1-2 : Illustration of terahertz radiation by optical rectification
Laser pulse Δω~1/Δτ THz pulse
1.2.2
Generation by Photoconductive Antenna
Femtosecond laser excites a biased semiconductor with photon energies greater than its bandgap, will produce electrons and holes at the illumination point in the conduction and valence bands (Figure 1-3). Owing to fast changing of the density of the carriers and accelerated by the applied dc bias, electromagnetic field radiating into free-space. The production of currents with a full-width half-maximum (FWHM) of 1ps (or less) depends on the carrier lifetime in the semiconductor [3].
Bias Voltage Pump beam THz radiated Bias Voltage Pump beam THz radiated
Figure 1-3 : Schematic of PC antenna
The carrier density behavior in time is given by
/
/
tcarriers due to laser pulse excitation, with Δt the laser pulse width and n0 the
generated carrier density at t = 0. The generated carriers are accelerated by the bias field with a velocity rate given by
,
/
,/
(
,)
e h e h rel e h eff
dv
dt
= −
v
τ
+
q E m
/
, ,e h (6)where are the average velocity of the carrier, are the charge of the electron and hole,
, e h
v
q
e h,rel
τ is the momentum relaxation time, and E is the local electric field,
which is less than the applied bias Eb because of the screen effect of space charges.
The relation is
/ 3
bE E
=
−
P
ε
r (7)where εr is the dielectric constant and P is the polarization induced by the
separation of electrons and holes. The polarization depends on time according to the expression
/ / rec
dP dt = −P
τ
+J (8)where τrec is the recombination time between electrons and holes (τrec= 10 ps for LT-GaAs) and J= envh + (–e)nve is the current density.
The far-field radiation is given by
/
/
THz
E
∝ ∂ ∂ ∝ ∂ ∂ + ∂ ∂
J
t
ev n
t en v
/ t
, (9) where v = ve – vh. The transient electromagnetic field ETHz consists of two terms: thefirst term describes the carrier density charge effect while the second term describes the effect of charge acceleration due to the electric field bias.
1.2.3 Generation by laser induced plasma
In 1993, Hamster et al. first observed terahertz emission from laser-induced plasmas. This is a very novel method of generating terahertz which is emitting from laser induced plasma based on amplified laser systems. The basic concept of these emitters is to focus an ultrafast high energy laser pulse in a gaseous medium such as ambient air. Reaching optical field strengths as high as 5 10 W cm× 14 2which is enough to
ionize the air and form a plasma in the focal region.
Up to now, there are three different methods to generating terahertz from plasma as our knowledge:
1. Emission based on ponderomotive force
The mechanism is that the polarization produced by the free electrons that are accelerated by the ponderomotive forces associated with the propagating laser pulse, i.e. due to a spatio-temporal optical intensity gradient within the plasma. In this method, a rotationally symmetric polarization is created around the beam propagation axis, this leads to an emission of terahertz radiation in a diverging cone about the optical propagation axis. Due to symmetry reasons no net terahertz field radiates along the optical propagation axis. [4]
Compared to other two methods employing laser-induced, the pulse energy of the terahertz generated by this method is relatively low.
2. Emission based on external bias fields
This method is applying an external bias field to the plasma region. It can increase the terahertz radiation strength and to direct it into the forward direction of the optical propagation axis. The terahertz pulse amplitude scales linearly with the external bias
field. The maximum achievable terahertz pulse energy for a given laser pulse energy is limited by the maximum external bias field. [5]
3. Emission based on optical second harmonic bias
This method is more efficient than above two, when laser pulses composed of a superposition of both fundamental and second harmonic spectral components which are focused into air.
Cook et al. initially attributed the terahertz generation process to four-wave rectification mediated by the third order nonlinearity of air [6] but later reported indications for a plasma-driven process [7]. In the four wave rectification process, the frequencies of the three input beams add to nearly zero (THz frequency) and the nonlinear polarization in the focal region and respectively the terahertz field amplitude are given by
(3) * *
2
( ) ( ) ( ) cos( )
THz plasma
E t ∝P ∝χ E E t E tω ω ω ϕ (10)
Where χ(3)( : 2Ω ω+ Ω −, ω,−ω) is the third order susceptibility, E
ω and E2ω is
the electric field of fundamental wave and the second harmonic wave, respectively.
2
kω l
ϕ = Δ
2
k
is the phase difference between the fundamental and second harmonic beams, ω is the wave vector of the second harmonic beam and is the path difference between the fundamental wave and the second harmonic wave along the beam propagation direction.
l
Δ
1.3 Terahertz Detection Methods
In 1984, Auston first generated and detected the THz pulses by photoconductive antennas [8]. In photoconductive antennas detection the antenna is gated with a femtosecond pulse. The gating pulse creates carriers and the terahertz pulse provides the bias field to create a detectable current in the detection antenna. The output polarity is sensitive to the direction of the field. The output is typically connected to a computer via a lock-in amplifier so that when the delay of the gate pulse is scanned over a several picoseconds region the electric field of the terahertz pulse is mapped out on the screen. For several years it was thought that the length of the optical gating pulse and the decay rate of the semiconductor were crucial to the detector responsitivity and time resolution. It was therefore assumed that no advantage could be gained from using shorter gating pulses, as the carrier lifetime of the carriers would always determine the response time of the detector. This in turn would therefore limit the detection capability of a typical GaAs photoconductive antenna to low frequencies.
1.3.2
Detection by Electric Optical Sampling
In 1995, the free space electric optical sampling (FEOS) detection scheme was first introduced by the groups of X.-C. Zhang. [9] This method has widely used and allowed for coherent detection of the temporal evolution of the electric field in the ultrashort transients.
