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DIPLOMA THESIS
Femtosecond Laser Induced Damage ThresholdMeasurements with Compressed Laser Pulses
Benedek Nagy
Supervisor: Dr. Peter Dombi
senior research fellow
Wigner Research Centre for Physics
Consultant: Dr. Zsolt Papp
assistant professor
BME Institute of Physics
Department of Physics
BME
2014
Nagy Benedek, the undersigned, Master of Physics student at the Budapest Uni-
versity of Technology and Economics declare that this Diploma Thesis was prepared
on my own, with the leading of the supervisor without any aid not allowed, I used
only the referred sources.
Every part I took from other sources word by word or in the same meaning, but
rephrased is cited with the source.
Budapest, January 2, 2014
signature
2
3
Contents
1 Introduction 5
1.1 Laser Damage and its Basic Phenomena . . . . . . . . . . . . . . . . 6
1.2 Models for Damage Mechanisms . . . . . . . . . . . . . . . . . . . . . 6
1.2.1 Theoretical Models . . . . . . . . . . . . . . . . . . . . . . . . 6
1.2.2 Dependence of Damage on Various Laser Parameters . . . . . 10
2 Methods and Instruments Used 13
2.1 ISO Standard Based and Other Measurement Procedures . . . . . . . 13
2.2 Lasers Used . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 15
2.2.1 Amplified Ti:S Laser System . . . . . . . . . . . . . . . . . . . 15
2.2.2 Long Cavity Ti:S Oscillators . . . . . . . . . . . . . . . . . . . 18
2.3 Measurement Setup . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21
2.4 Sample Optics Tested . . . . . . . . . . . . . . . . . . . . . . . . . . . 22
3 Results 25
3.1 Damage Thresholds of Different Optical Elements . . . . . . . . . . . 26
3.1.1 Damage Thresholds of Femtosecond Beam Steering Mirrors . . 26
3.1.2 Damage Threshold of Gratings . . . . . . . . . . . . . . . . . 27
3.1.3 Damage Threshold of Broadband Mirrors . . . . . . . . . . . . 29
3.2 Focal Spot Size Dependence of Damage . . . . . . . . . . . . . . . . . 29
3.3 Repetition Rate Dependence of Damage . . . . . . . . . . . . . . . . 31
3.4 Measurement Errors . . . . . . . . . . . . . . . . . . . . . . . . . . . 34
3.5 Alternative Real Time and Offline Diagnostic Techniques . . . . . . . 34
3.5.1 Thermal Camera . . . . . . . . . . . . . . . . . . . . . . . . . 34
3.5.2 ZyGO Interferometer . . . . . . . . . . . . . . . . . . . . . . . 35
4 Conclusion and Future Plans 38
4.1 Conclusion . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 38
4.2 Future Plans . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 39
References 40
4
1 Introduction
At leading high intensity femtosecond laser systems in the world, the optical damage
threshold of various optical elements used in the laser chain is a critical parameter.
Because of damage limitations, the laser beam has to be substantially expanded
at the duty amplifier stages of the system, resulting in the usage of large-aperture,
expensive optical elements (with up to 1 meter diameter in some cases). This rep-
resents a significant cost factor during the building of such a laser system.
The above technology is (or will be) used e.g. at the Rutherford Appleton Lab-
oratory (RAL), whose Astra Gemeni project is able to produce laser pulses with
focused intensity higher than 1021 W/cm2[1], at the National Ignition Laboratory
(NIF), where a 500 TW (1 TW= 1012 W) laser is planned to apply for fusion
ignition[2] and at the Petawatt-Field-Synthesizer (PFS) project at the Max-Planck-
Institut fur Quantenoptik (Garching), which aims to combine few-cycle pulse dura-
tions with petawatt scale peak powers[3] as well as at the Extreme Light Infrastruc-
ture (ELI), where the aim is to achieve femtosecond multi-PW (1 PW= 1015 W)
powered pulses[4]. It is a challenge to apply smaller and thus more cost-efficient
optical elements with higher damage threshold in these high energy ultrafast lasers.
Therefore, Laser Induced Damage Threshold (LIDT) investigations with femtosec-
ond pulses are necessary for developing and designing mirrors, gratings and optical
coatings[5].
In this Thesis I give an overview of my femtosecond LIDT measurements results.
LIDT is an important specification of optical elements such as mirrors, gratings,
etc. In high energy pulsed laser physics LIDT must be taken into account during
construction of a laser system. Therefore, LIDT measurements are inevitable for
various optical elements. The LIDT depends on the pulse energy, pulse duration,
pulse repetition rate and other parameters of the beam. There are various theories
describing the damage mechanisms that explain the measured effects. LIDT is better
known in the pico- and nanosecond region so experiments made by femtosecond
laser pulses are important. In this Thesis, I report on the results of my femtosecond
damage threshold measurements that I performed on various samples. Due to the
fact that there are only few comparable LIDT measurements with different repetition
rate lasers I report on LIDT caused by a 1 kHz and a 3.6 MHz repetition rate lasers
as well.
The structure of my Thesis is as follows. I briefly summarize the most important
terminology in the next subsection. In Subsection 1.2 I present models for damage
5
mechanisms and introduce earlier results on LIDT dependencies from other studies.
I will introduce basic measurement procedures, the lasers available in the laboratory
at the Wigner Research Centre for Physics, the applied measurement setup and the
detailed properties of the samples in subsections of Section 2. In Section 3 I present
my results on LIDT measurements. I close my Thesis with a short summary of the
results, a conclusion of the work performed and future plans in Section 4.
1.1 Laser Damage and its Basic Phenomena
Physical damage mechanisms of materials with large band gap (>3 eV) and in
picosecond pulse length region are ablation of atomic layers, conventional melt-
ing, boiling, formation of color centres, shallow strap and lattice defects[6]. In the
femtosecond region, Coulomb explosion due to various optical ionization processes,
plasma formation and thermoelastic breaking may occur as well[5].
An interaction is called optical damage if there is an irreversible alteration, prac-
tically visible on the surface of the material with a modern high resolution optical
microscope or some other suitable method[6]. Damage threshold is the minimum
power density which causes damage on the surface. The ablation parameter is a
quantitatively measurable parameter of the damaged surface, e.g. the depth or the
diameter of the crater. The ablation threshold is the optical power density which
causes ablation[6]. Below the damage threshold so called incubation is visible. These
are temporary defects not followed by ablation[7].
The common unit for LIDT is the peak fluence in J/cm2. This is given by[5]:
F = 2P
frep
cos θ
w20π
, (1)
where P is the average power, frep is the repetition frequency, θ is the beam angle
of incidence, w0 is the beam radius (1/e2 radius, assuming a Gaussian beam).
1.2 Models for Damage Mechanisms
1.2.1 Theoretical Models
In general, damage is caused at a critical electron density in the conduction band
(1016 − 1018 1/cm3), which corresponds to a critical power density where damage
occurs to the material. This critical electron density, and the corresponding critical
power density, is dependent on different parameters of the laser pulse.
6
In dielectrics with a band gap higher than 3 eV the few tens of picoseconds and
longer pulsed laser beam excites the conduction-band electrons and increases their
kinetic energy. This is transferred to the lattice and when the heat is sufficient,
damage occurs. This model predicts a τ12 dependence of the damage threshold on
the pulse length[6, 8] for longer than 20 ps pulses due to the time that the kinetic
energy of the electron transfers to the lattice. At the beginning the heat increases
at lattice defects, surface injuries where the absorption is higher than in the rest of
the material. For damage the temperature at the local absorption center needs to
increase near the melting point or the temperature where material cracking occurs.
