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Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA America VUV Frequency combs Ohio State University 2010 Phase-coherent synthesis of the electromagnetic spectrum

Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

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Page 1: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

Dylan Yost, Arman Cingoz, Tom Allison and Jun YeJILA, University of Colorado Boulder

Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA America

VUV Frequency combs

Ohio State University2010

Phase-coherent synthesis of the electromagnetic spectrum

Page 2: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

VUV metrology and quantum optics with frequency combs

• Precision test of fundamental physics

•Simple atoms = Tough wavelengths

•EUV atomic clocks? Shorter is better.

(1s2) 1S

(1s2s) 1S, 3S

(1s2p) 1P, 3P

(1snp) 1P, 3P

58 nm

He

Page 3: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

Motivation for VUV frequency combs

• VUV monochromator (5 meters long gets frequency resolution of 10-5).

• VUV frequency comb could offer frequency resolution of 10-9 -10-12 at VUV/XUV wavelengths.

• Cover the whole spectrum and utilize automatic calibration.

• Compact table-top source.

Page 4: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

Frequency Comb Technologyin the VUV, XUV?

• An infinite train of identical VUV pulses and arbitrary wavelengths in a compact setup.

• High harmonic generation for frequency conversion (convert 1070 nm comb to XUV).

• Power requirements for XUV comb generation: ~100 MHz repetition rate and 10 J pulse energy

>1 Kilowatt precision frequency comb

Step 1: IonizationThree step model

Step 2: Field Reversal

Step 3: Recombination

EU

r

EU

r

U

r

Page 5: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

Cavity-based coherent pulse buildup

Frequency Domain

Frequency comb

Cavity modes

Jones et al., Phys. Rev. A 69, 051803 (R) (2004)

Time Domain Jones & Ye, Opt. Lett. 27, 1848 (2002)

2

2 2π4T

4T

F

=L

=N

Cavity enhancement:

Tin

• Linear response • Preserves coherence• Power enhancement

Page 6: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

Intra-cavity HHG at 100 MHz

C. Gohle, et. al., Nature 436, 234 (2005).

R. J. Jones et. al., Phys. Rev. Lett. 94, 193201 (2005).

Page 7: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

Challenges to overcome

•Relatively low harmonic orders

•Relatively low power

•Power scaling?

•Can we maintain a linear response for the cavity?

•Brewster plate output couplers introduce linear and nonlinear dispersion

R. J. Jones et. al., Phys. Rev. Lett. 94, 193201 (2005).

C. Gohle, et. al., Nature 436, 234 (2005).

Page 8: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

Low dispersion high reflector at 1070 nm Etching adds birefringence but nearly no additional loss or dispersion fundamental nearly unaffected by subwavelength grating

Operation in XUV (50-150 nm)SiO2 fresnel reflection: ~45%Overall grating efficiency: ~10%

Diffracted Harmonics

Xenon jet

HHG

70 degree Incidence

Power Scalability!

HHG output-coupling viaa Small-Period Diffraction Grating

D. C. Yost et. al. Optics letters 33, 1099 (2008)

Page 9: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

XUV frequency combs with grating OCand Yb similariton frequency combs

Phosphor screen (Sodium salicylate)

• Yb laser offered 10 W of 1070 nm light• Power increase of nearly 104 at 60 nm• Highest HHG orders ever produced at ~100 MHz rep

rates• Power scaling greatly increased harmonic power

5th 7 9 11 13 15 17 19

10 W - 50 nW per harmonic

21

Yost, Schibli, Ye, Opt. Lett. 33, 1099 (2008)

214 nm 153nm 119 97 82 71 63 56 51 nm

Page 10: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

New Yb Fiber System

~120 fs pulses, 154 MHz repetition rate with 80 W average power

Requires record-level pulse stretch/compression rates of ~4000

Full high bandwidth control over fceo and frep

See SCALING OF YB-FIBER FREQUENCY COMBS-

Axel Ruehl

Page 11: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

Preliminary Results

• 5 kW of average intracavity power with HHG output coupler demonstrated

• ~10 times improvement in harmonic yield

• Currently limited by mirror coatings grating

• Higher damage coatings, new grating design and new cavity geometry under development

Page 12: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

Testing the high harmonic coherence

Interfere pulses n and n+1 (7th harmonic):

demonstrate a coherence length 100,000X longer than in previous work

L. Xu et al., Opt. Lett. 21, 2008 (1996).

Page 13: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

VUV Coherence Tests

Demonstrated pulse-to-pulse coherence at 7th harmonic. -Coherence time lower bound of 15 ns (20 MHz linewidth measurement limited by shot noise).

•Shows pulse to pulse coherence (frequency comb), but is not a very sensitive test of phase noise

Page 14: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

Argon Spectroscopy

5 electric dipole transitions possibly within the 13th Harm. Bandwidth (2 probable) Natural linewidths 10 – 20 MHz Comb spectroscopy should allow for absolute frequency determination at the MHz level Will be the most sensitive test of frequency comb coherence

Page 15: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

Frequency Resolved Spectroscopy

• Absolute Frequency Determination by optical lock of IR frequency comb to Iodine stabilized Nd:YAG

• Preserve coherence through HHG process by minimizing cavity lock noise

• Reduce Doppler widths to ~10 MHz and frequency resolved spectroscopy through crossed beam geometry.

Page 16: Dylan Yost, Arman Cingoz, Tom Allison and Jun Ye JILA, University of Colorado Boulder Collaboration with Axel Ruehl, Ingmar Hartl and Martin Fermann IMRA

Outlook

Thanks to: Axel Ruehl, Ingmar Hartl and Martin Fermann at IMRA America.

Ye group members past and present, especially R. Jason Jones, Thomas Schibli, Kevin Moll and Mike Thorpe