ΔI Balanced detector Wallaston prism Probe beam λ/4 plate <110>ZnTe THz Beam
Figure 1-4 : The scheme of EO sampling setup
Figure 1-4 is the schematic of FEOS setup, it consists of EO crystal, quarter wave plate (or compensator), wallaston prism, balanced detector.
First, when there is no terahertz field present, the optical probe beam will not be affected by the EO crystal, then by rotating the angle of quarter wave plate, to make the polarization become circularly. This circularly polarized beam will be split into two orthogonal polarization components (s- and p-polarization) with equal intensity. The balanced detector measures the intensity difference between these two components, the value is zero. When terahertz meet the EO crystal, the electric field of a teraherz pulse will induce a small birefringence in an EO crystal through Pockels effect. Passing through such crystal, the initially linearly polarized optical probe beam will change into elliptical polarization. This ellipticity is proportional to the electric field which applied to the crystal. Then the elliptical polarization probe beam will be split into two orthogonal polarization parts by wallaston prism. The difference can be detected by balanced detector, terahertz amplitude is proportional to the signal. In
general, the duration of terahertz pulse is several picosecond (or subpicosecond) much longer than the laser pulse (femtosecond order), the terahertz field can be approximately treated as a dc bias field. Thus, by scanning the delay between terahertz and probe beam the whole terahertz time domain profile can be figured out.
The balanced detection signal for an EOS crystal such as <110> ZnTe can be calculated. ZnTe is a very common EO crystal used in terahertz EO sampling. It belongs to zinc-blende structure with 43m point group symmetry, the only nonzero coefficient of the electro tensor is γ41.
41 41 41 0 0 0 0 0 0 0 0 0 0 0 0 0 0 0 ij γ γ γ γ ⎡ ⎤ ⎢ ⎥ ⎢ ⎥ ⎢ ⎥ = ⎢ ⎢ ⎥ ⎢ ⎥ ⎢ ⎥ ⎢ ⎥ ⎣ ⎦ ⎥ (11) γ41=3.9 pm V
Here describe the angle ψ dependence of the signal in EO sampling with (110) ZnTe. When an arbitrary electric field EJG=( ,E E Ex y, z) propagate along the (110) axis is applied to the EO crystal, in the crystal axes coordinate system (x, y, z), the refractive index ellispsoid can be written as
2 2 2 41 41 41 2 2 x 2 y 2 z o x y z E yz E zx E xy n γ γ γ + + + + + 1 = (12)
After rotating the (x, y, z) coordinate system around the z axis by 45°, the equation (12) becomes:
Z’’ Z(001) ,Z kp Y(010) kTHz X’ Ep φ α θ ETHZ X (110) ZnTe Y’’ Y
Figure 1-5 : Angles of the THz wave and probe beam polarization directions
2 2 41 2 2 2 2 2 41 41 1 1 1 1 1 1 1 1 ( 2 2 ) ( 2 2 ) 2 ( 2 2 ) 2 2 2 2 2 2 1 1 1 1 2 ( 2 2 ) 2 ( ) 1 2 2 2 2 x o o o y z z x y x y E r x n n n E r x y z E r x y y z ′ ′− ′ + ′+ ′ + + ′+ ′ ′ ′ ′ ′ ′ + − + − = ′ (13) And Ey = − Ex 2 2 2 41 41 41 2 2 2
1
1
(
z)
(
z)
2 2
x o o oz
x
E r
y
E r
E r y z
n
n
n
′
′
+
+
′
−
+
+
′ ′ =
1
(14)Then the (x’, y’, z’) coordinate system is rotated around the x’ axis by θ :
θ
θ
θ
θ
cos sin sin cos z y z z y y x x ′′ + ′′ = ′ ′′ − ′′ = ′ ′′ = ′ (15)of the THz beam polarization with respect to the (001) axis) shown in Figure 1-5.
cos
2
sin
2
z THz x THzE
E
E
E
α
α
=
=
(16)With these definitions and some calculations, the index ellipsoid of Eq. (14) becomes:
2 2 2 41 41 2 2 2 2 41 2 1 1
( cos ) { [cos sin cos( 2 )]}
1
{ [cos cos cos( 2 )]} 1
THz THz o o THz o x E r y E r n n z E r n
α
α
θ
α θ
α
θ
α θ
′′ + + ′′ − + + ′′ + − − + = (17) And 1 2 tan (2 tan ) 1 1 ( ) ( ) , 0,1... 2 2 n n n n θ α π π α π − = − − − ≤ < + = (18)By setting " 0 ( " "x = y z plane), then solve the equation, we can get two eigenvalues.
2 0
2
1,2 41
1
[cos sin cos( 2 )]
THz
E n
λ = −γ α θ ± α+ θ (19)
The refractive indices for visible-near IR light propagating along the x” direction are: 3 2 0 0 41 3 2 0 41
( )
[cos sin
cos(
2 )]
2
( )
[cos cos
cos(
2 )]
2
y THz z THzn
n
n
E r
n
n
n
E r
α
α
θ
α θ
α
α
θ
α θ
′′ ′′≈ +
+
+
≈ +
−
+
(20)The intensity detected by balance detector can be expressed as:
(21) ,, ,, 3 41
( , )
sin[2(
)]sin{ [ ( )
( )] }
(cos sin 2
2sin cos2 )
p y z o THz
I
I
n
n
L
c
n E r L
I
ω
α ϕ
ϕ θ
α
α
ω
α
ϕ
α
Δ
=
−
−
=
+
ϕ
where L is crystal length, φ is the angle of the probe beam polarization with respect to
the (001) axis shown in Figure 1-5.
