A state-of-the-art Titanium Sapphire laser system Assignment and Demonstration in Laser physics VT-2007 Introduction This assignment and demonstration will focus on the so called "kilohertz" laser system. This system is part of the Lund Laser Center and is used for ultrafast physics research. The kHz laser produces femtosecond laser pulses with a duration of about 35 fs (1fs =10-15 s) and an energy of 1.6 mJ at a central wavelength of 800 nm (infra red). The kHz system comprises four parts. An oscillator that produces 15 fs pulses in the IR, a stretcher that streches the pulses to 180 ps, an amplifier stage that increases the pulses energy up 1.6 mJ and a compressor that compresses the pulses to 35 fs. Introduction to femtosecond lasers Pulsed lasers are powerful tools in many research areas and in the industry.Since the very first days of the laser, there has been a quest to achieve shorter and shorter laser pulses. Light pulses shorter than 100 fs were observed for the first time in 1981; pulses of 6 fs were obtained by a group at Bell Laboratories in 1987. These ultra short pulses are of great interest for many applications. - In the temporal domain: fs light pulses are equivalent to a super-stroboscope and enable us to look at ultrafast phenomena. For instance, one can observe the first steps of chemical reactions. - In nonlinear optics: the energy is released during the very short duration of the pulses. Very high peak powers (up to Petawatts) can be reached using short pulses. The generation of ultrashort pulses implies the amplification of a broad frequency spectrum. The time-frequency uncertainty relation gives t a with a almost equal to 1 (depending on the temporal profile chosen). From that relation we can see that to a small t corresponds to a large frequency spectra . This important relation will have many consequences on the choice of the different parts used to build the laser. (The amplification media should amplify a broad frequency spectrum, the mirrors must be broadband, etc.) Titanium sapphire has an energy level diagram, which is typical for solid laser materials (four level lasers). The unique property of this material is a broad absorption band, which can be pumped by fixed-frequency lasers and a wide lower laser level. The bandwidth over which laser can be obtained is wide enough to allow for 3 fs long pulses. The absorption band has its peak at around 500 nm and the emission spectrum is peaked around 800 nm. Since the absorption and emission bands are well separated, losses due to reabsorption of the laser radiation are minimized. 2 Relaxation 3 Pump Lasing 500 nm 800 nm 4 Relaxation 1 Two conditions determine the frequency components available to build up a wide frequency spectrum. The first is the (approximately) resonance condition for a standing wave: n=L or expressed in frequency =nc/2L where L is the length of the cavity. The second one is the spectral bandwidth of the laser. The laser bandwidth is mainly limited by the gain profile of the amplifying medium. Passive Kerr lens mode locking (Svelto 344- 345) In a cavity consisting only of a gain medium, end mirror and output coupling mirror, all modes are oscillating in random phase. By introducing additional components in the cavity, it is possible to phase-lock these modes to each other. Depending on the method by which the phases are locked one refers to either active or passive modelocking. When the phase difference between the modes is constant, the modes are oscillating in phase and interfere constructively. If we add the E-fields from the standing modes, the sum as function of time will be a short pulse propagating back and forth in the cavity. At low intensities, the refractive index (for a given wavelength) is constant. At high intensities, the refractive index vary by n=n1+n2I. Due to the fact that the laser has a spatial intensity variation, the refractive index will be larger in the center of the beam, where the intensity is the highest. This makes the crystal behave like a lens (referred to as a Kerr lens). A Kerr lens can be used to create losses for CW radiation, whereas the losses for high intensity pulses obtained by mode-locking are minimal. Thus, a Kerr lens can be used for passive mode-locking. It is common that Kerr lensing in the amplifying medium is used. The amplifying medium is used both to obtain gain and to obtain modelocking. Titanium sapphire crystal Aperture Low intensities large losses Laser beam x n=n1+n2I I High intensity small losses The beams spatial profile creates the "Kerr lens" Dispersion compensation (Svelto 347-355) Due to dispersion, different frequency components propagate with different velocities in all materials. In solids, glass, crystals etc., the effect can be significant. In nearly all materials, shorter wavelengths propagate slower than longer wavelengths. This phenomenon is known as positive group velocity dispersion (GVD). The consequence is that a short pulse consisting of many wavelengths is stretched in time. In order to compensate this effect, negative group velocity dispersion is needed. Negative GVD means that short wavelengths propagate more rapidly than longer wavelengths. This can be obtained with the prism arrangement shown below. R B Amplification of the laser light As mentioned previously, the oscillator of the kHz laser system delivers laser light pulses of 15 fs with an energy of 2 nJ. This power is not enough for the applications we are aiming at. The laser pulses are then amplified to 3 mJ, using the Chirped Pulse Amplification technique (1989). The figure below summarizes the main steps of the amplification. 