The increase of the temperature is controlled by the thermal diffusion of the lattice
which leads to the τ12 scaling of LIDT. The typical time scale for the lattice to
transfer energy is 0.1-1 ps. This was observed for narrow band gap materials as
femtosecond region laser induced surface modification was monitored by von der
Linde et al. with a femtosecond time resolve microscope[9].
In the femtosecond region the electrons will be excited into the conduction band
from the valence band by photoionization, but they cannot transfer their energy
to the lattice due to the short time scale. Getting more energy from the radiation
of the laser, collisional avalanche ionization starts. Below a certain pulse length
the avalanche ionization effect is enough to cause damage. Decreasing the pulse
length more the LIDT decrease slows down hence the thermal effects have less
importance because the electron density in the conduction band is nearly permanent,
a saturation can be observed. However under 100 fs a drop can may be predicted in
the damage threshold[6] due to the predominance of multiphoton ionization. This
was measured by Mero et al. on Al2O3 [10] and by Stuart et al. on SiO2[6].
In dielectrics the band gap is quite wide, the conduction band is empty and the
material is often transparent. At infrared (IR) and near infrared (NIR) regions single
photon ionization is nearly impossible in wide band gap dielectrics with femtosecond
lasers. Measurements down to 7 fs were made[7]. At ultrashort pulse length non-
linear effects (multiphoton ionization, tunnel ionization) are able to transfer the
electrons to the conduction band. The kinetic energy of the charge carrier electrons
increase due to the additional laser radiation and above a critical kinetic energy
they transfer more electrons to the conduction band by collision, this is the collision
ionization. The newly freed electrons may get more energy from the laser radiation
and excite even more electrons to the conduction band and so on. This is the so
called avalanche ionization. Below 350 fs pulse length, tunnel ionization starts to
play role[7], but in certain processes only tunnel ionization can be dominant[11].
7
The ionized dielectric material reacts as a metal with a time dependent electron
density in the conduction band and thus kinetic energy of the electrons transfers to
the lattice by collision.
The description of the ionization procedure can be evaluated from the Fokker-
Planck equation[6] and leads to an electron density rate equation[7]:
∂ne
∂t=
nv − ne
nv
(wPI + newAI)−ne
τr, (2)
where ne and nv denote the electron density in the conduction and valence band
respectively, wPI the photoionization rate in 1/cm3s, wAI the avalanche ionization
rate in 1/s and τr to the electron relaxation time from the conduction band. At
low energies collision of two electrons is dominant which is accompanied by photon
radiation. At high energies three body collision may occur. In simpler models the
energy transferred to the photons or electrons is transferred simply to the electrons
in the conduction band. Although it is possible that the relaxation of the free
charge carriers leads to metastable self-trapped excitons (STE)[12]. STE increases
the ablation threshold for pulse length greater than 50 fs, thus decreases the maximal
kinetic energy of the electrons in the conduction band. Moreover, when the pulse
duration is higher than the recombination time, STE can be retransferred to the
conduction band by photoionization or avalanche ionization.
The photoionization process depends on the electromagnetic field as introduced
by Keldysh in his theory[13] which is often used nowadays as well. The Keldysh
parameter is
γ = ω
√m∗U
eEl
, (3)
where El is the electric field applied to the laser radiation, e is the elementary
charge, U is the band gap, m∗ is the electron effective mass and ω is the laser central
frequency. This parameter tells which type of ionization process is dominant for a
certain intensity, wavelength and ionization potential[14]. If the Keldysh parameter
is significantly below 1.5 tunnel ionization occurs, if it is much above 1.5 multiphoton
ionization plays role in the process and if it is approximately around 1.5 intermediate
of the tunnel and multiphoton ionization dominates. Whether the Keldysh theory is
valid for pulsed laser fields was questioned as measurement showed other results as
predicted by the theory[15], however it has been widely used and validated for other
cases in atomic and molecular physics as well as for various metallic photoemission
processes, therefore, I will also use this scale quantity.
According to the Keldysh theory multiphoton ionization dominates at low in-
tensity and tunnel ionization may be neglected[7]. However the effective band gap
8
decreases with the intensity of the laser in the Keldysh formula, the multiphoton
ionization is less significant and the real photoionization will be less than estimated
by the multiphoton ionization. At higher intensity the probability of tunnel ioniza-
tion increases and the process becomes dominant. Collision ionization occurs when
the energy of a free electron is high enough to excite another one from the valence
band to the conduction band. This energy level is above the ionization potential and
depends on the intensity of the laser and on the electron density in the conduction
band.
Once the electron is excited to the conduction band (with multiphoton or tunnel
ionization) it can decrease its energy by Joule-heat during the time of the laser pulse.
The time dependence of the thermal energy (Wth) can be written in the
∂neWth
∂t=
1
2σRE
2 − PimpneJeff (4)
form[8], where E is the electric field of the laser, σR is the conductivity, therefore12σRE
2 is the energy decrease of the electrons due to the Joule-heat, PimpneJeff is
the energy loss due to collision ionization as Pimp is the probability of ionization by
electron impact and Jeff is the band gap including the quiver energy of the electron
which means that the band gap J decreases due to the electron quiver and therefore
the electron needs less transferred energy.
It is an important issue what to define as LIDT in the models. A simple approach
based on the Drude-Lorentz model leads to critical electron density in the conduction
band[5]:
ncr =ϵ0ϵelm
∗
e2ω2, (5)
where m∗ denotes the effective mass of the electron, ϵel the susceptibility of the
bound electrons, ω the laser frequency, ϵ0 the vacuum permittivity and e to the
elementary charge. Various groups found that the typical critical electron density
is about 1021 cm−3[6, 10, 15, 16]. That is, near the critical density, the absorption
length is on the order of a wavelength. This implies that for a pulse just above the
damage threshold, a thin layer of dense plasma will be formed at the tail end of
the pulse. This layer will be even thinner as the material fully ionizes at intensities
above threshold[6]. The damage and ablation thresholds are often related to the
electron density in the conduction band, and particularly to the critical electron
density. When the electron density exceeds the critical electron density (ncr =
1.7 × 1021 cm−3 in fused silica for a laser wavelength of 800 nm[16]), the material
turns highly absorbing. The criterion ne = ncr thus appears as a necessary condition
9
for dramatic modification (ablation and/or damage) of a material, but in general
does not describe with the highest accuracy the exact numerical and experimental
conditions yielding such profound changes of the material[7].
It is important to mention that single shot and multiple shot LIDT may dif-
fer significantly as shown by the theories as well. As described above, there are
mechanisms that require multiple shots or in the case of one shot having insufficient
energy, multiple shots can transfer enough energy to start the mechanism which
leads to damage in the material. Therefore it is obvious that the LIDT decreases
as the number of pulses increase. Although above a certain number of pulses the
threshold fluence does not decrease significantly[17, 18], as the number of electrons
being trapped is proportional to the concentration of conduction band electrons
and pre-existing defect sites. This process will introduce additional energy levels
and excitation routes for the following laser shot. The relative strength of this pro-
cess to additionally initiate free and heated electrons by combined multiphoton and
avalanche ionization seems to decrease with increasing the number of pulses until
finally reaching a constant level[18].
1.2.2 Dependence of Damage on Various Laser Parameters
Dependence on pulse length As described above the LIDT peak fluence is
scaling with the square root of the pulse length (F ∝ τ12 ) in the picosecond region.
