Frequency comb lasers on the move to extreme wavelengths Kjeld Eikema LCVU day 17 Dec Christoph Gohle, Dominik Kandula, Tjeerd Pinkert Anne Lisa Wolf, Steven van den Berg (NMI) Wim Ubachs, Wim Hogervorst
Outline Introduction frequency comb lasers Goals First comb excitation of Ca ions in a trap First comb excitation of Helium, at 51 nm Summary & outlook
Addition of waves to pulses
Modelocked laser ~ frequency comb More than a million lasing modes can work together to form < 5fs pulses Laser resonator
Time and frequency picture frequency Int. 0 time Equivalent !!!
Frequency comb structure frequency Int. 0 R. Holzwarth et al. PRL 85, 2264 (2000), D.J. Jones et al. Science 288, 635 (2000) f n = f 0 + n. f rep f rep = c / 2L f 0 = f rep x φ CE / 2 Controlled repetition rate + Phase relationship between the pulses = Frequency comb time φ CE = /2 φ CE = 0 v g ≠ v φ
Time & frequency consequences Very precise pulse control Attosecond timing resolution revolution Reproducible phase coherent optical pulses Absolute long distance measurement Very precise frequency ruler for THz-PHz Optical frequency calibration revolution Optical atomic clocks ‘Fingerprinting’ parallel spectroscopy
Ti:Sa Frequency comb implementation LCVU 2 Ti:Sa based comb lasers 1 Fiber-based comb laser (Menlo Systems) f rep : MHz nJ pulse energy 500 – 2000 nm
Fiber frequency comb LCVU nm & nm, f rep = 250 MHz Project of Valdas Maslinskas
Measuring with frequency combs frequency Int. 0 f0f0 frfr Atomic clock f VIS-NIR comb MHz CW ultra- stable laser Precision spectroscopy Hz Counter
Goal 1: trace attosecond electron dynamics Attosecond dynamics in mK molecular ions Tryptofan complexes (Trp Ala 2 and Trp Leu 2 ) Remacle & Levine PNAS 103, 6793 (2006)
Tools for attosecond dynamics studies Powerful and precisely controlled electromagnetic waves with sub-femtosecond resolution Pump-probe via VIS-UV – XUV phase coherent pulses or via re-collision of electron wavepackets (HHG!) Cold and localized molecules: molecular ions in a trap, sympathetically cooled by atomic ions to mK temperature Many other things we probably did not think about...
Goal 2: XUV precision test of QED 1S 2S Hydrogen 2x 243 nm 1S-2S: (34) Hz Lamb shift 1S: (22) MHz M. Fischer et al., PRL 92, (2004) Uranium 91+ Lamb shift 1S = (4.6) eV 1S 1/2 2P 3/ (6) eV A. Gumberidze et al., PRL 94, (2005) Higher-order QED scales with >= Z 4
Tests in Helium and Helium+ ions HydrogenHeliumHelium+Lithium 2+ 1S 2S 243 nm 1S 2 1S2S 120 nm 1S 2S 60 nm 1S 2S 30 nm 51 nm 1S5P
Searching for a change of alpha Comparison lab UV spectra vs. IR telescope absorption lines in quasar spectra (looking back billions of years)
Direct UV frequency comb excitation Frequency comb 788 nm 2 nd Harmonic generation 394 nm tt 22 5 ns 10 5 modes 5 ns 190 MHz Time domain Frequency domain f n =f 0 + n f r f m = 2 f 0 + m f r
Ca + ions Direct frequency comb spec. of Ca + Paul trap Freq. comb 394 nm
Ions in a trap Calcium ion trap & Anne Lisa Wolf
The setup
Direct frequency comb signal of Ca +
Mode number determination for Ca times more accurate than before Corrections for light-shifts etc. included Accuracy: 0.5 MHz
Helium groundstate status Energy of He 1s 2 1 S 0 ( MHz) Theory: Drake & Yan Can. J. of Phys. 86, 45 (2008) MHz Eikema et al. PRL 71 (1993) PRA 55, 1866 (1997) Bergeson et al. PRL 80, 3475 (1998) Measurements with nanosecond duration VUV (120 nm) or XUV (58.4 nm) single pulses
HHG: High-Harmonic-Generation IR pulses – mJ levelXUV pulses – nJ level W/cm 2 lens/mirror Required for 1s 2 – 1s5p transtion: nm gas jet