The optimum signal can be realized at the largest phase retardation if 2 n n, 0, 1, 2...
α + θ = π = ± ± which means terahertz beam should be parallel or perpendicular to probe beam to get maximum detected signal.
1.4 Laser System Used
Figure 1-6 is the laser setup which is consisted of a Spectra-Physics Millennia V diode-pumped laser that generates 5W of green light that pumps a Tsunami Titanium-doped sapphire laser with output of approximately 35 fs pulses at 800nm. The pulse repetition rate is 82 MHz and the output power is up to 500 mW.
Millennia V Ti:Sapphire laser (Tsunami, Spectra-Physics)
Ti:Sapphire Regenerative amplifier (Spitfire, Spectra-Physics)
800 nm, 35fs, 500mW
Empower
800 nm, 50 fs, 2mJ
Figure 1-6 : The scheme of femtosecond laser system
The Ti:Sapphire beam is then directed into the Spitfire Ti:Sapphire regenerative amplifier system as the seeder. The pump beam for the amplification process in the Spitfire is Spectra-Physics Empower, a frequency doubled diode-pumped Nd:YLF
laser (527nm). The Spitfire amplifies the original seed pulses by a million times from 3nJ of energy per pulse to 2mJ per pulse, repetition rate 1KHz, or generates 20mJ pulse energy at repetition rate of 10Hz. Table 1-2 is the description of Tsunami and Spitfire.
Table 1-2 : The description of Tsunami and Spitfire
Laser Tsunami Spitfire
Repetition rate 82MHz 1KHz 10Hz
Wavelength 800nm 800nm 800nm
Pulse duration 35fs 50fs 50fs
Pulse energy 6nJ 2mJ 20mJ
1.5 The Characteristics of THz Generated by Laser
Induced Plasma by Four Wave Mixing
With the coming of the amplified laser system, one can easily reach pulse energy sufficient to ionize atoms and molecule in ambient air in the focused beam. If it is in an ambient air at 1 atm pressure, a plasma can be generated with a length of a few millimeter and a diameter of up to 100 μm can be produced by a 1 kHz Ti:Sapphire amplified laser system with pulse energies in the few hundreds of micro-joule regime.
plasma 100 μm-thick BBO
Lens, f=20cm
Figure 1-7 : Schematic of the laser induced plasma setup used for THz generation
Following the approach of Cook et al.[10], we construct a setup of terahertz time domain spectroscopy system with laser induced plasma to generate terahertz. Figure 1-7 is the illustration of terahertz generation setup, we employed 1kHz Ti:sapphire laser system (Spitfire) at 800nm with maximum pulse energy of 2 , pulse duration 50fs. We focus the pluses through a
J
m
100 mμ thick type-I β-barium borate (BBO) crystal with a lens (f=20 ), which has been phase matched for second harmonic generation (SHG), placed at an adjustable distance from the focus point. The generated terahertz is detected by free space EO sampling with 1 thick ZnTe crystal. The terahertz time domain electric field is shown in Figure 1-8, and its corresponding frequency domain spectrum is depicted in the inset.
cm
0 5 10 15 -0.0030 -0.0015 0.0000 0.0015 0.0030 THz am plitude (a .u.) delay(ps) 1 2 3 0.00000 0.00001 0.00002 0.00003 0.00004 0.00005 0.00006 Frequency (THz) A m pl it ud e FF T
Figure 1-8 : The THz time domain waveform inset: its corresponding frequency domain
First, we rotate the BBO crystal against the beam axis which means varying the angle between fundamental beam (ω ) and second harmonic beam (2ω ). But during the
experiment we found that there was terahertz which generated from the BBO crystal. By use of a teflon to block the laser beam behind BBO, we can measure the terahertz radiation from the BBO crystal, see Figure 1-9. The solid line is theoretically expected sin ( )4 α of the SHG efficiency. The terahertz generated from BBO was
identified as optical rectification of fundamental beam. The terahertz radiation from BBO reach maximum when SHG efficiency is zero. Figure 1-10 show the terahertz signal generated by four wave mixing that is numerically subtracted the signal generated by BBO because the THz signal from BBO will overlap the signal from plasma. We can see that the maximum signal is at the angle ±40° to the maximum
0 50 100 150 200 250 300 350 400 -0.00006 -0.00004 -0.00002 0.00000 0.00002 0.00004 0.00006 0.00008 0.00010 0.00012 0.00014 TH z a m plitude [a .u.] BBO angle [o] THz generated from BBO SHG efficiency
Figure 1-9 : Terahertz radiation from BBO versus its azimuthal angle
0 50 100 150 200 250 300 350 400 -0.0035 -0.0030 -0.0025 -0.0020 -0.0015 -0.0010 -0.0005 0.0000 0.0005 0.0010 0.0015 0.0020 0.0025 T H z a m p li tu d e[ a. u .] BBO angle[o] THz generated from plasma SHG efficiency
Four wave mixing predicts that the generated THz signal is proportional to the third order nonlinearity, electric field of second harmonic wave, the square of electric field of fundamental wave and their relative phase ϕ.
(3) 2
2 sin( ) THz
E ∝χ E Eω ω ϕ (22)
We can change the phase by varying the distance d between BBO and the focus point.
The phase shift ϕ
2
(2n n )
c ω ω ωd
ϕ = − (23)
where n2ω and nω are the refractive index of air at frequency ω and 2ω .
Figure 1-11 shows that terahertz amplitude is varied by adjusting the distance from BBO to focus point. The moving range only from 4.9 to 6.3 is due to the damage threshold of BBO and its dimension area. The pump beam size is larger than BBO dimension area when the distance is larger than 6.4cm, and close to the damage threshold of BBO crystal when the distance less than 4.9 .
cm cm 4 6 8 10 -0.004 0.000 0.004 TH z a m pli tude [a .u.]