This dependence does not apply in sub picosecond region as there is not enough
time to transfer the energy to the lattice. Under 100 fs a break down in the a LIDT
peak fluence was predicted and proved by measurements[6, 10].
Dependence on pulse repetition rate There are only very few measurements
which investigated the LIDT dependence on various repetition rates and these mea-
surements are not matching either. Mero et al. performed measurements on a Ta2O5
single layer at 1, 10, 100 and 1000 Hz and did not observe significant changes or any
trends in the LIDT[17]. Hertwig et al. achieved similar results on ion-doped glass
sample[19]. In spite of these results Bonse et al. demonstrated a decreasing trend
in LIDT values, with measurements taken at 10, 100 and 1000 Hz on a Ta2O5/SiO2
high reflector multilayer[20]. One order of magnitude increase in the repetition rate
leads to approximately 25% decrease in the LIDT. Due to the sparse literature, it is
an important task to investigate the LIDT dependence on the pulse repetition rate
especially for higher repetition rates than 1 kHz.
10
Dependence on beam diameter Martin and Hertwig et al. studied the spot
size dependence of the LIDT[19, 21]. An earlier study was used to predict the
dependence published by DeShazer et al. in 1973[22]. The results matched well
with the theory therefore I briefly summarize it here. The model assumes Poisson
distributed defects and lower LIDT at a defect site. The probability of a defect site
got hit by a Gaussian laser beam is
P (w0) = 1− exp
[−π
8ln 2
(w0
d0
)2], (6)
where w0 is the Gaussian spot size and d0 is the average distance between defects.
For the next step, the model assumes the coating defects on the surface to have a
LIDT Fd much less than the intrinsic LIDT Fi. Therefore the total LIDT can be
given using the probability in Eq. (6):
F (w0) = FdP (w0) + Fi [1− P (w0)] . (7)
This leads to an increasing LIDT with the decrease of the spot size. It has to
be noted that the LIDT predicted by that model reaches a boundary Fd quite
quickly depending on the w0
d0ratio. Decreasing the beam diameter leads to Fi hence
F (w0 → 0) → Fi. Therefore increase or decrease of the spot size above and below a
certain one respectively does not influence the LIDT significantly.
Dependence on central wavelength There are many results available at 800 nm
due to the widespread use of Titanium-Sapphire (Ti:S) lasers. Therefore wavelength
dependent measurements are in the vicinity of 800 nm. The LIDT dependence on
the central wavelength can be summarized by using a study published by Jupe et
al.[16]. The avalanche ionization (WAI) rate is scaling linearly with the absorption
cross section (σ), and from the Drude model
σ =e2
cϵ0n0m
τc1 + ω2τ 2c
, (8)
where τc is the resulting collision time, ω is the laser frequency, m∗ is effective
electron mass, e the elementary charge, n0 is the photon number and ϵ0 is the vac-
uum permittivity. Multiphoton ionization provides a substantial contribution to the
damage mechanism for ultrashort laser pulses. Considering the large differences in
cross-sections of n and n+1 photon absorption, a quantized behavior of the damage
threshold is expected. The presented theoretical approach indicates clear steps in
the ionization characteristic behavior of the material with photon energies varying
11
over orders of the multiphoton process. Therefore, the LIDT should also show a
respective change at the transition point between the n and n+1 photon orders. A
step of between two and three photon ionization is approximately at 670 nm which
could be observed experimentally as well. Thus corresponding to this model the
calculated LIDT has a non-monotonous dependence on the wavelength: at all n and
n+1 photon orders it has a sharp step and then a slow relaxation until the next n+1
and n+2 photon order. This effect was measured by Ristau et al. as well[23].
In my experiments, I will focus on the following aspects of LIDT: I will compare
different sample optics, discuss the results on focal spot size and repetition rate
dependence focusing on a comparison between kHz and MHz repetition rates for
the first time to my knowledge.
12
2 Methods and Instruments Used
2.1 ISO Standard Based and Other Measurement Proce-
dures
The LIDT measurement procedure is mostly based on the ISO 112541 standards[24].
There are two main principles in the ISO standard. One is the 1-on-1 and other is
the S-on-1 measurement routine. The basics are that LIDT is measured by single
shot or S shot induced damage respectively. Therefore the procedure is different for
the two cases. The standard defines them as follows[24]:
1-on-1 A number of test sites are positioned into the beam and irradiated at differ-
ent energy densities or power densities. From this data, the damage threshold
can be determined. Test a minimum of 10 sites for each energy-density or
power-density increment. The range of pulse energies or beam powers em-
ployed shall be sufficiently broad to include points of zero damage frequency,
as well as points of 100% damage probability.
S-on-1 An unexposed test site is positioned into the beam and irradiated by a
series of Np pulses with a selected energy, Qtp, of the typical pulse. If damage
is observed by the on-line damage detection system before the series of Np
pulses is completed, stop the irradiation of the site and record the minimum
number of pulses Nmin. Repeat this procedure for different energy densities
of the typical pulse. The number of pulses, Np, shall be constant for the
entire test procedure and shall be selected such that the specific laser-induced
damage behavior of the specimen is registered by the S-on-1 test.
At both procedures the threshold is defined as the highest quantity of incident
laser radiation to the optical surface for which the extrapolated probability of dam-
age is zero. The probability corresponding to a certain energy differs with the two
methods. The probability is simply the ratio of the damaged sites and total number
of exposed sites on that certain energy for the 1-on-1 procedure. The probability
calculation for the S-on-1 process is more difficult and has to be done as described
here. The pulse energy scale is divided into a series of intervals (Q−∆Q,Q+∆Q)
covering the energy range accessible by the experimental set-up. For the calculation
of damage probability for a certain energy value, Q, and for a selected number, N ,
1There is a revision of the standard published in 2011 (ISO 21254) but the main principles are
the same.
13
of pulses, data points with Qtp(Q−∆Q,Q+∆Q) are selected from the file of data
points. Data points with Nmin ≤ N correspond to sites damaged, meanwhile data
points with Nmin > N or Np ≥ N correspond to sites not damaged during the test.
The damage probability for the energy, Q, is calculated by the ratio of the number
of data points corresponding to damaged sites with respect to the total number of
data points considered for the evaluation[24].
It must be mentioned that the papers published in this theme do not use the ISO
rule in general. The reason for this are different optics specifications which do not
match the ISO standard and makes another procedure acceptable. I also did not
apply the ISO standards strictly due to practical reasons. I performed a mixture of
the 1-on-1 and the S-on-1 procedures. I was able to measure the illumination time
but I was unable to stop the beam suddenly at a damage occasion. Therefore my
test was using the same number of pulses as in S-on-1 but the probability was only
the ratio of the damaged and all sites as in 1-on-1. The damage threshold fluence
was defined as the intersection of the linear fit of the data points and the y = 0
line as shown in Fig. 2 The test in practice used during my measurements works as
follows.
1. Direct a low power laser beam on the optical element at 10 different points
one after the other as shown in Fig. 1(a).
2. Record the histogram of the exposure sites as in Fig. 1(b).
3. If the surface is damaged, decrease the power, if it is not, increase it. Than
return to step 1.
(a) (b)
Figure 1: LIDT measurement [25]. Exposure sites shown on a mirror (a) and the
exposure histogram (b).
14
Figure 2: Damage probabilities of borosilicate glass and the determination of damage
threshold value from the measurement.
The exposure histogram can be recorded in a more obvious way (see Fig. 2.)