15 fs ; 89 MHz from the oscillator Pockel’s cell Pulsed YLF laser Stretching of pulses 180 ps ; 89 MHz Grating stretcher Selection of a First pulse amplification 180 ps; 1kHz Second amplification 180 ps ; 1kHz Q-switched Compression Laser YLF Grating compressor 35 fs ; 1kHz Pulse stretching If we directly amplify the short pulses from the oscillator, we will reach very high peak intensities. The high intensities would damage the amplifier medium. In order to decrease the peak intensities we induce a varying phase (a chirp) on the different spectral components of the pulse, leading to a stretching of the pulse duration. In the kHz system a grating stretcher is used. The different frequencies will not have the same optical path length, and the pulses get as long as 180 ps. Amplification stage The stretched pulses (180 ps) are sent into the first amplification stage. This is performed by using Pockel’s cells and polarizers. The first amplification step is done by a regenerative amplifier cavity, with two concave mirors. The selected pulses do a few round trips before they are coupled out. The Ti:Sapphire crystal in the regenerative cavity is pumped by a frequency doubled Nd-YLF laser. The beam is then sent to two other amplification stages. In these amplifiers the pulses pass the gain medium twice (two pass amplifier). Compression After the amplification we still have long pulses. In order to achieve high power we have to recompress the pulses. To achieve that, we use a grating compressor. As in the stretcher, the different optical frequency components will not have the same path in the cavity. The compressor compensates for the chirp of the pulses and recompresses the pulses in time. We then get high intensity peaks. Measurement techniques To be able to control the pulses we need to measure and characterize our fs pulses. The only methods available on that timescale (fs) are optical. The fastest electronic detector can only detect on a ps timescale. We have to use the pulse itself to measure it. 1- Preparatory exercises 1) Calculate the average and the peak power at the output of the kHz oscillator (2nJ, 15 fs at a repetition rate of 89MHz). 2) After the grating stretcher, each pulse have a duration of 180 ps. Calculate the average and peak power of these pulses (take into account that there is a 50% loss in the grating stretcher). 3) Calculate the peak intensity in W/cm2 at the output of the amplifier (1.7 mJ, 35 fs) if the beam is focused on a target with a spot size of 1mm diameter. 4) It is often difficult to have an idea of a femtosecond. To be aware of how short it is, calculate the distance covered by the light in 1 fs. The cavity of the regenerative amplifier is approximately 3.6 m long. Calculate the time needed for the seed pulse for a round trip. To achieve optimum amplification, we have approximately 20 passes. What is the theoretical limit for the repetition rate of the amplified pulse train? (The real limit, 1 kHz repetition rate is imposed by the repetition rate of the pump laser.) 5) Assume a Gaussian shaped pulse in the time domain of 15 fs with a central wavelength λ0 of 800 nm. Determine the corresponding spectrum: - in the angular frequency domain ω0, Δω. - in the wavelength domain λ0, Δλ. If by spectral narrowing the bandwidth is reduced to half, how will the pulse duration change? Assignment 1) Mode locking The optical length of the oscillator cavity is 1,7 m. Calculate the mode spacing in the frequency domain. The bandwidth of a Ti:Sapphire crystal is 100 THz centered on ν0=375 THz , which enables generation of 3 fs pulses. The spatial extension of a fs pulse is ~10 μm. In this exercise, it is desired to have a longer pulse to be able to visualize the pulse in the cavity. We reduce the bandwidth to 10 GHz. The broadening mechanism is assumed to be mainly inhomogeneous, which implies a Gaussian line shape. The intensities of the modes in the cavity are proportional to the gain. Plot the electric field amplitude of the modes as a function of mode frequency. The cavity modes are standing waves. Plot the superposition of the cavity modes for random phases of the modes at t=0 in function of the cavity length. The Matlab command: phi=2π*rand(1,N) is useful. Make a time evolution of the superposed standing waves (choose an appropriate timescale). Under mode locked operation the phase difference between consecutive modes is constant. Plot the electric field in the cavity at time t=0 and make a time evolution. Calculate the temporal length of the pulse out of spatial extension. The time frequency dependence of a Gaussian pulse is: t 2 ln 2 Does the calculated temporal length fulfill the time frequency dependence? 2) Dispersion Titanium Sapphire is a broadband amplifier medium. We can assume that in the frequency domain we have a Gaussian spectrum: E ,0 E 0 e i ( ) 0 exp 2 The oscillator of the kHz lab delivers pulses whose spectra is centered on λ 0=800 nm and a width of Δλ=70 nm. With Matlab or any other program, retrieve the shape of the pulse in the time domain for a phase φ(ω)=0 (no phase difference between the different spectral components). When a pulse with a broadband frequency goes through a material of a length L whose refractive index n(ω) changes with ω the phase can be written as L n . That can c be written under a Taylor expansion form: 0 0 1 Each coefficient n! n 0 0 2 2 2! 2 ... 0 n n is a constant that can be obtained for a given material. 0 Modify the former program to add a phase to the spectrum. Retrieve the pulse in the time domain for several α1(ω), and α2(ω). Can you identify the changes induced by these chirp rates? Plot these results on a graph. Hint: typical order of magnitude for α1(ω) is 10-15 s, α2(ω) is 10-28s2 A typical dispersive media is a SF57 glass plate whose chirp rate is α2=2.25.10-25 s2/m. Compute the passage of a pulse (λ0=800, Δλ=70nm) through 1mm of this material. Plot the incoming and outgoing pulses on a graph and estimate their duration. A few notes about MATLAB FFT. MATLAB has an FFT routine defined as: X( k ) 1 N N x( n )e i 2 ( k 1 )( n 1 ) N (1) (here k is an index) n 1 What you want to do is E (t ) E ( )e it d (2) To go from the first to the second, we write: min (n 1)d t t min (k 1)dt and discretize (2) as: N E (k ) E (n)e itminmin imin ( k 1) dt itmin ( n 1) d i ( k 1)( n 1) dtd n 1 This implies that dtd Matlab FFT routine. 2 . Choose a reasonable t min ! Now you can use the N