BBO to focus distance[cm]
measured fit
The blue-solid line is the theoretical fitting. Changing the distance d is not only altering the relative phase but also changing the SHG efficiency and the beam spot size on the BBO crystal. The SHG power conversion efficiency [11] is defined as
2 1 1 tanh ( (0) ) 2 SHG A z η = κ (24) where 3 2 0 0 2 d n μ ω κ ε ⎛ ⎞ ⎛ ⎞ =⎜ ⎟ ⎜ ⎟
⎝ ⎠ ⎝ ⎠ is the phase mismatch. And we can derive that
( )
1 sin tanh( ) THz E d ϕ ∝ (25) 0 100 200 300 400 0.0000 0.0005 0.0010 0.0015 0.0020 0.0025 THz a m p litu d e(a.u.)Laser pulse energy (μJ) fitting curve
THz amplitude(a.u.)
Figure 1-12 : THz amplitude versus laser pulse energy
We measured the THz signal intensity with varying the laser pulse energy before the BBO crystal, The results are shown in Figure 1-12, while the BBO angle was set at 185 and the distance ° d =4.7cm.
2 2
E ω ∝Eω ∝Iω (26)
Eq. (22) has quadratic dependence
(3) 2 THz
E ∝χ Iω (27)
The pulse energy below 300 Jμ can be fitted well with Eq. (27), but the THz signal falls below the fitted quadratic curve in the higher pulse energies portion. It may be likely due to the defocusing of the laser beam by the plasma and reduces the effective peak intensity. In addition, at larger plasma volumes, phase mismatch and THz absorption effects are more likely to become significant. [12]
Reference
[1] http://www.advancedphotonix.com/ap_products/terahertz_whatis.asp
[2] A.Leitenstorfer, et al., Detectors and sources for ultrabroadband electro-optic sampling: Experiment and theory Applied Physics Letters 74, 1516-1518 (1999).
[3] Masahiko Tani, et al , Generation and detection of terahertz pulsed radiation with photoconductive antennas and its application to imaging, Meas. Sci. Technol. 13 (2002) 1739–1745
[4] Hamster H, Sullivan A, Gordon S, White W and Falcone R W, 1993 Phys. Rev. Lett. 71 2715 [5] Loffler T, Jacob F and Roskos H G 2000, Appl. Phys. Lett. 77 453
[6] You D, Jones R R and Bucksbaum P H 1993 Opt. Lett. 18 290
[7] Darrow J T, Zhang X-C and Auston D H 1992 IEEE J. Quantum Electron. 28 1607
[8] Auston D H, Cheung K P and Smith P R 1984 Picosecond photoconducting Hertzian dipoles Appl. Phys. Lett. 45 284–6
[9] Q. Wu and X.-C. Zhang, Free-space electro-optic sampling of terahertz beams APL_vol67_p3523_1995
[10] D. J. Cook, Intense terahertz pulses by four-wave rectification in air, OL_25_1210_2000 [11] Photonics 6ed, Yariv and Yeh
[12] Markus Kress, Torsten Löff ler, Susanne Eden, Mark Thomson, and Hartmut G. Roskos, Terahertz-pulse generation by photoionization of air with laser pulses composed of both fundamental and second-harmonic waves, OPTICS LETTERS / Vol. 29, No. 10 / May 15, 2004
Chapter 2
Optical constant of ε-GaSe crystal
in THz regime
2.1 Introduction to GaSe
2.1.1 GaSe properties
Gallium selenide (GaSe) is a semiconductor belongs to the III-VI layered semiconductor family like GaS and InSe, which has relatively large direct band gap of about 2.0 at room temperature. There are four polytypes of GaSe (β-, γ-, δ- and ε-type) classed by the package type of separate layers and their amount in the unit cell. The methods of growing ε-GaSe crystal are mainly the Czochralski and Bridgman-Stockbarger methods. Gas transport reactions also yield the ε polytype with a large number of stacking faults. Needle crystals of γ, δ and ε polytypes are formed by vacuum sublimation.
eV
Figure 2-1 shows the structure of ε-GaSe, and atomic configuration of ε-GaSe layers. The ε-GaSe consists of two layers and crystallizes with the space group , three anions form a tetrahedron along with the metal atom. The atoms are located in the planes normal to the c-axis in the sequence of Se–Ga–Ga–Se. Each layer consists of two planes of Ga atoms and surrounded by the unit planes of the Se atoms on two sides. Two sheets of the same layer are bonded with a mixture of covalent and ionic bonds, but the layers are hold by weak van der Waal’s forces. Weakness of the
1 3h
electrical properties.
Figure 2-1 : The atomic configuration of ε-GaSe
It is highly transparent in the infrared region between the wavelengths 0.65 – 18 mμ , is also a promising candidate material for nonlinear optical conversion devices in the near- to far-infrared. Besides the removal of the constraint of the lattice mismatch, GaSe thin film has the advantages of stability to against heating and oxidation under the ultra high vacuum condition.
Due to its relatively large band gap energy of 2.0 , therefore impurity doping in GaSe has been investigated with a large amount of interest because of possible technical applications for photoelectric devices in the visible region. The electric and optical properties of GaSe doped with elements of groups I, II, IV, and VII have been reported by many researchers. [1]
eV
Such as low scattering loss, large birefringence and nonlinear coefficient, wide transparency range, low absorption coefficient and mechanical strength. Few crystals have above properties, , KDP, are often used, Table 2-1 is the properties of these crystals [2].