This way the LIDT may be read easily from the histogram. If the dependence on
different pulse attributes needs to be measured the procedure has to be repeated at
the desired pulse parameters.
2.2 Lasers Used
I used two different laser sources for damage measurements at Wigner Research
Centre for Physics. In this section these systems are introduced.
2.2.1 Amplified Ti:S Laser System
A mode-locked Ti:S laser with a Coherent LEGEND regenerative amplifier is used
at the laboratory of the Ultrafast and Attosecond Physics Group. The spectrum of
the pulse before and after the amplifier is shown in Fig. 3(a). The pulse length is
measured by an APE Mini autocorrelator. A typical measurement window is shown
in Fig. 3(b). The parameters of the laser beam after the amplifier are shown in
Table 1.
Laser Parameters at the Damage Workstation The laser described above
is used in other measurements in the laboratory as well. Therefore the parameters
at the damage workstation differs from the above, the maximum average power is
600 mW. The beam diameter depends on the lens built into the setup (see Fig. 10.),
the beam diameter in focus is 20 µm and 160 µm with a 200 mm and 750 mm
focusing lens respectively. I will call these focusing geometries medium and loose
focusing below.
15
(a) (b)
Figure 3: Spectra of the pulse before (black) and after (red) the LEGEND amplifier
(a). Pulse length measured by autocorrelator (b).
Parameter Value
Central wavelength (λ) 800 nm
Average power (P ) 4.1 W
Beam diameter at 1/e2, Gaussian-fit 9 mm ± 0.5 mm
Polarization Linear, horizontal
Repetition rate 1 kHz
Pulse length, FWHM (τ) 35 fs
Pulse energy stability rms 0.25 %
Pulse bandwidth, FWHM 30 nm
Table 1: Laser beam parameters after the amplifier.
In LIDT measurement it is very important to calculate the peak fluence. This
depends on the shape of the beam. I measured the beam profile with a Thorlabs
BC106-VIS CCD camera. The beam can be well fitted with a Gaussian (Fig. 4(a)
and 4(b)) hence the peak fluence may be calculated as already mentioned in Eq. (1)
(including the correction factor for Gaussian beams). The measurement results with
the 750 mm focusing lens are shown in Fig. 4 and 5.
I also applied a lens with short, 35 mm focal length to achieve tight focusing.
Due to the 6 µm pixel pitch of the camera I had to enlarge the focal spot with a
simple microscope objective and calibrate the magnification of the system. Thus
the size of the focal spot is 8.95 ± 0.23 µm and 9.04 ± 0.21 µm for the x and y
16
(a) (b)
Figure 4: Beam profile at the workstation measured with Thorlabs BC106-VIS CCD
with f=750 mm. Beam profile and Gaussian fit on the x axis (a) and y axis (b).
(a) (b)
Figure 5: Beam profile at the workstation measured with Thorlabs BC106-VIS CCD
with f=750 mm. 2D (a) and 3D (b) view of the profile.
Name Lens focal length (mm) Focal spot size (µm)
Tight 35 9
Medium 200 20
Loose 750 160
Table 2: A summery of the used focusing geometries and their notation.
directions, respectively. The diameter is measured at 1/e2 width. For the damage
measurements to be discussed below, these three focusing geometries are to be used
as summarized in Table 2.
17
(a) (b)
Figure 6: Scheme of a long cavity oscillator (a) and the circular pattern formed on
the M5 mirror in the so-called Herriott-cell (b). M1-M10: chirped and high reflector
mirrors, P1, P2: Brewster prisms, OC: output coupler, CP: compensation plate, L:
lens with 60 mm focal length, SESAM: semiconductor saturable absorber mirror.
2.2.2 Long Cavity Ti:S Oscillators
7.36 MHz Repetition Rate Oscillator Another light source to investigate dam-
age phenomena with is a long-cavity Ti:S oscillator of the same group. This provides
pulses with much higher energy than standard oscillators with a high (MHz) repeti-
tion rate[26]. Thus, we expect damage processes to behave substantially differently
than in the case of a beam with kHz repetition rate. A former student built this
laser[27]. My task was to put this laser to work with a new Ti:S crystal.
Therefore, I installed a new Ti:S crystal with an α = 4.95 1/cm absorption and
4.6 mm optical path length which was put into the laser head. Firstly, a short cavity
laser was set up with the new crystal where 1.5 W output power was achieved with
6 W pump power. Then, I set up the long cavity oscillator the scheme of which is
shown in Fig. 6(a). By extending the cavity, the repetition rate decreases and high
pulse energies can be achieved. The so-called Herriott-cell extends the cavity length
as the beam bounces between e.g. two mirrors, a spherical and a flat mirror in our
case[28]. The Herriott-cell is formed by the M5 and M6 mirrors together with the
M4 incoupling and M7 outcoupling mirrors. The Herriott-cell is not depicted fully
realistically, as the subsequent reflections form a circular pattern on the mirrors as
shown in Fig. 6(b). A certain combination of radii of curvatures, number of bounces
and mirror distances results in a net ABCD matrix of unity for the Herriott-cell.
Thus, introducing this into the cavity, oscillator stability is not compromised. In
18
(a) (b)
Figure 7: The spectrum of the chirped pulse oscillator (red line) together with the
reflectivity of the SESAM used (blue line) and the intracavity GDD of the laser (black
line) as a function of wavelength (a). The autocorrelation of 7.36 MHz repetition rate
oscillator measured by the APEMini autocorrelator (b). The FWHM is approximately
147 fs which corresponds to a 97 fs pulse length at FWHM.
the 7.36 MHz laser that I put into operation there are 7 such bounces from each
large-aperture mirror.
Thus, the laser cavity is 40 m long and the available continuous wave mode
(CW) power was 650 mW. The mode locking can be started by a semiconductor
saturable absorber mirror (SESAM). The best pulse was achieved by 680 mW mode
locked power (The highest power was 820 mW), and its spectra can be seen in
Fig. 7(a) (red line). The Figure also shows the reflectivity of the SESAM (blue line)
and the intracavity Group Delay Dispersion (GDD) of the laser (black line). The
repetition rate of the laser is 7.36 MHz, so the pulse energy is 92 nJ. I also built
the pulse compressor with which the achieved best pulse length was 82 fs, but the
average achievable is 93-99 fs, measured by an APE Mini autocorrelator as shown in
Fig. 7(b). The FWHM of the autocorrelation shown in the figure is approximately
147 fs which corresponds to a 97 fs pulse length at FWHM. The compressor is shown
in Fig. 8.
Since I was not able to cause damage at the quick tests with this system the
setup was moved to another long-cavity laser with even lower repetition rate and
approximately two times higher pulse energy as described in the next section.
3.6 MHz Repetition Rate Oscillator The third laser of the group is a Ti:S
oscillator with 80 m long cavity. This laser has been working for years so my task
19
Figure 8: The compressor after the laser oscillator (a) and the compressor gratings
enlarged (b).
Figure 9: The spectrum of the 3.6 MHz oscillator.
was only to perform the LIDT measurements. First I made a quick test whether
the peak fluence available is high enough to cause damage. The lower repetition
rate leads to a higher peak fluence. The output power with short cavity, used for
proper setting of the laser head, is more then 1.2 W, with long cavity the CW
power is 520 mW, and the mode locked power is 680 mW. This is all achieved with
10.2 W pump power. The oscillator setup was shown in Fig. 6 at above paragraph
of this section. M1, M2, M6 and M9 mirrors are curved with radii of curvature
RM1 = 10 cm, RM2 = 15 cm, RM6 = 16 m, RM9 = 80 cm respectively, the others
are flat. P1 and P2 Brewster prisms are for fine-tuning intracavity dispersion.