Hoge-harmonische generatie Model van P. Corkum, PRL 1994
High-harmonic generation T Train of x-ray bursts Generation of 170 attosecond pulses: Lopez-Martens et al, PRL 94, (2005) ~ 5 fs
Problem: single pulse frequency chirp ‘Clean’ or ‘Fourier limited’ well defined central frequency ‘Chirped’ Unclear frequency due to amplification & harmonic conversion
Solution: two or more pulses time frequency
Direct UV frequency comb excitation Frequency comb 788 nm 2 nd Harmonic generation 394 nm tt 22 5 ns 10 5 modes 5 ns 190 MHz Time domain Frequency domain f n =f 0 + n f r f m = 2 f 0 + m f r
Direct XUV frequency comb excitation Frequency comb 773 nm Two-pulse amplifier 15 th Harmonic generation 51 nm ttt 15 7 ns 10 6 modes 10 4 modes 7 ns 150 MHz Time domain Frequency domain f n =f 0 + n f r f m =15 f 0 + m f r
Frequency comb up-conversion IR DUV frequency VUVXUVX-RAY harmonic conversion IR pulses with CE controlXUV W/cm 2 UV Xe or Ar jet
How accurate does it have to be? 51 nm ! CE ~ /100 CE ~ 0 =20 MHz T = 6.6 ns
2 identical pulses Accuracy required CE ~ /200 ! Delay 6.6 ns, accuracy ~ 10 attoseconds (10∙ s) While amplifying more than x at 10 GW/cm 2 power levels, over the full 6 mm beam diameter !
Amplification of the comb with a NOPCPA ss pp ii The good: High gain (=short path length) Broad bandwidth (non-collinear) No thermal effects Phase preserved of signal (but...) The tricky: Picosecond pump laser Synchronization < 1 ps Angle sensitivity p k p pump idler signal (2) fluorescence cone seed s k s
Setup for He spectroscopy at 51 nm regen amp. 2 mJ power amp. 2 x 200 mJ SHG sync. 7 ps osc nm comb laser ~780 nm f rep =150 MHz NOPCPA HHG 51 nm pulses, 6.6 ns apart 1s5p 1 P 1 1s 2 1 S 0 Helium 51 nm 2x 2 mJ 200 fs Relay imaging
Phase measurement setup BS 50% BS 5% NOPCPA Pump laser BS NG Oscillator PC2 PC1 G BS BS 5% D fiber Computer CCD Camera PBS
Phase accuracy between 2 pulses At the moment for pulses 6.6 ns apart: Interferometric measurement to 1/600 th of IR ! Phase flatness across the IR beam: ~ 1/200 th of IR Many tricks involved to control and measure this! Christoph Gohle Dominik Kandula
Photos of the lab
XUV comb generation and He excitation HHG Spherical grating XUV detector Krypton jet XUV Beam Monochromator slit 2 times >2 mJ, 200 fs Helium beam 90 o ! IR ionization beam
HHHG: Holey-High-Harmonic-Generation IR pulses – mJ levelXUV pulses – nJ level W/cm 2 f=50 cm
Harmonic generation double pulses In ~772nm Harm. : (nm) 7 : : : : : 51
HHG with double NOPCPA pulses 15 th harmonic in Krypton ~ 51 nm nJ pulses Fundamental at 795 nm
First helium 1s5p signal at 51 nm... comb laser repetition rate scan He-ion signal FFT
Better Helium 1s5p signal at 51 nm 150 MHz Total scan of pulse delay < 0.5 fs ! 8 attoseconds change per scan step
Photo He experiment
Xe two-pulse 125 nm excitation Short delay for mode identification, long delay for accuracy Decreasing contrast is caused by the residual 10 MHz Doppler width Best fringe position fitting result: 40 kHz Phase errors reduce to <1 MHz at longer delays 13 times better than CW/ns pulsed experiments. Zinkstok et al., PRA 73, (R) (2006)
Summary First demonstration of direct frequency comb excitation of calcium ions in a trap at UV wavelengths First XUV frequency comb excitation of helium: on route to MHz precision In preparation: Calibration He ground state, two-photon excitation etc. Sympathetic ion cooling of atomic and molecular ions Attosecond electron dynamics in biomolecules Extension of XUV combs for helium+ 51 nm