3
LiNbO AgGaSe2
Table 2-1 : Properties of some common used crystals, GaSe, LiNbO3,KDP, ZnGeP2,AgGaSe2
Crystals GaSe LiNbO 3 KDP ZnGeP 2 AgGaSe2
Nonlinear coefficient (pm V/ ) 22 63 d = d33 =25.2 d36 =0.7 d36 =70 d36 =43 Absorption coefficient(cm−1) 0.45 0.0042&c 0.0028⊥c 0.058⊥c 0.006&c 1.52 0.012-0.2 Refractive index no (at 1.064μm) ne 2.91 2.57 2.23 2.14 1.49 1.48 3.22 3.26 2.70 2.68 Transparency range (μm) 0.62~18 0.4~5.5 0.176~1.4 0.74~12 0.76~17
Among these nonlinear optical crystals, GaSe has a wide transparency range from a wavelength of 0.62 to 18 mμ with low optical absorption coefficient lower than
. The
1
refractive indices in the ordinary and extraordinary direction). It has high nonlinear optical coefficients among the top five birefringent crystals. Due to its large birefringence, it can satisfy phase matching (PM) conditions for optical configurations within the nonlinear optical crystals. Incoherent parametric generation tunable in the range of 3.5–18 mμ in GaSe (type–I PM) was obtained by using actively mode-locked Er:YAG laser as a pump source[3]. Besides, there are a number of reports about using difference frequency generation (DFG) to achieve widely tunable and coherent mid-IR for GaSe. Recently, numerous papers reported on terahertz generation from GaSe, because it has lowest absorption coefficients in the THz wavelength region, see Figure 2-2.
Figure 2-2 : Absorption spectra for e-ray in GaSe, CdSe, GaP, GaAs, , based on reference 4
3
Consequently, GaSe has the largest figure of merit ( 2 3 eff
d nα ) for the THz generation, 2
which is several orders of magnitude larger than that for bulk LiNbO3 at 1 THz. An
efficient and coherent high power THz wave tunable in the two extremely wide ranges of 2.7–38.4 and 58.2–3540 mμ , with typical linewidths of 6000 MHz, has been achieved by Ding’s group for the first time. [5]
2.1.2 The growth of GaSe
The GaSe crystals are grown and provided by Prof. Chen-Shiung Chang’s group in NCTU. GaSe crystals were grown by a vertical Bridgman method, this method is good for growing single crystal ingots.
This method involves heating polycrystalline material in a container above its melting point and slowly cooling it from one end where a seed crystal is located. Single crystal material is progressively formed along the length of the container. The process can be carried out in a horizontal or vertical geometry.
It is a popular method of producing certain semiconductor crystals, such as gallium selenide and gallium arsenide where the Czochralski process is more difficult.
c-axis
Figure 2-3 : The cleaved surface of GaSe
2.2 Analysis method
2.2.1 Analysis Method of Optical Constant from THz-TDS
As shown in Figure 2-4, the transmitted terahertz pulses propagate through the reference and sample. If the sample is thick enough, we can have a relatively clear separation in time between the main transmitted terahertz signal and the first refection signal which enable us to analyze the data on the main pulse only.
…
sample
i i ( ) ( , ) ( , ) exp( ( )) ( ) ( 1) exp( ) s s r r as sa E P d P d i E n d t t i c ω ν ν φ ω ω ≡ − = ω
where i ( )Er ω and i ( )Es ω are Fourier transform of E tr( ) and E ts( ), respectively.
( ,
s
P ν d) and Pr( , )ν d are the power transmittance for sample and reference.
n n= − iκ is the complex refractive index.
The refractive index n(ν) can be determined by the phase difference:
( ) 1 2
nν = + Δc φ πνd (1) and the absorption coefficient can be calculated by the transmittance:
( ) (1 ) ln[d Ps( , )d Pr( , )]d
α ν = − η⋅ ν ν (2)
η is the Fresnel reflection loss correcting factor due to the two sample/air interfaces.
These approximation experiments enabled the quite accurate determination of the refraction index n
( )
ν and absorption coefficient α ν of the sample crystal.( )
To analyze experimental data, one usually takes a model dielectric function which is the combination of one Drude peak and various Lorentz oscillators. Drude model can describe the free-carriers, and bound carriers can be described from the Lorentz model. Using the Drude-Lorentz model for the dielectric response analysis, we can extract parameters from the THz-TDS measured data, such as plasma frequencyωp, the
average momentum relaxation time τ , and the mobilityμ. The theoretical treatment is as follows:
and conduction band electrons in the terahertz region is given by [6]: 2 2 2 2 2 1 ( ) ( ) ( ) ( ) j j J j TO p j TO j n i S i i ε ω κ ω ω ε ω ω ω ω ω τ = = − = ∞ + − − − Γ +
∑
(3)where the summation is over the lattice oscillators with the strengthSj; the resonance
transverse optical phonon
ω
TOj ; the phonon relaxation rateΓ , and the average jmomentum relaxation time for carrier τ . The static dielectric constant is
,
dc jSj
ε =ε∞+
∑
ε∞ denotes the valance electron contribution to the high frequency dielectric function.From the Drude model approximation [6], the complex conductivity can be expressed as follows: l 2 0 ( ) (n i ) ( ) iσ ε ω κ ε ωε = − = ∞ + (4)
The complex conductivity can be presented as follows:
l( ) r( ) i i( )
σ ω =σ ω + σ ω (5)
Substituting Eq. (5) to Eq. (4), the real part and imaginary part of the conductivity can be derived as follows: 0 ( ) 2 r n σ ω = κωε (6) 2 2 0 ( ) ( ( ) ) i n σ ω =ε ω ε ∞ − +κ (7)
From Eq. (3) and Eq. (4), the complex conductivity can be described as follows: l 2 2 0 0 1 2 2 1 ( ) ( ) ( ) j j r i J j TO p j TO j i S i i i i σ ω σ ω σ ω ω ε ω ωε ω ω ω ω τ − = = + = − − − Γ +
∑
(8)The phonon resonance effect is also considered in Eq. (8). The measured real and imaginary part of the complex conductivity can be theoretical fitted by the following parameters: plasma frequency; the average momentum relaxation time, and the optical phonon frequency.