The emission spectrum depends on various parameters, such as on the beam
position on the SESAM and on the fine tuning of the laser head, especially on the
stability zone. The pulse was compressed by a double prism pair compressor[29].
With best spectrum, shown in Fig. 9, 87 fs pulse length could be reached. This was
the best achievable pulse length fluctuating between 82-93 fs depending on the laser
condition. The measurements were performed at these pulse length.
20
The laser parameters at the damage workstation do not differ significantly from
the above presented. To achieve tight focusing a lens with 11 mm focal length was
built into the setup. Medium and loose focusing geometries are not possible in this
case as they do not deliver high enough focused intensity for damage. The mea-
surement of the focal spot diameter was the same method as described in Sec. 2.2.1
above. The measured values are 8.42 ± 0.22 µm and 7.92 ± 0.19 µm for the x and
y directions, respectively.
2.3 Measurement Setup
In Fig. 10(a) and 10(b) a scheme and a photograph is shown respectively of the
medium and loose focusing measurement setup. The laser beam power is 0.5 W at
the work station powered by the LEGEND amplifier. The power is decreased by
a wheel absorption filter (WF). A shutter (SH) is built in the way of the beam to
enable single shot and repetition rate dependent measurements. The power reaching
the sample may be monitored with a photodiode (PD1). The beam is focused by
a f=200 mm (L) or a f=750 mm (L’) lens on the sample which is fixed on an x-y-z
translation stage (TS).
There are two real-time monitoring systems shown in Fig. 10(a). One shown in
the center is a stereo microscope built into the setup. A CCD camera is attached
to one of the oculars and the illumination of the sample is performed through the
(a) (b)
Figure 10: The schematic draw (a) and photograph (b) of the workstation. SH:
shutter, WF: wheel density filter, PD1: photo diode, L’: f=750 mm lens, L: f=200 mm
lens, BS: beam splitter (R=20%, T=80%), TS: translation stage, IR-CCD: thermal
camera.
21
other ocular. For measuring dielectric elements, a back illumination of the sample
proved to be more usable. Filtering the IR scatter of the sample the damage is
visible certainly on the CCD’s picture. The other on the left center is a thermal
camera (IR-CCD) with which the heating of the sample can also be visualized.
The setup used for the tight focusing measurements differs slightly from the one
used at loose focus. Due to the shortness of the focal length the lens had to be
put between the sample and the stereo microscope. So the microscope and the light
source had to be shifted and the beam could be perpendicular to the sample. This
setup is better than the previous one because setup could be kept unchanged after
changing the focusing lens. This setup was built on a breadboard, so it is portable
and all of the necessary elements can be handled easily.
2.4 Sample Optics Tested
Mirrors The most commonly and widely used optical elements in laser construc-
tion are mirrors. They play role in beam steering and focusing after amplifiers.
Chirped mirrors may be used in pulse compression systems as well with continu-
ously increasing pulse energy. There are many materials to deal with these tasks
and it is important to know the damage threshold for applying the proper mirror
in each case. Therefore I tested metallic and dielectric mirrors as well. A silver
and a high reflector mirror centered at 800 nm was manufactured by Optilab Ltd.
I will refer to these mirrors as Ag and HR800 mirrors respectively. The high reflec-
tor mirror is coated with a dielectric layer structure as described further on. The
dielectric layer stack is a TiO2-SiO2 layer pair repeated 24 times which is a (LH)24
stack, where L denotes the SiO2 (n=1.44) low index and H the TiO2 (n=2.3) high
index layer respectively. The whole stack is 5421 nm thick since every layer is a λ/4
layer at λ = 800 nm. Commercial mirrors supplied by Thorlabs were tested as well,
the samples used are summarized in Table 3. They can provide a comparison for
800 nm high reflectors even though they are not optimized for femtosecond appli-
cation as their group delay dispersion is not controlled, only their reflectivity. The
Thorlabs protected metal mirrors all have a protecting overcoat which may be, in the
most common case, an approximately 100 nm thick SiO2 layer. Unfortunately the
manufacturer does not provide with precise information on the overcoat thickness.
Gratings Since gratings are very important parts of amplified laser systems, espe-
cially in pulse compressors and amplifiers, it is important to investigate the damage
22
Mirror Material Protection Coating Design wavelength
HR800 mirror TiO2-SiO2 - 800 nm
Ag mirror Ag ∼100 nm SiO2 400 nm - 2 µm
BB05-E02 Unknown dielectric - 400 - 750 nm
BB05-E03 Unknown dielectric - 750 - 1100 nm
ME1-G01 Protected Al 450 nm - 20 µm
PF05-03-P01 Protected Ag ∼100 nm SiO2 450 nm - 2 µm
PF05-03-M01 Protected Au ∼100 nm SiO2 800 nm - 20 µm
Table 3: The used mirrors and their main properties.
threshold for these type of optical elements. As a first rough proof-of-principle test
I measured three commercial gratings with different groove densities, two with loose
focusing and one with tight focusing.
The gratings are not optimized for femtosecond pulse compression. The goal
of the study on these test pieces was to see whether a dielectric λ/4 overcoating
structure can increase their damage threshold significantly without compromising
diffraction efficiency. All of them are ruled gratings with Al reflective overcoat
provided by the manufacturer. Further on each one had a dielectric layer overcoated
half with three pairs of λ/4 layers of Si02 and TiO2. This leads to a (LH)3 layer,
what corresponds to a 677 nm overcoating thickness. The overcoating (performed
by Optilab Ltd.) of the gratings is shown in Fig. 11. The diffraction efficiency is not
influenced significantly at 800 nm what can be observed in Table 4. It can be seen
that at the GR25-0610 and GR25-1210 gratings the diffraction efficiency loss due to
the overlayers is approximately 10%, and at the third an efficiency increase can be
observed at approximately 20% due to the complexity of the hybrid structure not
particularly optimized for efficiency increase. Therefore, the hybrid metal-dielectric
grating structure can be efficiently compared to the pure metal grating structure in
LIDT measurements.
23
(a) GR25-0310 (b) GR25-0610 (c) GR25-1210
Figure 11: The three Thorlabs gratings with metal coated (M) and dielectric coated
(D) halves.
Grating d(µm) αblaze ηmetal(%) ηhybrid(%)
Thorlabs GR25-0310 3.3 8◦36’ 52.5 65.0
Thorlabs GR25-0610 1.6 17◦27’ 66.2 61.5
Thorlabs GR25-1210 0.83 36◦52’ 23.0 20.5
Table 4: The diffraction efficiency of the gratings used at 800 nm, where d, αblaze,
ηmetal and ηhybrid is the grating constant, the blaze angle, the first order diffraction
efficiency without and with overlayer respectively.
24
3 Results
There where four types of measurements performed during my work. First loose
and medium focus measurements were taken with the 1 kHz repetition rate laser
described in Sec. 2.2.1 using a 750 mm and a 200 mm focal length. These will be
called loose and medium focusing, respecitvely. The second series was measured
with the 3.6 MHz repetition rate laser described in Sec. 2.2.2 with tight focus using
a 11 mm focal length lens. The third series was taken again at the 1 kHz repetition
rate laser with tight focus with 35 mm focal length to get comparable results with
measurements of the 3.6 MHz repetition rate laser since in this case focal spot sized
were exactly the same as with the 3.6 MHz measurements. The loose, medium
and tight focusing corresponds to 160 µm, 20 µm and 9 µm focal spot diameter
Sample
Measurement by focusing
MHz kHz
tight tight medium loose
Borosilicate glass ✓
HR800 mirror, Optilab Ltd. ✓ ✓ ✓
Ag mirror, Optilab Ltd. ✓
BB05-E02 Broadband diel. mirror ✓
BB05-E03 Broadband diel. mirror ✓
ME1-G01 Prot. Al mirror ✓ ✓ ✓ ✓✓
PF05-03-P01 Prot. Ag mirror ✓ ✓
PF05-03-M01 Prot. Au mirror ✓ ✓
Evap. GR25-0310 ✓
Not evap. GR25-0310 ✓
Evap. GR25-0610 ✓
Not evap. GR25-0610 ✓
Evap. GR25-1210 ✓ ✓
Not evap. GR25-1210 ✓ ✓
Table 5: Summary of the samples tested in various focusing geometries.
25
respectively as shown in Table 2 of Sec. 2.2.1. Not all of the samples presented in
Sec. 2.4 were measured in all cases and in addition a borosilicate glass was measured
with medium focus. This is summarized in Table 5.
All measurements were taken with the method described in Sec. 2.1 and a damage
occasion was detected using a stereo microscope with a CCD as presented on the
setup in Sec. 2.3, since this proved to be the best solution for real time damage
detection. The microscope is also needed for positioning the beam on the sample.
Also the scattered light can be observed while damage occurs and after shuttering
the beam the damaged spot can be seen on the CCD. Therefore I used the microscope
with the CCD for all measurements. In each case the average power was measured
and rendered to the damage probabilities. The peak fluence was calculated according
to Eq. (1). For the peak fluence calculation at the different measurements the spot
size given in Sec. 2.2.1 and Sec. 2.2.2 was used for the 1 kHz and 3.6 MHz lasers
respectively. Results are presented further on sorted by importance.
3.1 Damage Thresholds of Different Optical Elements
3.1.1 Damage Thresholds of Femtosecond Beam Steering Mirrors
The four samples measured at the kHz laser with medium focus as shown in Table 5
are a borosilicate glass, a dielectric (HR800) and Ag mirror by Optilab Ltd. and a
Thorlabs Prot. Al mirror. The damaged exposure sites are shown in Fig. 12. The
highest LIDT was demonstrated by the borosilicate glass with 3.72 J/cm2 (shown
in Fig. 2 in Sec. 2.1). This is followed by the Ag mirror with 1.29 J/cm2. The third
is the HR800 mirror with 0.67 J/cm2 and the last is the Al mirror with 0.20 J/cm2.
With the knowledge of the band structure difference between metals and di-
electrics it is surprising that the LIDT of the Ag mirror is higher than that of the
HR800 mirror. Although this is consistent with earlier studies[5]. The band struc-
ture of metals allow easy excitation which should lead to a low LIDT. As all mirrors
are coated with a protective coating with unknown thickness (and material) I do not
measure the correct LIDT of the pure metal mirror only of the metal-dielectric struc-
ture. This is a very probable reason of the results. Due to the difference between
the methods and the applied laser parameters the results can only be compared
with earlier studies qualitatively. I could not find other publications comparing the
same or similar samples except the earlier cited Bachelor Thesis of von Conta[5].
Martin et al. measured Al as well and presented result of LIDT in the same order of
26
Figure 12: Damage probabilities of Al, Ag and HR800 mirrors with f=200 mm
focusing lens.
magnitude at various pulse numbers during S-on-12 tests[30]. Moreover, comparable
measurements can only be done between samples of the same manufacturer as the
coatings can be different and LIDT of the same mirror types but made by different
manufacturers may differ. A possible reason of the lower LIDT of the Al mirror
compared to the Ag mirror can be sought in the electron configuration difference of
the two materials. The Al has three electrons on the 3s and 3p orbitals in contrary
with the only one electron on the 5s orbital of Ag. Therefore the ionization energy
of Al is lower than the ionization energy of Ag and so the electrons can be excited
easier in Al and the energy transferred from the radiation gives greater part to the
electrons the kinetic energy of which leads to the avalanche ionization effect with
higher possibility.
3.1.2 Damage Threshold of Gratings
There were three gratings tested. All of them has a metal (Al) reflective coating on
the whole surface. One half of each gratings is evaporated with a dielectric overcoat
as described in detail in Sec. 2.4. The evaporated coating is a (LH)3 coating on top
of the metal coating as described above. The exposure sites of the gratings can be
seen in Fig. 13 for the two gratings participating in the ”loose kHz” measurement
and in Fig. 15(c) for the grating participating in the ”tight MHz” measurement. It
can be seen in these figures that the LIDT of the evaporated surfaces are higher as
the metal coated surfaces, as expected. To highlight this I summarized the LIDT
2For details see Sec.2.1.
27
Figure 13: Damage probabilities of different Thorlabs gratings with and without
dielectric layer with f=750 mm focusing lens (”loose kHz” measurements).
MeasurementDamage threshold (J/cm2)
Impr. factor
Evap. Not Evap.
Thorlabs GR25-0310 ”loose kHz” 0.084 0.032 2.63
Thorlabs GR25-0610 ”loose kHz” 0.16 0.06 2.67
Thorlabs GR25-1210 ”tight kHz” 0.56 0.28 2.00
Table 6: LIDT peak fluence values for the measured gratings with the metal- and
dielectric coated half and the improvement factor due to the dielectric overcoat.
of the gratings in Table 6. In most cases an improvement of more than a factor
of 2 was measured in the LIDT of the evaporated part over the metal coated part.
The diffraction efficiency is not influenced significantly by the evaporation of the
protective coating as shown in Sec. 2.4.
The significant improvement in LIDT for the hybrid gratings is clearly demon-
strated by these measurements. Since the high reflectivity (or more precisely, high
diffraction efficiency) effect is distributed over a number of layers in this case, such
high field strengths can not be created as in the case of the pure metal gratings.
This explains the improved damage thresholds. The samples were not produced for
800 nm pulse compression purposes. For this purpose it is rather gold coated holo-
graphic gratings that are used. However, my samples give a good approximation
on how much LIDT improvement could be achieved with a hybrid gold-dielectric
28
Figure 14: Damage probabilities of Thorlabs broadband mirrors with f=750 mm
focusing lens.
holographic grating. It is an interesting challenge for the future to find an optimum
in the layer number to increase LIDT and diffraction efficiency at the same time.
3.1.3 Damage Threshold of Broadband Mirrors
In Sec. 2.4 the Thorlabs broadband mirrors are presented. Even though these sam-
ples are not suitable for femtosecond pulse steering, they can provide a good com-
parison with standard 800 nm high reflectors as their reflectivity at the target wave-
length is high, therefore light is not absorbed or transmitted. Fig. 14 shows that
especially broadband mirrors LIDT is higher than the other designed for visible-NIR
light. The measured LIDT values are 0.148 J/cm2 and 0.074 J/cm2 for the BB05-
E03 IR mirror (high reflector for 750-1100 nm) and for the BB05-E02 visible-NIR
mirror (high reflector for 400-750 nm) respectively. This is also expected due to the
specifications of the mirrors.
High reflectors for the target (800 nm) wavelength will allow the damaging beam
to penetrate into the multilayer stack only up to a certain depth. This is not the case
for the BB05-E02 mirror any more as some spectral components of the damaging
beam can even be transmitted. This means a more complex electric field distribution
within the mirror structure and thus, damage has a higher probability.