Furthermore, with average momentum relaxation time, we can calculate mobility can be expressed as follows:
e m
τ
μ = ∗ (9)
2.2.2 Lorentz Model and simple Drude Model
Lorentz modelThe simplest model to describe the response of the medium to an electromagnetic field is the Lorentz model. In that model we consider an electron of mass with charge which bound to the nucleus in a similar way a small mass can be bounded to a large one: m e 2 0 2 ( ) ( ) ( ) ( ) d r t d r t m m m r t e dt + Γ dt + ω = − K K K JK E t (10)
To solve the differential equation, first, we can take Fourier transform of Eq. (10)
(
2 2)
0 ( ) ( )
mω i mω mω r ω eE
− − Γ + K = − JKω (11)
2 2 0 ( ) ( ) ( ) eE r m i ω ω ω ω ω − = − − Γ JK K (12)
The induced dipole moment is defined as
( ) ( )
p ω = −er ω
JK K
(13)
If there are N atoms in the unit volume, then the net dipole moment per unit volume is: 1 ( ) NV i( ) ( ) i P p N p V ω =
∑
ω = JK JK JK ω (14) 2 2 2 0 0 0 2 2 2 0 ( ) 1 ( ) ( ) p P Ne E m i i ω χ ω ε ω ε ω ω ω ω ω ω = = − − Γ = − − Γ ω (15)Here we set plasma frequency
2 0 p Ne m ω ε = (16)
The dielectric function is
2 2 2 0 ( ) 1 p i ω ε ω ω ω ω = + − − Γ (17)
Simple Drude model
If we set ω0 = , means that no electrons are bounded , i.e. free electron, Eq. (10) 0 becomes 2 2 ( ) ( ) ( ) d r t d r t m m e dt + Γ dt = − K K JK E t (18)
This is the well known Drude model used to describe the low frequency response of metals.
2 ( ) ( ) ( ) eE r m i ω ω ω ω = + Γ JK K (19) 2 2 ( ) p i ω χ ω ω ω = − + Γ (20) The current density is
J =Ne v =σE
JK JK
(21)
The complex conductivity can then be derive
l 2 0 2 1 2 ( ) Ne i i p m i i ε ω ω σ ω ω ω ω τ − = = + Γ + (22)
2.3 Experimental setup
We use mode-locked femtosecond Ti:sapphire laser (Spectra Physics Tsunami) as our light source. Figure 2-5 is the schematic of setup. The laser output is split into two beams, one is the pump beam; another one is the probe beam. The pump beam is focused on the emitter by an objective lens, a low-temperature grown Gallium arsenide (LT-GaAs) photoconductive dipole antenna is utilized. The generated THz pulses are collimated by gold-coated parabolic mirrors onto the sample. The transmitted pulses from the sample are focused by another parabolic gold mirror onto the THz detector, which is also a photoconductive antenna. The Ti:sapphire laser probe pulse that impinged on the LT-GaAs generates charge carriers and effectively turns the antenna on for a short time interval. The electrical signal of antenna detector is connected to a lock-in amplifier in order to increase the signal/noise ratio (SNR).
With dry nitrogen purge RH<5% Sample BS Detector Emitter THz-TDS
Figure 2-5 : The experimental setup of the PC antenna based THz-TDS
2.4 Experimental Results
2.4.1 Raman spectroscopy
The Raman scattering measurements were performed by a Jobin-Yvon U1000 Raman system [7]. The Raman spectra were excited by using the 514.5 nm line from an Argon-ion laser with a notch filter to filter out the Rayleigh scattering of the laser. Raman signals were collected by the double-grating spectrometer and detected by a LN2 cooled charge coupled device (CCD).
0 100 200 300 400 500 1000 1500 2000 2500 3000 117.2 112.5 115.3 78.0 133.0 211.5 306.6 Raman relati ve intensity shift
(
cm-1)
pure GaSe 0.2% Er:GaSe 0.5% Er:GaSeFigure 2-6 : Raman spectra of pure GaSe, 0.2% Er:GaSe, 0.5% Er:GaSe
The measured Raman spectra data are showed in Figure 2-6. There are phonon frequencies at 78cm−1, 115.3cm−1, 133.0cm−1, 211.5cm−1, 306.6cm−1, for pure GaSe,
0.2% Er:GaSe and 0.5% Er:GaSe. These are coincidence with the report [1], except 78cm−1. The low frequency band 19cm−1, 60cm−1 in reference 1 were not observed
because of the noise background of laser. At 115.3cm−1, 0.2% Er:GaSe has higher
Raman intensity, it may be due to the better crystalline. The splitting peaks at 112.5 and 117.2 for 0.5% Er:GaSe, it may be likely due to the defects in the crystal.
1 −
cm cm−1
continuously infusing to THz-TDS system to reduce water vapor absorption of THz radiation. The inset of Figure 2-7 is the frequency spectrum of the measured THz radiation. The signal to noise ratio (SNR) is about 1000000:1, and the absorption lines of water vapor at 0.557, 0.752, 0.988, 1.097, 1.113, 1.163, 1.208, 1.229 and 1.411 THz [7] are not existed.
We prepare two kinds of samples, pure GaSe and 0.2% Er:GaSe. The thickness of pure GaSe is about 669 mμ , 0.2% Er:GaSe is about 663 mμ .
0 1 2 3 4 5 10-23 10-22 10-21 10-20 10-19 10-18 10-17 10-16 10-15 10-14 10-13 10-12 10-11 Frequency (THz) P o we r FFT [ a .u.] 0 2 4 6 8 10 12 14 16 18 20 -0.0004 -0.0002 0.0000 0.0002 0.0004 0.0006 0.0008 T H z a m p litu d e [a .u .] delay[ps]
Figure 2-7 : The terahertz time domain waveform. Inset: The corresponding frequency spectrum
All the data are performed on the main pulse. Using the method in chapter 2.2.2, the real and imaginary parts of refractive index are shown in Figure 2-8 and Figure 2-9. The refractive index is approximately 3.2. A strong absorption peak is clearly
indicated at 0.589 THz. It can be attributed to an interlayer vibration of GaSe with E’-type symmetry. The presence of the low-frequency sharp peak of “rigid layer mode” at 19 cm-1 indicates the pure GaSe crystal to be in ε-phase. It is also clearly shown in the absorption spectrum, see Figure 2-10. The absorption coefficient of pure GaSe is below 10 from 0.2 to 1 THz. For 0.2% Er:GaSe, the average absorption coefficient is 55
1
cm−
1
cm− from 0.2 to 1 THz.
Using Lorentz-Drude model we can extract some parameters from the complex conductivity, such as plasma frequency; the average momentum relaxation time and the optical phonon frequency. The real part of conductivity of pure GaSe and 0.2% Er:GaSe is shown in Figure 2-11.
The measured and theoretical fitting of the imaginary part of complex conductivity is shown in Figure 2-12 and Figure 2-13.
0.4 0.6 0.8 1.0 1.2 2.6 2.8 3.0 3.2 3.4 3.6 3.8 4.0 pure GaSe 0.2% Er:GaSe n Frequency(THz)
0.4 0.6 0.8 1.0 1.2 0.0 0.2 0.4 0.6 0.8 1.0 pure GaSe 0.2% Er:GaSe k Frequency(THz)
Figure 2-9 : The imaginary part of refractive index of pure GaSe and 0.2% Er:GaSe
0.4 0.6 0.8 1.0 1.2 0 20 40 60 80 100 120 pure GaSe 0.2% Er:GaSe A b s o rp ti o n co ef fi cient ( cm -1 ) Frequency(THz)
0.4 0.6 0.8 1.0 1.2 -0 .5 0.0 0.5 1.0 1.5 2.0 R eal par t o f conduct ivity ( Ω −1 cm -1 ) F re q u e n cy (T H z) pure G aS e 0.2% E r:G aS e fitting curve
Figure 2-11 : The real part of conductivity of pure GaSe and 0.2% Er:GaSe
The measured real and imaginary part of the complex conductivity can be theoretical fitted by the following parameters: plasma frequency; the average momentum relaxation time, and the optical phonon frequency. The parameters obtained from fitting the measured experimental data are listed in Table 2-1.
Table 2-2 : Fitting parameters
Pure GaSe 0.2% Er:GaSe Phonon frequency ωTO 0.589 THz 0.589 THz Plasma frequency ωP 1.5 THz 22.05THz Momentum relaxation time <τ> 23 fs 10 fs Phonon 0.003 THz 0.0075 THz
relaxation rate Γj Oscillator strength Sj 0.06 0.085 0.4 0.6 0.8 1.0 1.2 0.0 0.5 1.0 1.5 Im
(
σ)
( Ω −1 cm -1 ) Frequency(THz) pure GaSe fitting curveFigure 2-12 : The imaginary part of conductivity of pure GaSe and its theoretical fitting
0.2 0.4 0.6 0.8 1.0 1.2 0.0 0.5 1.0 Frequency(THz) Im
(
σ)
( Ω −1 cm -1 ) 0.2% Er:GaSe fitting curveFigure 2-13 : The imaginary part of conductivity of 0.2% Er:GaSe and its theoretical fitting
31 0 9.1 10
m = × − kg . Therefore, the mobility of the pure GaSe is derived as 2
81cm V s
μ = , for 0.2% Er:GaSe μ =39cm V s2 . The mobility measured by Hall
Reference
[1] K. Allakhverdiev et.al , “Lattice vibrations of pure and doped GaSe, Materials”, Research Bulletin 41 (2006) 751–763
[2] David N. Nikogosyan, “Nonlinear Optical Crystals: A Complete Survey”, Springer
[3] K. L. Vodopyanov et.al, “High efficiency middle IR parametric superradiance in ZnGeP2 and GaSe crystals pumped by an erbium laser”, Opt. Commun. 83, 322 (1991).
[4] E. D. Palik, Handbook of Optical Constants of Solids, Academic, NY, Vol. I (1985);Vol. II (1991); and Vol. III (1998).
[5] Wei Shi and Yujie J. Ding, “A monochromatic and high-power terahertz source tunable in the ranges of 2.7–38.4 and 58.2–3540 mm for variety of potential applications”, APL 84 1635 2004 [6] B. L. Yu, F. Zeng, V. Kartazayev, and R. R. Alfano, “Terahertz studies of the dielectric response
and second-order phonons in a GaSe crystal”, Appl. Phys. Lett. 87, 182104 (2005). [7] http://rdweb.adm.nctu.edu.tw/page.php?serial=344
[8] Martin van Exter, Ch. Fattinger, and D. Grischkowsky “Terahertz time-domain spectroscopy of water vapor”, Opt. Lett. Vol. 14, No. 20 1989
[9] Yu-Kuei Hsu and Chen-Shiung Chang, “Electrical properties of GaSe doped with Er”, JAP, 96, 1563 (2002).