3.2 Focal Spot Size Dependence of Damage
The aim of these measurement was to compare LIDT at different focal spot sizes of
the damaging beam. As described in Sec. 1.2.2 there is a theoretical model for the
spot size dependence of the damage threshold.
29
As shown in Table 5 the Optilab HR800 and the Thorlabs Al mirrors were
measured with the 1 kHz laser at two different focusing geometries. As at the mea-
surements of the tight focus the pulse length differs, one can only give a qualitative
prediction spot size dependence of the damage threshold. At the tight focus mea-
surement the pulse length was 82 fs in contrast with the medium or loose focus where
it was 35 fs. As described in Sec. 1.2.2 decreasing the spot size leads to an increase
in the LIDT. Therefore the predicted LIDT at loose focusing has to be higher as at
medium focusing.
As also presented in Sec. 1.2.2 there is a drop in LIDT below 100 fs pulse length.
This indicates an increasing LIDT at the transition from 35 fs to 82 fs which cor-
responds to the loose/medium and tight focus measurements respectively. As both
of pulse length increase and spot size decrease lead to increase in LIDT the LIDT
measured at tight focus is predicted to be the highest.
In Table 7 the LIDT peak fluence values are summarized for the loose, medium
and tight focus measurements on the kHz repetition rate laser. It can be seen that
the Al mirror behaves as predicted as the LIDT increases in strict monotonicity
from loose to tight focus. Looking at the total improvement factor of the Al it
has to be considered that the pulse length at the loose focusing geometry was 35 fs
(τl = 35 fs) in contrast to the tight focusing geometry, where it was 82 fs (τt = 82 fs).
A total improvement factor of six seems high at first sight compared to the former
published results where a factor of two[19] and a factor of three[22] can be found.
However, if calculating with the τ12 scaling law of LIDT and divide and multiply the
tight focus result with√τt and
√τl respectively we get 0.33 J/cm2 which leads to a
scaling factor of four. It has to be noted that the τ12 scaling law underestimates the
LIDT in the subpicosecond region[6] and there is a breakdown in the LIDT under
100 fs[10]. Therefore the difference between the pulse length plays a significant
SampleDamage threshold (J/cm2)
loose medium tight
ME1-G01 Prot. Al mirror 0.083; 0.075 0.20 0.5
HR800 mirror, Optilab Ltd. - 0.67 0.4
Table 7: LIDT peak fluence values for the measured samples at different spot size
on the Thorlabs Al and the HR800 mirrors.
30
role in the improvement factor and my results can be considered as satisfactory.
On the other hand, the HR800 mirror does not correspond to the predictions. A
possible reason is that the two samples used in the measurement were different in
the optimal angle of incidence. The one measured at medium focus was optimized
for 45 degrees incidence and the other used at tight focus was optimized for normal
incidence. It is known that mirrors from different coating charges can have different
damage thresholds due to varying chamber conditions, cleanliness etc. In addition
(and probably this is the largest effect), the values given carry a significant error
which I estimate to be 15% discussed in detail in Sec. 3.4. These effects together
can explain the observed differences in the damage thresholds, therefore the latter
measurements on the high reflectors can not be considered as conclusive and will
have to be repeated.
3.3 Repetition Rate Dependence of Damage
My aim of the tight focusing measurements was to compare LIDT induced by 1 kHz
and 3.6 MHz repetition rate lasers. Since the pulse energy of the high repetition rate
oscillator only allows for damaging at very tight focusing conditions with a sub-10-
micron focal spot, I had to perform similar measurements with the kHz amplifier too.
There were many effects measured and published as shown in Sec. 1.2 but there was
no information about LIDT measured by kHz-MHz repetition rates with the same
parameters. The prediction was that at higher repetition rate the LIDT decreases
since the sample has less time to ”relax”, the possible heating effects’ relaxation
time may be longer than the time between two pulses in the MHz region but shorter
than or much comparable to the time between two pulses in the kHz region. In the
literature for Hz-kHz comparison we can find decreasing[20] and comparable (almost
equal)[17, 19] results as well.
Because one of the laser was an amplified Ti:S laser system (Sec. 2.2.1) and the
other was a long cavity Ti:S laser (Sec. 2.2.2) it was a quite difficult task to achieve
the same parameters. The most important parameters to match were the pulse
length, the focal spot size and the beam quality. Both lasers are operating at 800 nm
wavelength. Due to the more exact, precise and reproducible adjustment of the
amplified laser system I tried to achieve the best pulse on the long cavity oscillator
and after that I adjusted the amplified laser system to match the conditions. The
amplified laser system’s pulse length can be easily adjusted with the amplifier’s
compressor grating to match the typical 80-90 fs pulse length of the MHz oscillator
31
SamplePeak Fluence (J/cm2)
PfkHz
PfMHz
1 kHz 3.6 MHz
Not evaporated grating GR25-1210 0.28 0.031 9.03
Evaporated grating GR25-1210 0.56 0.043 13.02
Thor. Prot. Ag mirror: PF05-03-P01 1.26 0.133 9.47
Thor. Prot. Au mirror: PF05-03-M01 1.20 0.095 12.63
Thor. Prot. Al mirror: ME1-G01 0.52 0.024 21.67
HR800 mirror, Optilab Ltd. 0.42 0.102 4.12
Table 8: LIDT peak fluence the values for the measured samples at the kHz and
MHz lasers, and its ratio.
so this seemed to be a proper solution. I chose a 11 mm lens, with which I could
cause damage during the quick tests, which led to a spot size of 8.42± 0.22 µm and
7.92± 0.19 µm for the x and y direction respectively as described in Sec. 2.2.2. Due
to the different beam diameter of the two lasers I had to try lenses with different
focal length to ensure the same spot size at the amplified laser system. A 35 mm lens
was the best solution even in spot size and in focusing properties. So the achieved
focal spot size at the amplified laser system was 8.95± 0.23 µm and 9.04± 0.21 µm
for the x and y direction respectively as described in Sec. 2.2.1. This approximately
1 µm difference does not influence the LIDT significantly[19, 21].
I measured five samples as shown by Table 5. One grating, with both pure
metal and dielectric overcoated sides, one protected gold, protected aluminum and
protected silver mirror as described in Sec. 2.4. Further on I measured a 800 nm
high reflector mirror made by Optilab Ltd. also presented in Sec. 2.4. The damage
probability results on the mirrors with the 1 kHz laser and the 3.6 MHz laser and
the grating with both lasers are shown in Fig. 15(a), 15(b) and 15(c) respectively.
The LIDT values are summarized in Table 8. In the last column on the ratio
of the kHz and MHz damage thresholds can be seen. Except for the HR800 mirror
all ratios are between 9 and 22 with remarkable stablity irrespective of the sample
type. The approximately x10 scaling factor is noticeable comparing Fig. 15(a) and
15(b) as well. One possible reason for the smaller scaling factor of the HR800 mirror
may be the lower heat conduction ability thus heating effects have longer relaxation
time than time between two pulses at both leasers. The damaging probability of
32
(a) (b)
(c)
Figure 15: Damage probabilities of different samples. Prot. Au, prot. Ag, prot. Al
and HR800 mirrors with the kHz (a) and the MHz laser system (b). Grating with
both kHz and MHz laser system (c).
the grating is plotted with a logarithmic scale on the x axis. This highlights the
difference between the two measurement as the MHz results are in the 0.02-0.1 and
the kHz results are in the 0.2-1 region as observable in Fig. 15(c). The origin of
such a huge difference between kHz and MHz damage thresholds need to be inves-
tigated further on to identify potentially different damage mechanisms (including,
for example, thermally assisted femtosecond damage). However these measurements
represent a first step to investigate an important new phenomenon. The low damage
threshold at high repetition rate has to be taken into account in the construction
33
of some high intensity fiber lasers delivering femtosecond pulses at MHz repetition
rates.