Chapter 3
Study of Optical Parametric
Amplification in Terahertz
3.1
Introduction to Optical Parametric Amplification
The field of nonlinear optics was initiated shortly after the demonstration of the laser with the experiment of second harmonic generation by Franken and colleagues in 1961. Due to the increase of power spectral brightness, the nonlinear experiment were possible be achieved.
Optical parametric amplifier (OPA) is one of second order nonlinear process. The process of OPA is similar to difference frequency generation (DFG), only differs from the initial conditions, the signal beam is much weaker than pump beam, after the interaction the signal beam can get significant amplification.
The second order nonlinear interaction is characterized by the generation of a nonlinear polarization 0 ( ) ( , , ) : ( ) ( ) p p p s i p p s s P ω =ε χ ω ω ωHG − E ω E ω JJK JJK JJK (1)
where (PJJKp ωp) is the nonlinear polarization at frequency ωp, ε0 is the dielectric
constant, (HGχ ω ω ω− p, , )s i is the nonlinear susceptibility, JJKEp(ωp) and EJJKs( )ωs are the interacting fields.
geometries, due to the different geometry, the two configurations have the different applications and characteristics. For example, collinear OPA has wider tuning range, non collinear OPA has broader bandwidth.
Figure 3-1 : Geometries of OPA
Consider three beams propagate and interact in a nonlinear medium, pump beam, signal beam, idler beam, at frequency ωp,
ω
s andω
i, respectively.In the interaction, the energy conservation should be satisfied.
p s i ω = ω + = = =ω i K (2)
At the same time, to make more efficient interaction, the momentum conservation (or phase matching condition) must be satisfied
p s kK =kK +k . (3) where kp, G s k G
and are the wave vectors of pump, signal and idler beam, respectively. This process leads to an increase in the signal photon flux and therefore the signal beam is amplified.
i
kG
According to the polarization of the three interacted beams, OPA can be classified by
Collinear OPA Non Collinear OPA
ks ki kp ks ks ki ks kp (2) χ (2) χ (2) χ
two types, type-I and type-II OPA. If both signal beam and idler beam have the same polarization and perpendicular to the polarization of the pump beam, that is type-I phase matching. If only one of the two beams have the same polarization with the pump beam, that is type-II phase matching. [5]
3.2
Theory of OPA
3.2.1
Coupled wave Equations
Started from Maxwell’s equations
0 0 D B E t B D H J t ∇ ⋅ = ∂ ∇× = − ∂ ∇ ⋅ = ∂ ∇× = + ∂ JK JK JK JK JK JK JK JK JK JJK JK (4) (5) (6) (7)
and the constitutive equations
0 r D=ε ε E JK JK JK P + (8) B=μ H JK JJK (9) 0 2 2 0 0 2 0 2 NL E H t E E t t t μ μ σ μ ε μ ∂ ∇×∇× = − ∇× ∂ ∂ ∂ ∂ = − − − ∂ ∂ ∂ JK JK JK JK JJK JK JK JJJK P (10)
Assume the medium is magnetically inactivity and monochromatic plane wave propagating in the near field in z-direction.
2 2 0 0 0 2 2 E E E z μ σ t μ ε t μ ∂ − ∂ − ∂ = ∂ ∂ ∂ 2 2 P t ∂ ∂ m − m − (11)
With i( , ) Re( imexp ( m )), (12)
m E z t =
∑
E j ω t k z ( , ) Re( exp ( )) i im m m P z t =∑
P j ω t k z (13) where i x or y= represents the direction of polarization, m p or s or i= the beam of interaction. Substitute Eq. (12) and (13) into Eq. (10) and apply slowly-varying-amplitude approximation (SVA)2 2 (d E) 2 (k dE dz dz) (14) We can derive 0 2 m m m E c m j P z n μ ω ∂ = − ∂ (15)
The nonlinear polarization components with envelope representation are
* 0 2 j kz s eff i p P = ε d E E e− Δ (16a) * 0 2 j kz i eff s p P = ε d E E e− Δ (16b) 0 2 j kz p eff s i P = ε d E E e+ Δ (16c) p s k k k k Δ =K K −K −Ki eff
d is called effective nonlinear optical coefficient, depending on the propagation
direction and polarization of the beam.
* s eff j kz s i p s d E j E E e z n c ω − Δ ∂ = − ∂ (17a) * i eff j kz i s p i d E j E E e z n c ω − Δ ∂ = − ∂ (17b) p p eff j kz s i p E d j E E e z n c ω + Δ ∂ = − ∂ (17c)
Eq. (17) can describe second order nonlinear phenomena, such as second harmonic generation (SHG), difference frequency generation (DFG), optical parametric amplification (OPA). By some manipulations, Eq. (17) can be cast into the form called Manley-Rowe relations, Eq. (18).
1 i 1 s 1 p i s p dI dI dI dz dz dz ω =ω = −ω (18) where 1 0 2 2 j j j I = ε cM E
3.2.2
Pump non-depletion condition
In a strong pumping field, the photon of signal beam stimulates the generation of additional the photon at signal wavelength and the photon at idler wavelength. Similarly, the generation of idler beam stimulates the generation of signal photon. Therefore, it will reinforce the generation of the photon of idler and vice versa, giving a positive feedback.
Consider the condition pump non-depletion, with initial conditions , initial signal beam amplitude
constant
p
E ≅
0 s
E and no idler beam generated Ei0 = 0