3.4 Measurement Errors
All measurements presented above have errors due to measurement inaccuracies,
laser instabilities and statistical error.
In all cases measurement inaccuracies of the power, the pulse length, the focal
spot size (given by the magnification and/or the beam profiler camera evaluation
software) are estimated to be less than 1%. The laser instability, mostly appearing in
the power instability, caused error higher than the measurement inaccuracies. These
errors were evaluated to account for a total 4-7% error in the measured damage
threshold values.
Above all errors the highest corresponds to the statistical error observed in the
measurement procedure. Due to the properties of statistical errors it is very hard
to evaluate precisely. This type of error originates from the finite numbers and size
of the damage exposure sites and the statistical distribution of surface and bulk
defects on the mirror. Since the damage fluence depends strong on whether the
beam hits a crystal defect or not the results have great statistical fluctuation. This
can be decreased by measuring many samples with the same method or increase the
measurement points of the sample. I estimate the statistical error to be around 15%
according to experiences after a large number of tests.
3.5 Alternative Real Time and Offline Diagnostic Techniques
3.5.1 Thermal Camera
An alternative, useful and not typically used real time diagnostic technique is a
thermal camera with which the thermally assisted femtosecond damage processes
can be investigated. In spite of the fact that heating effects are not expected in
the femtosecond region with kHz repetition rate, upon measuring dielectric samples
the camera gives a nice image of the heating of the sample. In Fig. 16(a). the
evaluation software can be seen with an exposure of a HR800 mirror. The maximum
temperature was nearly 70 degrees. The camera does not work properly with metal
mirrors due to the fact that metal has better heat conductivity and reflects thermal
rays as well. So the heat of the environment is seen by the camera with a very little
heating point as shown in Fig. 16(b).
34
(a) (b)
Figure 16: Thermal camera exposure evaluation on HR800 (a) and Al mirror (b).
The heat camera diagnostics will enable testing damage mechanisms and differ-
ences between kHz and MHz repetition rates in the future. It will help to investigate
the assumption of thermally assisted femtosecond damage at MHz repetition rate.
3.5.2 ZyGO Interferometer
Offline diagnostics can be made by a ZyGO interferometer available in the laboratory
which is a high resolution microscope with white-light interferometric objectives
resulting in a depth resolution of down to 0.1 nm. The sample can be scanned
in z direction giving proper information about the characteristic of the damage.
Two dimensional, a lineout and a three dimensional image made by the ZyGO
interferometer is shown in Fig. 17(a), 17(b) and 17(c) respectively.
It is known that the different pulse length leads to different shaped damage
spots[6, 31] due to different damage mechanisms[32]. Different peak fluence at the
same pulse length gives different sites as well[23]. Therefore it seemed to be interest-
ing whether there are differences between the kHz and MHz laser caused exposure
sites. I took the protected gold mirror, hence I could determine precisely the dam-
age sites on the surface, and scanned the sample with the ZyGO interferometer. I
found that there are similar and different damage sites as well for the two lasers.
The pictures taken by the ZyGO are shown in Fig. 18. Both the kHz and the MHz
laser caused damage sites with bumps to their edges and fey hundreds nm deep
craters sites. Only the kHz laser caused small and very shallow sites with a depth
of approximately 15 nm and only the MHz laser caused sharp and very deep sites
35
(a) (b)
(c)
Figure 17: ZyGO based diagnostic technique shown on Al mirror’s crater: ZyGO
2D image (a), lineout of the 2D image (b), 3D image (c).
with a depth of approximately 2 µm. The mechanisms which correspond to deep
and shallow crater sites of the same laser needs further investigations.
36
(a)kHzbumps3D
profile
(b)kHzbumps1D
profile
(c)MHzbumps3D
profile
(d)MHzbumps1D
profile
(e)kHzshallow
2D
profile
(f)kHzshallow
1Dprofile
(g)MHzshallow
2Dprofile
(h)MHzshallow
1Dprofile
(i)kHzveryshallow
2Dprofile
(j)kHzveryshallow
1Dprofile
(k)MHzverydeep2D
profile
(l)MHzverydeep1D
profile
Figure
18:Sim
ilar
(a)-(h)an
ddifferentdamag
essites(i)-(l)of1kHz(left)
and3.6
MHz(right)
laseron
aThor.
Prot.
Aumirror:
PF05-03-M01
sample.
37
4 Conclusion and Future Plans
4.1 Conclusion
The optical damage threshold of mirrors and gratings play an important role in
laser system manufacturing and development, therefore it is essential to know the
LIDT of the elements used. However, in spite of the abundance of nanosecond and
picosecond data, less information is available for femtosecond damage threshold.
For this reason I made several femtosecond LIDT measurements on typically used
ultrafast optical elements as my Master Thesis work and took conclusions to be
summarized here.
During my master Thesis work, first I acquired useful skills in Ti:S laser sys-
tems, especially in adjusting the laser head and the oscillator, in building and ad-
justing pulse compressors (containing grating pairs and double prism pairs) and in
using femtosecond diagnostic devices such as spectrometers, autocorrelators, beam
profiler, photodiodes, etc. I built a portable LIDT measurement setup and took
measurements on different samples with two different laser systems based on ISO
standards and other consistent methods. I measured and discussed the LIDT of some
gratings and mirrors as well. The results, where comparable, were well matching
the earlier ones found in literature. I showed that even a 3-pair dielectric multi-
layer overcoating on a metal grating can significantly increase its damage threshold
without affecting its diffraction efficiency. For the first time to my knowledge, I also
compared femtosecond damage thresholds with kHz and MHz repetition rates and
found a remarkable order-of-magnitude difference the origin of which requires further
investigation. I investigated practical real time and offline diagnostic methods which
can be applied during LIDT measurements. In addition, I also compared damage
thresholds with different focal spot sizes in tight and loose focusing geometries.
38
4.2 Future Plans
We plan to write an article on the results of these measurements mainly focusing
on the striking differences between the kHz and MHz damage threshold values.
A further task is to devise a semi-automatic detection system with a quantitatively
measurable threshold indicating the onset of damage (e.g. using a simple photodiode
to detect scattered light from the damage sites) and to build a Schlieren detection
setup using automatic image processing and evaluation. With these tools at hand, a
large number of optical components can be tested for ultrashort-pulse femtosecond
damage and even online damage monitoring methods can be devised to enable safe
laser operation at large-scale facilities.
Acknowledgments
I would like to acknowledge my supervisor Peter Dombi, who made possible all
these measurements, gave me a great confidence and guidelines, reacted quickly to
my questions, even on holidays in the last days and encouraged me with his manner.
I have to thank also Lenard Vamos’ and Peter Racz’s practical advices given
me during the LIDT measurements and laser adjustment. I also thank to Daniel
Oszetzky who has helped me taking the ZyGO images.
A very special acknowledgment goes to my parents Tibor Nagy and Marianna
Nagyne Ficza, who believed in me all the time and accepted that I wrote the main
of my Thesis during the feast days of the birth our Lord, Jesus Christ.
39
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